May 19 - 25, 2024: Issue 626

Our Youth page is for young people aged 13+ - if you are younger than this we have news for you in the Children's pageNews items and articles run at the top of this page. Information, local resources, events and local organisations, sports groups etc. are at the base of this page. All Previous pages for you are listed in Past Features

 

Jordan Lawler Wins 2024 World Surf League GWM Sydney Surf Pro.!: WSL Leaves North Narrabeen In A High Stoke - Tahiti Pro. Commences This Week At Venue For Paris 2024 Olympics Surfing Comp. 

Jordan Lawler being chaired by the home crowed. Photo Credit: © WSL / Matt Dunbar

The WSL roadshow has rolled into North Narrabeen and rolled out again, leaving the site of this National Surfing Reserve a little bit too quiet after 6 days in a row of spectacular surfing by some of the best athletes. There is a lingering, palpable, high stoke.

Just as happened at the Bonsoy Gold Coast Pro the week before, when icons of surfing Mick Fanning, Joel Parkinson, and Stephanie Gilmore joined Kelly Slater in a World Champ's Super Heat celebrating the best of competitive surfing, local legends were part of this iconic surf festival.

On Sunday May 12, Mother's Day, the last heat of the day saw a group of local surfing greats take over the line-up at North Narrabeen for a 40-minute spectacle to see who still rules the roost and entertain the solid Sunday crowds that lined the shore. 

Surfers included 2018 Grand Masters World Champion Rob Bain, Two-time World Champion Tom Carrol, Former CT competitor and big wave world record holder Laura Enever, two-time World Champion and North Narrabeen Boardriders Club President Damian Hardman, and CT event winner Nathan Hedge. 


Pictured: The Bonsoy Legends Heat hit the water at North Narrabeen with legends [Left to Right] Damian Hardman, Rob Bain, Laura Enever, Tom Carrol and Nathan Hedge. Credit: © WSL / Matt Dunbar

All five surfers traded waves and had their moments, but it was Laura Enever who earned the biggest highlight of the session for a long left-hander with multiple turns completed on the sand. 

However, the highlight of this year's WSL GWM Sydney Surf Pro presented by Bonsoy was witnessing North Narrabeen's own Jordan Lawler take out the event.

On Tuesday, May 14, 2024, Isabella Nichols (AUS) and Jordan Lawler (AUS) claimed victory at Stop No. 2 of the 2024 World Surf League (WSL) Challenger Series (CS). In front of a packed beach at North Narrabeen, the Aussie duo were able to overcome a massive international field to take the win in super clean two-to-three-foot surf. 

North Narrabeen local Jordan Lawler (AUS) won in front of a huge home crowd, securing the title in scenes reminiscent of those 1970's to 1980's competitions at the same site. Although this win was a replay, to some degree, of his 2019 crowning in that WSL Sydney Surf Pro at the other beach renowned for hosting professional surfing competitions on the peninsula, Manly, this ranks as the biggest result of his career. 

In 2019 Jordy competed in the Qualifying Series events. Surfers who are not currently eligible for the Championship Tour (CT) events are able to compete in a Qualifying Series (QS) of events, earning points towards qualifying for the following year's CT.

The big difference between a Challenger Series event and a Qualifier Series event (the second-tier comps) is how they allocate points. A Challenger Series event hands out more points for the global QS leaderboard that surfers aim to climb, unlike a regular QS event.

The Challenger Series is the launchpad to the elite Championship Tour, pitting established surfers fighting to stay on tour against the next generation of premium talent. Across the events, the 2024 fields of 84 men and 52 women will battle for one of the 10 men's and 5 women's coveted spots at the top level of the sport.

Having missed qualifying for the Challenger Series in 2024, Lawler came into the event as a wildcard. With low expectations on himself, he was able to cruise through the draw and claim a memorable win. 

“Honestly, the last few months have been a real rollercoaster,” Lawler said afterwards. 

“After not qualifying for the Challenger Series this year, I was honestly thinking about calling it quits, so I’m just stoked I stuck with it. I was pretty low there for a while, and I hadn’t had a good result for a while, so I’m just so stoked right now. To make it to the Championship Tour has been my goal for so long and to win an event of this size can really help with that, I just can’t believe it.” 


Jordan Lawler getting some air. Photo Credit: © WSL / Matt Dunbar

In the 35-minute Final, Lawler came up against former Championship Tour (CT) competitor Alejo Muniz (BRA) in a classic frontside versus backside battle on the North Narrabeen lefts. Muniz had been in solid touch all week but it was the local knowledge and hometown support that got Lawler an early lead. 

Jordy was then able to build momentum throughout the matchup, eventually posting a 15.75 (out of a possible 20) two-wave total, his highest of the event and enough to put Muniz in a combination situation. In the dying minutes, Muniz found a 7.20 (out of a possible 10) to break the combination but was unable to back it up, leaving Lawler to claim victory. 

“Winning at home in front of all of these familiar faces is so amazing, I’m speechless,” Lawler said. "Growing up, I looked up to so many of these surfers, and to be competing against them and getting the win is like a dream come true, especially at home. I’ve worked so hard to be here, and I’m keen to get it done this year, qualifying for the Championship Tour.”

Jordan first picked up a board at the age of 4 down at Wilson’s Promontory, and started really getting into surfing at around age 11. His first comp was through the North Narrabeen Boardriders club when 12. He graduated from Narrabeen Sports High School in 2014.

The North Narrabeen Boardriders Club, established July 26, 1964, celebrates its 60th year in 2024. A black tie event is scheduled to take place in October.

In more great news for the club this week the NSW Government has allocated $632,000 for upgrades to North Narrabeen Surf Life Saving Club under the Surf Club Facility Program, which includes the extension to the north first mooted by Council in 2023. Details here.


Isabella Nichols and Jordan Lawler- winners. Photo Credit: © WSL / Cait Miers

Jordy currently sits at spot 4 in the 2024 Men's Challenger Series rankings, one spot behind Lennox Head’s Mikey McDonagh, who won the Gold Coast Pro., Stop No. 1 of the 2024 WSL Challenger Series (CS), on May 4, and two spots ahead of fellow peninsula surfer George Pittar.

Mr. Pittar has been on a bit of a roll in past weeks.

Hailing from just down the road in Manly, George Pittar was finally back on home soil after a whirlwind few months of competition. Pittar was awarded wildcards into two Championship Tour (CT) events, putting on an incredible performance that saw him earn an equal third-place finish at the Western Australia Margaret River Pro (April 11-21, 2024), even taking down world No. 1 Griffin Colapinto (AUS) along the way. He picked up more points after gaining a wildcard entry into the Rip Curl Pro Bells Beach presented by Bonsoy (March 26-April 25).  Pittar then commenced his Challenger Series season with a solid showing and Semifinal finish on the Gold Coast and continued that form at Narrabeen, picking up  3,320 points in the GWM Sydney Surf Pro presented by Bonsoyas for his efforts. George is also working to win a full-time spot on the CT in 2025. 

“It’s amazing to be back home and competing at an event of this size whilst sleeping in my own bed and enjoying mum’s home-cooked meals,” Pittar said. “It’s amazing to see all of the world’s best lighting up the Northern Beaches. I know it means a lot to the local surfing community. 

The last month has been amazing. It’s been great to get some results and scores at the CT level and show myself I can belong there and it definitely gives me so much confidence ahead of the CS season. It’s given me incentive to qualify and compete at the CT level full-time.” 

MORE HERE

 

The Irukandji's Win Eighth Team World Championship And Two Individual Gold Medals At The 2024 ISA World Junior Surfing Championship

Team Australia; The Irukandji's - The Australian Junior Surfing Team stand on the podium after winning gold at the ISA World Junior Surfing Championships.  Photo: ISA/Pablo Jimenez


In an outstanding display of skill, determination, and sportsmanship, the Australian junior surfing team, known as 'The Irukandji's', have claimed the overall gold at the 2024 ISA World Junior Surfing Championship as well as two individual gold medals for Dane Henry (U18 men's) and Ziggy Aloha Mackenzie (U16 women's). In one of the most commanding victories in ISA competition, today's (May 13 2024 Australian time) result makes the Irukandjis the winningest team in ISA World Junior history, ending an 11-year wait since their last triumph in 2013.

Individual gold medals for Dane Henry and Ziggy Mackenzie were backed up by a silver medal for Fletcher Kelleher and copper for Milla Brown. But the performance of the entire Irukandjis team was so strong that victory was almost secured before Finals Day even began, and a heat win for Brown, backed by Willow Hardy’s performance, in Girl’s U/18 Repechage Round 9 was enough to see Australia take the Team gold medal long before the Grand Finals began.

Kate Wilcomes, the Surfing Australia National High-Performance Director, expressed the broader implications of the team's success, stating, "This win represents where Australian Junior surfing is at and the dominance we intend to continue to deliver! This team and the support staff have not only worked hard, but they have also built and embraced the Irukandji's fighting spirit. We are all so proud of each and every one of these athletes and how they have represented Australia."

In a stacked Under 18 men’s Grand Final, Dane Henry became the first Australian to win this division in 15 years. The 17-year-old led the pack with an excellent heat total of 16.8 out of a possible 20, clinching the gold medal. Close behind was fellow Australian Fletcher Kelleher, who scored an impressive 15.97 out of 20. Their strong performances triumphed over tough competition from Brazil's Rickson Falcão (14.67) and Japan's Ikko Watanabe (8.70), showcasing the depth of talent in Australian junior surfing.

Henry led the Australian charge through the entire event, with the team captain posting seven scores in the excellent range, including a perfect 10-point ride. 

Henry reflected on his achievement and the team's success, "I'm so proud of everyone in my team; it's been the best experience of my life. I couldn't have done it without my mum; she's an absolute legend, and I wouldn't be up here without her." 

Overcome with emotion, he added, "Thank you to all the coaches, everyone back at home, from the bottom of my heart this is the best thing I've ever done in my life."


Dane Henry, Team Australia / Photo: Pablo Franco

Ziggy Mackenzie’s (AUS) road to the Final was made smoother after she took a wave in her Girl’s U/16 Main Event Final with 1 second to go. Needing a 6.54, the 15-year-old grabbed a 6.57 to guarantee herself a medal. In an extremely tight final, a 6.83 from Mackenzie proved to be the high point and when her backup of a 5.93 arrived late in the heat, it was enough to seal the deal and plant her name as a World Junior Champion alongside fellow Australians Stephanie Gilmore and Tyler Wright.

Mackenzie said. “I feel like all the work that I’ve put in and all the support from the Australian team has all come together. I think everyone was so excited but so nervous at the same time coming into this event. We’ve got such a strong team and we really wanted to just push and push as hard as we can. We’re on top and I’m so stoked for the team.”

Ziggy Mackenzie showcased her talent in the Under 16 division against an international field. "I just tried to keep calm and collected. I knew we had the (team) gold already, so I kind of wanted to go out there and surf how I surf and show the world Ziggy". Mackenzie explained. 

She later expressed her elation, saying, "I'm blown away, I'm so stoked. To be here with Australia has been an insane experience and I'm so happy to have come out on top and for team Australia to have come out on top as well, everyone's stoked."


Ziggy Mackenzie, Team Australia / Photo: Sean Evans

Clancy Dawson, Surfing Australia Performance Pathway Manager, highlighted the foundation of the team’s success, stating: “What an incredible performance by our team. Our vision is to be the most dominant surfing nation, and our results in this event exemplify that goal. All medal-winning athletes came through our 'Talent Identification Program' and have been working with the Surfing Australia High Performance Team for the last four years.

This program is designed to identify the most promising juniors at the ages of 13-14 and help them not only become the world's best surfers but also the world's best people. Dominant team and individual results like these make us extremely proud of the long-term work and strategy that goes into shaping the next generation of Australian surfers. Dane Henry exemplifies the degree of innovative high-performance surfing we foster, taking that competitive edge at an ISA event to a whole new level.”

The event was not without it's controversy for the Irukandjis, particularly during the Under 18 girls' repechage. Western Australia's Willow Hardy was in the spotlight over the weekend for maintaining her composure under highly stressful circumstances. Hardy, who needed a small score of a 2.4 to advance with only 50 seconds left in the heat, was interfered with by Portugal's Erica Máximo White. Máximo attempted to push Hardy off her craft and yelled verbal abuse before trying to grab Hardy's leash (attached to both her board and her leg). Despite the interference and unsporting conduct, Hardy surfed the wave to the required score to progress. 

Coach Pete Duncan lodged a successful protest, resulting in Máximo's disqualification. Duncan remarked, "While there is a tactical element to competitive surfing, there is no place for unsporting conduct. We are incredibly proud of the way Willow remained composed in what was an uncomfortable and potentially dangerous situation." Máximo later apologized via Instagram, expressing regret to Hardy, the Australian Team, and the ISA.

Hawaiian girls account for the most gold medals in the WJSC, and Vaihiti Inso continued that tradition when she won the 11th gold medal for Hawaii. The new U/18 World Champion was proud to represent her team and her culture with the victory, but was also thrilled to display a solid show of surfing. Winning the Grand Final with an 8.50 and 8.17, largely on the strength of her powerful and stylish forehand carves on the lefts of La Bocana, her 16.67 heat total left her fellow finalists in need of near-perfection to reach her.

“I’m almost speechless,” Inso said. “Honestly my main goal was not the result but just to put on a good performance and I hope I did that. I love surfing and before there was no lefts and all of a sudden the lefts just came that way. So mahalo ke Akua for the waves and God for everything.”

After impressive performances across both U/16 and U/18, 2022 U/16 copper medallist Tya Zebrowski (FRA) was able to add an U/18 silver medal to her count, with Sara Freyre (USA) and Milla Brown (AUS) winning the bronze and silver medals respectively.


Vaihiti Inso, Team Hawaii / Photo: Jersson Barboza

ISA President, Fernando Aguerre, said:

“What an incredible week. Some of the best waves in the history of our ISA events in El Salvador, and we have had many. It’s been a great partnership with the government of El Salvador. Thank you to President Bukele and thank you to the people of El Salvador for receiving us as warm as ever.

“Congratulations to all the medalists. You are now going home as champions, and the top surfers in the world in the junior divisions. Some of you will be in the Olympics this year, just 75 days away, in Tahiti. Most of you will not, but most of you have the opportunity to be in the 2028 Olympic Games in Los Angeles.”

The ISA World Junior Surfing Championship, held this year in Surf City, El Salvador, saw 441 young surfers from around the globe compete in various divisions. The event is renowned for showcasing the world's best upcoming talent in surfing and offering a glimpse into the sport's future.

As the Irukandjis return home with gold, they bring not only medals but also immense pride and inspiration to the Australian surfing community while putting the rest of the surfing world on notice.

About the ISA:

The International Surfing Association (ISA) is recognized by the International Olympic Committee as the world governing authority for surfing.  This championship has proved to be a direct pathway to the Olympic Games, with  Olympic Bronze Medallist Owen Wright, eight-time World Champion Stephanie Gilmore, two-time World Champion Tyler Wright and Sally Fitzgibbons among the past ISA World Junior Champions.

Results

Team Rankings
Gold – Australia
Silver – Hawaii
Bronze – France
Copper – USA

Boy’s U/16
Gold – Dylan Donegan (ESP)
Silver – Lukas Skinner (ENG)
Bronze – Thiago Passeri (ARG)
Copper – Alexis Owen (NZL)

Girl’s U/16
Gold – Ziggy Mackenzie (AUS)
Silver – Clémence Schorsch (FRA)
Bronze – Louise Le Pront (RSA)
Copper – Eden Walla (USA)

Boy’s U/18
Gold – Dane Henry (AUS)
Silver – Fletcher Kelleher (AUS)
Bronze – Rickson Falcão (BRA)
Copper – Ikko Watanabe (JPN)

Girl’s U/18
Gold – Vaihiti Inso (HAW)
Silver – Tya Zebrowski (FRA)
Bronze – Sara Freyre (USA)
Copper – Milla Brown (AUS)

2024 ISA World Junior Surfing Championship - Team Irukandjis

U18 Girls
Milla Brown (Newport, NSW)
Willow Hardy (Gnarabup, WA)
Isi Campbell (Denmark, WA)

U18 Boys
Eden Hasson (Port Stephens, NSW)
Dane Henry (Fingal Head, NSW)
Fletcher Kelleher (Freshwater, NSW)

U16 Girls
Ziggy Mackenzie (Bilinga, Qld) 
Charli Hately (Tugun, Qld)
Ocea Curtis (Lennox Head, NSW)

U16 Boys
Lachlan Arghyros (Kingscliff, NSW)
Maverick Wilson (Dunsborough, WA)
Ocean Lancaster (Merewether, NSW)

Follow the team and the Irukandjis on Surfing Australia's Socials.

Surfing Australia is thankful for the support it has received from the Australian Government - through the Australian Sports Commission - to help enhance the Irukandjis medal chances at Paris 2024.

2024 Surf City El Salvador ISA World Junior Surfing Championship: Day 9 Action + Closing Ceremony Awards


Ziggy Mckenzie. Credit: ISA / Pablo Jimenez


Ziggy Mackenzie. Credit: ISA / Sean Evans


 Ziggy Mackenzie. Credit: ISA / Pablo Franco


Milla Brown. Credit: ISA / Sean Evans


Milla Brown. Credit: ISA / Pablo Jimenez


Milla Brown. Credit: ISA / Sean Evans


Milla Brown Willow Hardy. Credit: ISA / Pablo Franco


 Ziggy Mackenzie. Credit: ISA / Jersson Barboza


Ziggy Mackenzie. Credit: ISA / Jersson Barboza


Ziggy Mackenzie. Credit: ISA / Sean Evans


Ziggy Mackenzie.  ISA / Pablo Franco


Dane Henry. Credit: ISA / Sean Evans


 Fletcher Kelleher. Credit: ISA / Jersson Barboza


Fletcher Kelleher. Credit: ISA / Jersson Barboza


Dane Henry. Credit: ISA / Pablo Jimenez


Fletcher Kelleher. Credit: ISA / Pablo Jimenez


Milla Brown. Credit: ISA / Pablo Jimenez


 Ziggy McKenzie. Credit: ISA / Pablo Jimenez


Credit: ISA / Sean Evans

Cool Old Truck Spotted At Mona Vale This Week

Her owner said she is 76 years old!


Why are auroras so hard to predict? And when can we expect more?

Aurora visible from Cope Cope, Victoria on May 11 2024. cafuego/FlickrCC BY-SA
Brett CarterRMIT University and Hannah SchunkerUniversity of Newcastle

On Saturday evening before Mother’s Day, Australians witnessed a rare celestial spectacle: a breathtaking display of aurora australis, also known as the southern lights.

Social media was flooded with photos of the vivid pinks, greens and blues lighting up the skies from local beaches and backyards all over the country.

Auroras are normally visible near Earth’s north and south poles. In Australia, they are typically only seen in Tasmania. However, due to rare and special space weather conditions, this time people could see them as far north as Queensland.

The Australian Space Weather Forecasting Centre first issued a potential extreme (G5, most severe level) geomagnetic storm warning on Saturday morning.

Lucky Australians who received this warning, and those who happened to look outside that evening, were rewarded with an amazing spectacle. However, by sunset on Sunday, the chance of aurora had subsided, leaving many hopeful viewers in the dark.

What happened? Why are auroras so hard to predict, and how reliable are aurora forecasts? To answer this, we need to know a bit more about space weather.

What Is Space Weather?

Auroras on Earth are related to the Sun’s magnetic field. The Sun’s activity increases and decreases over an 11-year period called the solar cycle. We are currently approaching the solar cycle maximum, meaning there’s a higher number of sunspots on the Sun’s surface.

These sunspot regions have intense magnetic fields, which can lead to huge explosions of electromagnetic radiation called “solar flares”, and eruptions of material into space, called “coronal mass ejections”.

When this material is directed towards Earth, it collides with Earth’s protective magnetic field, kicking off a series of complex interactions between the magnetic field and the plasma in the ionosphere, part of Earth’s upper atmosphere.

The charged particles resulting from these interactions then interact with the upper atmosphere, causing beautiful and dynamic auroras. The conditions in space produced by this chain of events are what we call “space weather”.

Everyday space weather generally poses no threat, but these events – known as geomagnetic storms – can impact power supplysatellites, communications and GPS, potentially leaving lasting damage.

Saturday’s dazzling display was produced by the most intense geomagnetic storm since November 2003. Fortunately, this time there have been no reports of major disruptions to power grids, but SpaceX’s Starlink constellation was reportedly impacted.

Why Are Geomagnetic Storms Hard To Predict?

Last weekend’s geomagnetic storm was caused by a large and complex region of sunspots that launched a series of solar flares and a train of coronal mass ejections.

Space weather prediction is challenging, and the physics is complex. Even when we see an eruption on the Sun, it’s not clear if or when it will hit Earth, or how strong the effects might be.

Predicted arrival times can be off by up to 12 hours, and it is only when the eruption arrives at monitoring spacecraft close to our planet that can we can gauge the strength of an impending geomagnetic storm.

As a result, aurora hunters really only have up to a few hours advanced notice to decide whether venturing outside is worthwhile or not.

Can We Expect More Auroras Soon?

At the time of writing, the sunspot region responsible for the recent display is still spitting out X-class flares and eruptions, but it’s no longer facing Earth directly. It is possible this region will still be active when it faces Earth again, but this remains to be seen.

However, as we approach solar cycle maximum, other large complex sunspot regions are likely to form and, if the conditions are right, produce more spectacular aurora displays.

A pink and green sky reflected in still water, stars visible at the top.
Aurora australis captured from Joyce’s Creek, Victoria on May 11. Patrick Kavanagh/FlickrCC BY

How To Check For Aurora Forecasts?

Thousands of Australians lined the beaches looking towards the horizon on Sunday night hoping for a second show, only to be disappointed. Official space weather and aurora forecasts provide a wide range of possibilities that must be communicated with the appropriate nuance.

The most reliable sources of information about space weather and aurora are agencies such as the Bureau of Meteorology’s Australian Space Weather Forecasting Centre or the United States NOAA Space Weather Prediction Center.

Not only do they provide aurora forecasts, but they also play a vital role in safeguarding infrastructure from the negative impacts of space weather.

Space Weather Research

Looking ahead, scientists in Australia and around the world are working hard to improve our understanding and prediction of space weather events.

By studying the Sun’s magnetic activity and developing advanced forecasting models of the complex processes that happen between the Sun and Earth, we can better predict and prepare for future space weather events.

A better understanding will help protect important technologies that we rely upon. It will also alert people to step outside and witness a phenomenon that not only lights up the sky, but ignites a profound sense of wonder.


Correction: this article was amended to correct the name of the Australian Space Weather Forecasting Centre.The Conversation

Brett Carter, Associate Professor, RMIT University and Hannah Schunker, ARC Future Fellow, University of Newcastle

This article is republished from The Conversation under a Creative Commons license. Read the original article.

What causes the different colours of the aurora? An expert explains the electric rainbow

Timothy SchmidtUNSW Sydney

Last week, a huge solar flare sent a wave of energetic particles from the Sun surging out through space. Over the weekend, the wave reached Earth, and people around the world enjoyed the sight of unusually vivid aurora in both hemispheres.

While the aurora is normally only visible close to the poles, this weekend it was spotted as far south as Hawaii in the northern hemisphere, and as far north as Mackay in the south.

This spectacular spike in auroral activity appears to have ended, but don’t worry if you missed out. The Sun is approaching the peak of its 11-year sunspot cycle, and periods of intense aurora are likely to return over the next year or so.

If you saw the aurora, or any of the photos, you might be wondering what exactly was going on. What makes the glow, and the different colours? The answer is all about atoms, how they get excited – and how they relax.

When Electrons Meet The Atmosphere

The auroras are caused by charged subatomic particles (mostly electrons) smashing into Earth’s atmosphere. These are emitted from the Sun all the time, but there are more during times of greater solar activity.

Most of our atmosphere is protected from the influx of charged particles by Earth’s magnetic field. But near the poles, they can sneak in and wreak havoc.

Earth’s atmosphere is about 20% oxygen and 80% nitrogen, with some trace amounts of other things like water, carbon dioxide (0.04%) and argon.

A person standing on a dark road at night looking up at a bright pink-red sky.
The May 2024 aurora was visible in the Emilia-Romagna region of northern Italy as well. Luca Argalia/FlickrCC BY-NC-SA

When high-speed electrons smash into oxygen molecules in the upper atmosphere, they split the oxygen molecules (O₂) into individual atoms. Ultraviolet light from the Sun does this too, and the oxygen atoms generated can react with O₂ molecules to produce ozone (O₃), the molecule that protects us from harmful UV radiation.

But, in the case of the aurora, the oxygen atoms generated are in an excited state. This means the atoms’ electrons are arranged in an unstable way that can “relax” by giving off energy in the form of light.

What Makes The Green Light?

As you see in fireworks, atoms of different elements produce different colours of light when they are energised.

Copper atoms give a blue light, barium is green, and sodium atoms produce a yellow–orange colour that you may also have seen in older street lamps. These emissions are “allowed” by the rules of quantum mechanics, which means they happen very quickly.

When a sodium atom is in an excited state it only stays there for around 17 billionths of a second before firing out a yellow–orange photon.

But, in the aurora, many of the oxygen atoms are created in excited states with no “allowed” ways to relax by emitting light. Nevertheless, nature finds a way.

The green light that dominates the aurora is emitted by oxygen atoms relaxing from a state called “¹S” to a state called “¹D”. This is a relatively slow process, which on average takes almost a whole second.

In fact, this transition is so slow it won’t usually happen at the kind of air pressure we see at ground level, because the excited atom will have lost energy by bumping into another atom before it has a chance to send out a lovely green photon. But in the atmosphere’s upper reaches, where there is lower air pressure and therefore fewer oxygen molecules, they have more time before bumping into one another and therefore have a chance to release a photon.

For this reason, it took scientists a long time to figure out that the green light of the aurora was coming from oxygen atoms. The yellow–orange glow of sodium was known in the 1860s, but it wasn’t until the 1920s that Canadian scientists figured out the auroral green was due to oxygen.

What Makes The Red Light?

The green light comes from a so-called “forbidden” transition, which happens when an electron in the oxygen atom executes an unlikely leap from one orbital pattern to another. (Forbidden transitions are much less probable than allowed ones, which means they take longer to occur.)

However, even after emitting that green photon, the oxygen atom finds itself in yet another excited state with no allowed relaxation. The only escape is via another forbidden transition, from the ¹D to the ³P state – which emits red light.

This transition is even more forbidden, so to speak, and the ¹D state has to survive for about about two minutes before it can finally break the rules and give off red light. Because it takes so long, the red light only appears at high altitudes, where the collisions with other atoms and molecules are scarce.

Also, because there is such a small amount of oxygen up there, the red light tends to appear only in intense auroras – like the ones we have just had.

This is why the red light appears above the green. While they both originate in forbidden relaxations of oxygen atoms, the red light is emitted much more slowly and has a higher chance of being extinguished by collisions with other atoms at lower altitudes.

Other Colours, And Why Cameras See Them Better

While green is the most common colour to see in the aurora, and red the second most common, there are also other colours. In particular, ionised nitrogen molecules (N₂⁺, which are missing one electron and have a positive electrical charge), can emit blue and red light. This can produce a magenta hue at low altitudes.

All these colours are visible to the naked eye if the aurora is bright enough. However, they show up with more intensity in the camera lens.

There are two reasons for this. First, cameras have the benefit of a long exposure, which means they can spend more time collecting light to produce an image than our eyes can. As a result, they can make a picture in dimmer conditions.

The second is that the colour sensors in our eyes don’t work very well in the dark – so we tend to see in black and white in low light conditions. Cameras don’t have this limitation.

Not to worry, though. When the aurora is bright enough, the colours are clearly visible to the naked eye.The Conversation

Timothy Schmidt, Professor of Chemistry, UNSW Sydney

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Bert Evans Apprentice Scholarships 2024 are now open!

Do you know a first-year apprentice in NSW who could use some financial assistance? Maybe it’s you!   

The Bert Evans Apprentice Scholarships help NSW apprentices facing hardship to excel and complete their apprenticeships, helping them to develop a fulfilling career and strengthening the growth of your industry.

Up to 150 successful applicants will receive a $5,000 scholarship annually for up to three years, totalling $15,000.    

The funds could be utilised to help purchase new tools, pay for fuel or take additional training courses.   

First-year apprentices, including school-based apprentices, whose employers are in regional or metropolitan NSW, are eligible to apply.     

The Bert Evans Apprentice Scholarships form part of the NSW Government Apprenticeship and Traineeship Roadmap (2024-2026), which will drive the development of Apprenticeships and Traineeships in NSW over the next three years, taking an inclusive and learner-centered approach.       

Applications are open until 31 May 2024.      

For more information around eligibility criteria and how to apply, visit education.nsw.gov.au/skills-nsw/bert-evans-scholarships


Music to the ears: new recording and touring grants

Applications open on 20 March and close 20 May 2024.

Musicians and artists are set to receive a boost under the NSW  Government with the opening of grants focused on rebuilding the NSW touring circuit.

Sound NSW’s new Touring and Travel Fund and Recording and Promotion Grants will inject $3 million into the local contemporary music sector to deliver more new and original music, enable touring opportunities, and open doors for career-defining professional development.

With a focus on fostering growth and sustainability for the contemporary music industry, the programs support NSW artists to be globally competitive, develop industry networks and connect with new audiences locally and internationally.

Touring and Travel Fund

Designed to address the time-sensitive nature of venue availability and performance opportunities, Sound NSW’s $2 million Touring and Travel Fund offers quick response grants of up to $2500 per person for domestic activity and up to $7500 per person for international activity.

Applications for Sound NSW’s Touring and Travel Fund will be assessed on a quick-response basis against eligibility criteria.

Applications open on 20 March via nsw.gov.au/sound-nsw and close 20 May 2024.

Recording and Promotion Grants

Sound NSW’s $1 million Recording and Promotion Grants program will support NSW contemporary musicians to record and release new, original creative projects. NSW artists can apply for grants of:

  • up to $25,000 for short-form releases, such as a single or EP
  • up to $50,000 for long-form releases, such as an album
  • up to $25,000 matched funding for artists signed to a major label. 

Applications open 20 March and close 17 April 2024 at nsw.gov.au/sound-nsw

Minister for the Arts John Graham said:

“We are determined to rebuild the touring circuit, up and down the NSW coast, through our inland tours and suburbs. This fund will do just that.

“We’re delivering on our commitment to bring music back in NSW with this much-needed investment. These fast-response grants will support more new and original music from our musicians, enable tours across Australia and the world, and move NSW a step closer to being a global powerhouse for contemporary music.”

Head of Sound NSW Emily Collins said:

“Recording, releasing and performing new music is essential to the contemporary music industry and the growth and sustainability of artists’ careers, but the upfront costs are often greater than the income generated for many musicians.

“Sound NSW is excited to help bridge this gap by providing this vital funding, removing these prohibitive barriers and supporting NSW artists to do what they do best – making great music.”

School Leavers Support

Explore the School Leavers Information Kit (SLIK) as your guide to education, training and work options in 2022;
As you prepare to finish your final year of school, the next phase of your journey will be full of interesting and exciting opportunities. You will discover new passions and develop new skills and knowledge.

We know that this transition can sometimes be challenging. With changes to the education and workforce landscape, you might be wondering if your planned decisions are still a good option or what new alternatives are available and how to pursue them.

There are lots of options for education, training and work in 2022 to help you further your career. This information kit has been designed to help you understand what those options might be and assist you to choose the right one for you. Including:
  • Download or explore the SLIK here to help guide Your Career.
  • School Leavers Information Kit (PDF 5.2MB).
  • School Leavers Information Kit (DOCX 0.9MB).
  • The SLIK has also been translated into additional languages.
  • Download our information booklets if you are rural, regional and remote, Aboriginal or Torres Strait Islander, or living with disability.
  • Support for Regional, Rural and Remote School Leavers (PDF 2MB).
  • Support for Regional, Rural and Remote School Leavers (DOCX 0.9MB).
  • Support for Aboriginal and/or Torres Strait Islander School Leavers (PDF 2MB).
  • Support for Aboriginal and/or Torres Strait Islander School Leavers (DOCX 1.1MB).
  • Support for School Leavers with Disability (PDF 2MB).
  • Support for School Leavers with Disability (DOCX 0.9MB).
  • Download the Parents and Guardian’s Guide for School Leavers, which summarises the resources and information available to help you explore all the education, training, and work options available to your young person.

School Leavers Information Service

Are you aged between 15 and 24 and looking for career guidance?

Call 1800 CAREER (1800 227 337).

SMS 'SLIS2022' to 0429 009 435.

Our information officers will help you:
  • navigate the School Leavers Information Kit (SLIK),
  • access and use the Your Career website and tools; and
  • find relevant support services if needed.
You may also be referred to a qualified career practitioner for a 45-minute personalised career guidance session. Our career practitioners will provide information, advice and assistance relating to a wide range of matters, such as career planning and management, training and studying, and looking for work.

You can call to book your session on 1800 CAREER (1800 227 337) Monday to Friday, from 9am to 7pm (AEST). Sessions with a career practitioner can be booked from Monday to Friday, 9am to 7pm.

This is a free service, however minimal call/text costs may apply.

Call 1800 CAREER (1800 227 337) or SMS SLIS2022 to 0429 009 435 to start a conversation about how the tools in Your Career can help you or to book a free session with a career practitioner.

All downloads and more available at: www.yourcareer.gov.au/school-leavers-support

Word Of The Week: exuberant

Word of the Week remains a keynote in 2024, simply to throw some disruption in amongst the 'yeah-nah' mix. 

Adjective

1. full of energy, excitement, and cheerfulness. 2. characterised by a vigorously imaginative artistic style. 3. growing luxuriantly or profusely.

From: mid-15c., "over-abundant," from Latin exuberantem (nominative exuberans) "superfluous; extraordinary," present participle of exuberare "be abundant, grow luxuriously," from ex, here probably "thoroughly" + uberare "be fruitful," related to uber "udder,". From 1510s as "growing luxuriantly;" figurative use, of affections, joyous emotions, etc., is by 1640s - 16c: late Middle English (in the sense ‘overflowing, abounding’): from French exubérant, from Latin exuberant- ‘being abundantly fruitful’, from the verb exuberare (based on uber ‘fertile’). 1630's; 'an overflowing'. 

Compare udder (noun)

Old English udder "milk gland of a cow, goat, etc.," from Proto-Germanic udr- (source also of Old Frisian uder, Middle Dutch uyder, Dutch uijer, Old High German utar, German Euter, and, with unexplained change of consonant, Old Norse jugr), from eue-dh-r "udder" (source also of Sanskrit udhar, Greek outhar, Latin uber "udder").

15,000 squares, 500 hours, 19 months: how I used embroidery to make sense of Australia’s catastrophic fires

Tracey Clement, Impossible Numbers. Tracey Clement
Tracey Clement, Australian Catholic University

I slip the needle through a small loop of black thread, pull it tight and snip. Done. I have just tied off the very last stitch on an embroidered scroll that has taken me more than 500 hours across 19 months to complete.

All of my artwork is extremely labour-intensive. But I have to admit, this is a bit excessive, even for me. It’s not surprising that I have been asked more than once “why not just outsource the labour?” and even “what is the point?”

I always sigh and think enviously of plumbers. I am 100% sure hardworking tradies are never asked to justify the point of their work.

Why do I work so hard? There is no one easy answer, it’s different every time. The labour intensity of my processes adds time into the equation and this both carries meaning and can change the meaning of the work as it goes on (and on and on). I always learn something unexpected.

A finger points to a knot on the back of a messy abstract embroidery done in black, red, orange and yellow
The last stitch! Tracey Clement

I put my little scissors down and, before busting out the bubbles, I snap a picture for Instagram because #selfpromotion, but also because this is news, albeit of a very slow-breaking kind. This is what I’ve learned after stitching for seemingly endless hours: while no news may be good news, “slow news” is even better.

My embroidered scroll is titled Impossible Numbers. It started as my attempt to memorialise the estimated 3,000,000,000 non-human lives lost in the devastating bushfires of 2019–20, a number impossible to actually comprehend.

Doomscrolling an emergency

During that long and awful summer Sydney was often shrouded in an eerie orange haze. You could smell smoke. Ash fell. But, like many Australians, I experienced the worst of it by doomscrolling fast news.

I was both horrified and fascinated by images of fires so huge and hot they generated their own weather, by pictures of houses reduced to smoking skeletal outlines that somehow remained standing, by headlines comparing the fires to armageddon and the apocalypse.

This hyperbolic language implies we are locked in a war of good versus evil. Even headlines in the vein of “Firefighters battle blazes” pit us (people) against them (the forces of nature). And in the heat of the moment the language of war feels right. I’ve succumbed to it myself. But it is dangerous. This language reinforces the idea we can dominate nature; it frames the fires as a conflict that we can end by winning.

A hand holds a phone taking a picture of a long abstract embroidery in black, red, orange and yellow.
Viewing the world through the phone. Tracey Clement

I will admit watching a goat-toting woman berate a sitting prime minister left me with a short-lived, but mildly satisfying, feeling of shared righteous indignation. But mostly doomscrolling just fuelled my sorrow and left me feeling impotent as, inevitably, the fast news cycled on to the next crisis (and the next, and the next).

Slowing it down

In October 2022, I finally stopped trying to process the bushfires, and all their terrifying implications, through the fast-news language of war. I picked up a needle instead.

Of course 3,000,000,000 stitches would be too many, even for me, so I decided to stitch a grid of some 15,000 squares, which I filled with innumerable stitches – a nod to the endless stream of pixels that usually deliver our news.

I started wanting to honour the 3 billion dead, that impossible number, but after months of stitching I realised I was “writing” a kind of slow-news story. It may sound ridiculous, but this tactic has been used before. The Bayeux Tapestry is a slow-news story that documents the Norman conquest of England through embroidery. It took years to stitch, and some 950 years later it is still in circulation.

As an alternative to doomscrolling easily digestible fast-news stories of good triumphing (or not) over evil, I have created an actual fabric scroll which depicts a stylised firestorm building in intensity until it becomes all-consuming.

A middle-aged white woman peeks out from behind a very long abstract embroidery in black, red, orange and yellow.
The artist with Impossible Numbers. Tracey Clement

Despite mimicking pixels, Impossible Numbers is resolutely handmade. It is too messy, too crude, to be anything else. It is bleedingly obvious (and there was blood) the will of a person is inextricably stitched into this image of devastating fire. Human labour is literally entangled in this artwork; it shows us as part of the picture, part of nature. And this is good news

Impossible Numbers doesn’t have a victorious ending, or any ending at all. The scroll is not fully unrolled. There is no end in sight: the story isn’t over, it’s ongoing.

In this way it points to the future; a future in which we are not fighting nature. And this is good news too.

If you don’t have a spare 500 hours to process the news into slow news, don’t worry. By the time I finally tied my last knot, I found I had transformed my fear and rage into something tangible, something both magnificent and beautiful (if I do say so myself), no longer about me.

It is now a slow-news story that is no longer about a particular event; something everyone can share. This is why I do the work.

Impossible Numbers is on display as part of The Blake Prize at the Casula Powerhouse, Sydney, until July 7.


This article is part of Making Art Work, our series on what inspires artists and the process of their work.The Conversation

Tracey Clement, Lecturer in Visual Art and McGlade Gallery Director, Australian Catholic University

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Cumberland Council’s book ban has been overturned, but what is really happening in Australian libraries?

Lisa M. Given, RMIT University and Sarah Polkinghorne, RMIT University

At Cumberland City Council in the western suburbs of Sydney, one man – Councillor Steve Christou – persuaded the council to ban books about same-sex parenting from the council’s libraries.

The change was short-lived. People fought back. More than 40,000 signed a petition to lift the ban.

Only two weeks later, the Council reversed its decision, voting decisively (13-2), following impassioned pleas by residents, and with many people protesting on the streets.

Librarians under attack

Librarians are leaders in the fight against book bans. They have faced significant backlash for their efforts. Australian Library and Information Association CEO Cathie Warburton has reported that

people are going into libraries, grabbing books off the shelves, reading them out loud and saying “These shouldn’t be here”, calling librarians horrible names and threatening doxxing and physical violence. It’s incredibly distressing.

Book banning efforts are often highly coordinated. People distribute lists of books that may (or may not) be in the collections of their local libraries. These culture-war attacks on libraries and librarians are often motivated by grievances against progress, such as LGBTQ+ visibility and acceptance, and other forms of diversity.

But they are also part of a wider reactionary movement. The issues extend beyond the specific content of individual books. Calls for book bans are evidence of a broader moral panic that presents a real danger to individuals and society at large.

Libraries and librarians are common targets because they are easy for the public to access, and because they represent (and foster) learning, ideas, imagination, equality, choice and barrier-free access to information for all.

Would-be book banners have very rarely read the books they challenge. When books are read, they are far less likely to be banned.

Histories of censorship

The Cumberland episode is only the latest in the global struggle for freedom of information access. Such censorship dates back at least as far as Shakespeare. The first American book ban occurred in 1637, when Thomas Morton’s New English Canaan was suppressed for its criticisms of Puritanism.

The issue remains highly contentious in the United States. PEN America’s latest report shows a 33% rise in the number of book challenges in US public schools, with almost 6,000 instances of books banned since 2021.

The Alabama House of Representatives recently passed Bill HB385. If it passes the Senate, the bill will override libraries’ book challenge policies. Librarians would have seven days to remove contentious material or face criminal penalties.

Australia also has a long history of censorship. Many titles we now consider “classics” faced bans, including Aldous Huxley’s Brave New World, James Baldwin’s Another Country and D.H. Lawrence’s Lady Chatterley’s Lover. As literary historian Nicole Moore documented, it was once “routine to have your suitcase searched [for obscene materials] on the way into Australia from another country”.

More recently, in March 2023, Maia Kobabe’s award-winning memoir Gender Queer was removed from a Queensland library, and faced many other challenges, globally. Bernard Gaynor, the conservative Catholic activist who led the call to ban the book, is taking the Minister for Communication and the Australian Classification Review Board to the Federal Court of Australia. The decision will come later this year.

Censorship remains a local – and global – concern.

In Australia, many titles we consider ‘classics’ were once banned. Lotus Studio/Shutterstock

Information access for all

Professional librarians have battled these kinds of challenges for decades. The American Library Association, founded in 1876, issued its first anti-censorship notice in 1939, in response to Nazi book burning and other international attempts to suppress information.

In 1953, the American Library Association issued their Freedom to Read statement, with ongoing support for libraries challenging book bans across the United States.

In a joint statement, the Australian Library and Information Association and the Australian Public Library Alliance explain that libraries “defend equity of access to information” and “cater for all members of the library community”.

This position reflects global standards for information access upheld by libraries worldwide. It includes the key principle that the “perception that material may offend or cause controversy to a person or a group of people is not, of itself, a reason to limit purchase or provision of an item containing that material”.

The International Federation of Library Associations states that censorship “runs counter to Article 19 of the Universal Declaration of Human Rights”. Libraries are expected to:

  • provide collections and services that are free of intentional censorship

  • base decisions on professional considerations (e.g., quality, currency, format, cost, etc.), rather than limiting based on political or religious considerations or cultural prejudice

  • educate people on issues of censorship and encourage them to practise freedom of expression and freedom of access to information

  • advocate for removal of censorship restrictions affecting libraries and society at large.

Policies and procedures

Librarians do more than handle attempts to ban books. They develop policies and procedures designed to ensure free access to information, for everyone. They are expert professionals, whose jobs often require difficult selection decisions and challenging conversations with angry or offended community members.

Libraries already have established processes to handle removal requests. They apply guidance from professional associations, including resources like the Selection & Reconsideration Policy Toolkit for Public, School, & Academic Libraries.

Requests to remove materials often start with informal conversations to address concerns and educate complainants about the library’s mandate for equitable access based on the whole community’s needs and interests. A formal process often requires a written submission. Library staff will then reconsider the book in light of the library’s collection policy.

Removing books from a collection does happen, as librarians must ensure the collection remains useful and relevant. Libraries routinely consult with community members and seek feedback to ensure collections match community needs. They also review materials to ensure outdated works (for example, older editions) are replaced with texts that include current information.

These are some of the routine, behind-the-scenes tasks, which collections librarian Scarlet Galvan explains are critical to ensure “collections are for use, not reinforcing assumptions”.

The need for community involvement

Librarians rely on individuals and communities to stand up and oppose censorship, as residents did in Cumberland. Vocal community and government support for libraries is critical to battling book bans. Many other professions, such as journalism and teaching, also play critical roles in documenting censorship and countering book challenges.

So how can you help? By signing petitions, speaking up at council meetings, volunteering to serve on a library board, voting for candidates who support libraries, and borrowing books about diverse families to ensure they have a circulation record of being used and valued.

As the outcry over the short-lived Cumberland City Council ban shows, everyday Australians value libraries and the information they provide to their communities. Public support is needed to defend against future attacks and to send a message to governments that banning books is not acceptable.The Conversation

Lisa M. Given, Professor of Information Sciences & Director, Social Change Enabling Impact Platform, RMIT University and Sarah Polkinghorne, Research Fellow, Social Change Enabling Impact Platform, RMIT University

This article is republished from The Conversation under a Creative Commons license. Read the original article.

We mapped a lost branch of the Nile River – which may be the key to a longstanding mystery of the pyramids

The pyramids at Giza, like dozens of others, are located several kilometres west of the current path of the Nile. Alex Cimbal / Shutterstock
Timothy J. Ralph, Macquarie University; Eman Ghoneim, University of North Carolina Wilmington, and Suzanne Onstine, University of Memphis

The largest field of pyramids in Egypt – consisting of 31 pyramids built over a millennium, including the famous Great Pyramid at Giza – lies along a narrow strip of land in the desert several kilometres west of the Nile River.

The Nile was at the heart of ancient Egyptian civilisation, and the location of so many pyramids some distance away from the river has until now not been fully explained.

In a new study published in Communications Earth & Environment, we addressed this puzzle. When the pyramids were built they sat next to a now-vanished branch of the Nile, which likely provided transport for workers and their materials.

A changing river

Like other rivers, the Nile adjusts and changes over time in response to climate change, floods and droughts. People and places also move with the river. In the past, civilisations fell and rose on its ebb and flow.

The Nile has not always looked or functioned the way it does now. By reading the landscape in Egypt, traces of the former river and its branches can be found hidden just beneath the land surface.

Now obscured by areas of cultivation and urban settlements, buried by centuries of mud from the modern river, the old channels and their stories have largely been lost to time. Once a mosaic of waterways and wetlands, the Nile is ready to share its secrets again.

Many scholars have discussed and sought answers to the mysteries of the Nile. Previous research has documented evidence for the existence of parts of ancient waterways or wetlands, particularly near the Giza pyramids.

Upstream near Luxor, Nile migration patterns have been investigated, and downstream abandoned channels have been discovered in the Nile Delta. Yet until now we did not have a comprehensive map and understanding of the waterways that fed the extensive pyramid chain from Lisht to Giza in the past.

The Ahramat Branch

A satellite photo of a section of the Nile river, showing the path of the now-vanished Ahramat branch and the pyramids dotted along it.
The water course of the ancient Ahramat Branch borders a large number of pyramids dating from the Old Kingdom to the Second Intermediate Period, spanning between the Third Dynasty and the Thirteenth Dynasty. Eman Ghoneim et al.

Using satellite imagery, high-resolution digital elevation data and historical maps, we identified and traced the long path of a previously unknown channel of the Nile. What we have called the Ahramat Branch once flowed along the Western Desert margin of the Nile floodplain, close to the ancient pyramids.

Many of the pyramids, built during the Old Kingdom (roughly 2700–2200 BCE) and the Middle Kingdom (2050–1650 BCE), have causeways that lead to the branch. Many of these paths terminate in temples that may have acted as river docks in the past.

This suggests the Ahramat Branch was active during multiple phases of pyramid construction and was probably used as a transportation waterway for workmen and building materials to the sites.

Some pyramids have longer or differently angled causeways than others, indicating the builders adapted their construction approaches to the changing riverscape and local conditions at the desert margin.

A group of people standing in a desert in front of ancient stone steps leading up from a vegetated hollow to a further stone structure, with a pyramid in the distance.
Members of the research team stand in front of the pyramid of Unas’s Valley Temple, which acted as a river harbour in antiquity. Eman Ghoneim

Other pyramids were connected to inlets associated with tributaries of the Ahramat Branch on the edge of the Western Desert. In all, analysis of the ground elevation of 31 pyramids and their proximity to the floodplain helped explain the position and relative water level of the Ahramat Branch during the time between the Old Kingdom and the Second Intermediate Period (roughly 2649–1540 BCE).

Digging deep

Once we had mapped the Ahramat Branch, we surveyed the landscape and its shape, and took deep core samples of soil and sediment to study the structure and sedimentology of the former river. We also worked with archaeologists, scientists and members of local communities to gather more context for our work.

The path of the defunct waterway lies between 2.5 and 10.25 kilometres west of the modern Nile river.

Our research suggests the branch ran for about 64 kilometres, was between two and eight metres deep, and between 200 and 700 metres wide. This is similar to the width of the river today.

At one of the sites we examined, near the town of Jirzah, the Ahramat Branch has a symmetrical channel shape. It has also been filled in with muddy and sandy sediment different to other surrounding deposits and the underlying bedrock. This indicates that the old channel has been slowly buried by fine sediment deposited by floods, as the main flow diverted towards the path of the modern river.

What happened to the Ahramat Branch?

Over time, the Ahramat Branch moved eastward and eventually water stopped flowing along it. We don’t know exactly why. Perhaps the Ahramat Branch and its daughter, the modern river, were active together for a time.

The river may have gradually moved to the lower-lying floodplain, towards the current location of the Nile. It is also possible that tectonic activity tilted the whole floodplain to the northeast.

Photo of a woman standing on desert ground examining a piece of rock, with the Great Pyramid of Giza and the Sphinx in the background.
Eman Ghoneim studies the surface topography of the section of the ancient Ahramat Branch located in front of the Pyramids of Giza and the Great Sphinx. Eman Ghoneim

A third possibility is that an increase in windblown sand may have filled up the river’s channel. Increases in sand deposition are most likely related to periods of desertification in the Sahara desert in North Africa.

The movement and diminishing of the Ahramat Branch might also be explained by an overall reduction in water flow due to reduced rainfall and greater aridity in the region, particularly during the end of the Old Kingdom.

This research shows that a multidisciplinary approach to river science is needed to gain a better understanding of dynamic river landscapes. If we want to understand and protect the rivers we have today – and the environmentally and culturally significant sites to which they are inextricably tied – we need a greater appreciation of the interconnected factors that affect rivers and how they can be managed.The Conversation

Timothy J. Ralph, Associate Professor, Macquarie University; Eman Ghoneim, Professor and Director of Space and Drone Remote Sensing Lab, University of North Carolina Wilmington, and Suzanne Onstine, Associate Professor, Department of History, University of Memphis

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Why so many animals have a third eyelid, including our pets – yet humans don’t

You can see this dog’s third eyelid in the corner of its eye. Shooty Photography/Shutterstock
Dan Baumgardt, University of Bristol

Our family dog used to have a rather noticeable extra eyelid that became especially apparent when he dozed off, usually upturned on the rug. This is the fleshy curtain seen at the corner of each eye, closest to the nose. It’s also commonly called the nictitating (literally “blinking”) membrane.

You may have noticed these “third” eyelids on your pets appear occasionally, perhaps during their sleepy moments, or when they’re enjoying a bit of affection. But what does this unusual structure actually do? And why don’t we have one as well?

Third eyelids sweep in a generally horizontal direction across the eye, instead of vertically as the upper and lower lids do. They’re actually a specialised fold of the conjunctiva – the thin, moist membrane that coats the other lids and the exposed white of your eye (the sclera). They’re found in many mammalian species, but are not unique to them. Birds, reptiles, amphibians and fish can also have a third eyelid.

The structure varies too; in many species a cartilage skeleton provides support, while others contain glands that secrete tears. This variation is probably to help animals adapt to multiple different environments – to the sea, the air and even arboreal habitats in trees.

Several different studies have examined third eyelids to help understand their role in hedgehogs, kangaroos and brown bears.

And research has shown the third eyelid functions much as the upper and lower lids do. It protects the eye, and sweeps away any invading debris. It also distributes tears across the eye’s surface, keeping it moist and preventing ulcers forming. This is particularly important in brachycephalic (flat-faced) dogs, like pugs and King Charles spaniels, whose protruding eyes are not as well protected compared to other breeds.

In the wild

Both domestic and wild animals (including species from canine, feline and equine families) need eye shielding and protection from foreign bodies. Wild animals may need them even more, since they might be exploring grasslands, or contending with bites and scratches from prey or rival animals.

Preventing, trapping and removing debris is crucial for desert animals like camels, where sand and dirt might damage the eye. Their third eyelid is partially transparent and this helps camels retain some vision in the middle of a sandstorm, while covering their eyes.

In bushlands, aardvarks also have third eyelids, perhaps to protect their eyes as they root around for insects.

The third eyelid may offer protection from water, and a translucent membrane can aid underwater vision of aquatic animals, including manatees (curiously, manatees come from the order Afrotheria, which also includes aardvarks). Larger species of sharks (blues for instance) typically protect their eyes with their third eyelid when hunting and feeding.

For birds, fast air currents can prove equally damaging. So, in birds of prey like falcons, the eyelid is used during rapid flight in hunting. Often air gusts will set off third eyelid blinking in these birds (including owls) as a natural protective reflex.

mysterious looking crow with visible third eyelid
This crow’s third eyelid is visible in this photo. Fotograf Julian/Shutterstock

In other avian species, it might protect against damage from sharp-beaked offspring. Imagine a bird returning with a prize of food to a nestful of voraciously hungry chicks, all pecking and scrabbling to get their share.

Studies suggest third eyelids play a unique role in woodpeckers, whose skulls undergo vibration trauma when drilling a tree trunk with their beak. Two problems arise as a result of this forceful head banging – damage to the softer eye tissue, and sawdust being thrown into them. In this case, the third eyelid may act as both a seatbelt and a visor.

In polar regions, where the white landscape reflects sunlight, ultraviolet rays can damage the eye. This can lead to temporary loss of vision – a condition known as snow blindness. So it’s possible that some arctic animals like polar bears have third eyelids that absorb UV light. There’s no established evidence of this yet, but their third eyelids are clear, assisting them in being skilled marine hunters.

Evolutionary loss

Humans and most primates (except lemurs and the calabar angwantibo, from the Lorisidae family) have evolved to the point where a proper third eyelid is no longer needed. Human and primate eyes are less likely to be damaged by hunting, rivalry and the environment. Plus, human eyes are highly sensitive and able to recognise and respond to danger by closing more quickly.

But the third eyelid isn’t entirely gone. Humans have a remnant of it called the plica semilunaris. This crescent-moon fold can be seen at the corner of our eyes too. Have a look yourself in the mirror.

Some scientists have argued the plica can still help drain tears. There are two small ducts at the angle of our eyelids, which allow excess and old tears to escape into the nasal cavity. That explains why you get a runny nose when you cry.

But would getting our true third eyelid back be of any use to us? Maybe the alien in Men in Black could offer an opinion. Perhaps it could allow us to naturally keep our eyes cleaner, less irritated, or dislodge that contact lens that won’t come out.

We’ll just have to accept we don’t share the clever nature of our pets’ third eyelids. But then we also can’t compete with their night vision, acute hearing or sense of smell. It’s a long list.The Conversation

Dan Baumgardt, Senior Lecturer, School of Physiology, Pharmacology and Neuroscience, University of Bristol

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Let It Be: rerelease of 1970 Beatles film reveals how the history of popular music is written

Adam Behr, Newcastle University

In one sense, Let It Be director Michael Lindsay-Hogg’s 1970 film documenting The Beatles’ recording sessions of January 1969, and their famous concert on the rooftop of the Apple building, could be viewed as something of a coda to the main event.

At the time, both the film and the accompanying album of the same name reached the public a month after the band’s break up was announced. In the present day, its rerelease follows Peter Jackson’s epic Get Back docuseries, which drew on the 60 hours of raw footage of the same sessions to provide a more complete account of the recordings.

So, why the fuss? Rereleases and remasters are a standard feature of both the film and music industries, and The Beatles’ media and commercial juggernaut has arguably led the way in this for a long time. First, there’s the sheer length of time since the film was last generally available – more than 50 years.

The answer also partly lies in the distinctive way in which, beyond their huge financial success, the narrative of The Beatles as a band has been woven into popular music and wider history. Peter Jackson’s 2020 series in many respects superseded Hogg’s film, providing a fuller picture of the sessions, which also fed into the Abbey Road album, the band’s last recording (even though Let It Be was released afterwards).

Same events, different perspectives

A highlight of both the film and series was the concluding rooftop concert, but Jackson’s programme was widely acknowledged for adding context to the band’s closing chapter. The hours of jamming and studio high-jinks revealed moments of camaraderie and a less rancorous atmosphere than had previously been thought.

So, beyond the events themselves, there’s an element of historiography at play here – a concern with how history is written and constructed. Since Let It Be’s original release, The Beatles have become an increasingly important aspect of popular music, and wider social history. Beyond the mystique acquired by inaccessibility for so long, the film gains interest as a document of how the band’s last days as an active unit were framed, and experienced, at the time.

In purely functional terms, it’s obviously easier to give a more complete account of the recording sessions in the nearly eight hours afforded by Peter Jackson’s Get Back than the one and a half hours available to Lindsay-Hogg on Let It Be.

Moments of discord appear in both, notably the famous encounter between a taciturn George Harrison – who walked out during the sessions – telling a cajoling Paul McCartney, about a guitar part: “I’ll play, you know, whatever you want me to play. Or I won’t play at all, if you don’t want me to play.”

These are diluted in the long stretch of Get Back, but become part of the central narrative of Let It Be. Filmmakers’ editorial decisions shape their stories, but are informed by their own contexts. Lindsay-Hogg was editing the film at a time when the band had just split, and trying to salvage a viable product from a somewhat chaotic process, since he’d originally been taken on to produce a television documentary and concert broadcast.

Re-tooling it as a film was a response to the band dropping the idea of a major event, the now legendary rooftop performance only emerging as a process of back and forth compromise.

Conversely, one of the iconic elements of Jackson’s Get Back series shows Paul McCartney coming up with the bare bones of the song of the same name more or less impromptu, and the pleasure in seeing how it develops. But that relies on the more leisurely pacing of the long form allowed by primary release on a streaming platform, as opposed to the editorial constraints of a cinema (or even television) release.

The streaming format was, of course, a long way off in the future when Lindsay-Hogg was working with the band. Jackson’s series also works more profoundly because of the classic status Get Back (the song) has accrued over half a century. For Lindsay-Hogg filming in 1969, it was just another jam – albeit by the world’s most famous band. In 2020, much of the audience was witnessing the genesis of a song they’d known their whole lives.

Framing popular music history

Get Back reviews the longitudinal process of a band at work, and one whose working processes had influenced many of the acts that followed in their wake. The Beatles’ success helped to shape the very idea of a band combining multiple songwriters and friends into a social, creative and business unit.

Their split was big news, and mattered in a way that the re-combinations of musicians into new working units had not done previously. Let It Be was tied into that historical moment, and the presence in the room of Lindsay-Hogg’s cameras helped to define it.

Viewed at the arrival of the 1970s, as the preeminent band of the 1960s announced their demise, Let It Be told the story of an ending, enhanced by the technical fact that it was blown up from a 16mm print, for TV, to 35mm for the cinema, adding a dark, grainy patina to the proceedings, now alleviated in the remastering process.

Now in 2024, it’s a document in a wider archive of Beatles lore and helps to inform the process of how the history of popular music is written.The Conversation

Adam Behr, Senior Lecturer in Popular and Contemporary Music, Newcastle University

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Fossil captures starfish splitting itself in two – showing this has been happening for 155 million years

The 155-million-year-old fossil Gunter Schweigert, CC BY
Aaron W. Hunter, University of Cambridge

One of the wildest wonders of nature is the ability of some animals to reproduce by splitting in half. There is still so much we don’t know about this process. So the discovery of a 155-million-year-old starfish fossil frozen partway through this process, published in a new study, could give scientists incredible new insights.

Our planet is teeming with invertebrates that, to our human eyes, may seem alien in the way they live and reproduce.

The starfish, or asteroid, is part of a group of animals called the echinoderms or spiny skinned animals that also includes sea lilies, sea urchins and sea cucumbers. They are found in almost every corner of our oceans and spend part of their life as microscopic larvae before developing into adults.

Starfish are among the oldest living animals on our planet. They appeared in a form we would recognise almost 480 million years ago and have survived five mass extinctions.

The reason for their evolutionary success could be in their ability to reproduce both sexually and asexually – by literally splitting in two and growing into two new animals. This is known as fissiparity. It is still sometimes observed in modern starfish and comes with the advantage of forming numerous offspring in a relatively short time and without “costing” the parent a great amount of energy or time.

Sexual reproduction, on the other hand, requires starfish and brittle stars to come together in huge numbers to spawn. The disadvantage of fissiparity is that this type of reproduction can result in a lack of genetic diversity in the population.

Biologists call the process of splitting in two parts fragmentation. Only a small number of animals can do this. For example, the common garden earthworm, which many gardeners have watched in amazement as one animal suddenly becomes two. Biologists can also watch starfish and brittle stars doing this in their labs or in marine stations.

But, until now, scientists weren’t sure how old this form of reproduction was. This phenomenon is most often seen in worm-like animals, and worm fossils are rare.

However, starfish can also split in two and have a much better fossil record. These animals still dominate our oceans, the deep seas are a carpet of them.

Close up of brown brittle star in women's hand
Brittle stars (in this case a serpent star) are still alive today. Ana y Erik/Shutterstock

Rebirth of a fossil star

In the past ten years, Ben Thuy, a palaeontologist, has revolutionised the way we look at the evolution and biology of a group of starfish-like animals called the brittle stars or ophiuroids.

First by looking at how these animals have evolved, survived and then thrived in response to mass extinction events or ecological pressure. His work, studying the way their skeleton is made up of calcite plates, has changed our view of not only how the modern brittle star body shape appeared in the fossil record but also how we classify these animals.

In palaeontology, we are always searching for that key fossil that radically changes our view of how life evolved and developed on this planet. For example, the 2021 discovery of 480-million-year-old starfish-like animals in the Anti-Atlas mountains in Morocco helped us understand how these animals first appeared.

Such fossils are the holy grail of palaeobiology. They can give us a snapshot of the history of life and show us the moment a new animal first evolved on our planet.

Only a few animals make it into the fossil record, and many of these are in fragments as they often fall apart once the body has decayed. However, Thuy’s brittle star discovery appears to show a brittle star in the process of reproducing asexually. The fossil has already been “born”. One half of the body appears to be fully developed while the other half shows signs of regeneration with three smaller arms clearly visible.

This discovery means that we know that these animals were reproducing in this way 90 million years before the asteroid collision that wiped out the dinosaurs.

Scientists don’t always agree on what a fossil shows. There is a chance the brittle star fossil is a new species or an unusual individual that happens to have six arms rather than the typical five.

There are many examples of starfish that have more than five arms, including species such as Coscinasterias calamaria or 11 armed starfish. They can also gain an extra arm through natural genetic variation in the population similar to eye colour in humans.

But the study authors used comparative studies of other brittle stars that appear to have undergone regeneration to argue that their fossil originally had six arms before it split in two. Therefore, the authors say, the fossil must be the result of clonal fragmentation and the first in the fossil record.

If they’re right, fossils have allowed us to see the moment a new starfish was born in deep time.The Conversation

Aaron W. Hunter, Science Guide & Visiting Researcher, Earth Sciences, University of Cambridge

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Florence Nightingale overcame the limits set on proper Victorian women – and brought modern science and statistics to nursing

Florence Nightingale experienced her personal call to nursing at age 16 and ultimately became known as the “Lady with the Lamp.” Photos.com/Getty Images
Melissa Pritchard, Arizona State University

For nearly 200 years, Florence Nightingale’s name has been synonymous with gentle compassion and mercy.

In the mid-19th century, Nightingale became perhaps the most celebrated woman of her era – second only to Queen Victoria – for instituting sanitation practices that sharply cut death rates among British soldiers fighting in the Crimean War. A handsome bronze statue in London’s Waterloo Place has immortalized Nightingale as a slight, graceful figure carrying a lamp, the embodiment of selfless womanhood.

But this iconic image overshadows many other accomplishments. Nightingale also transformed nursing into a respectable profession, founded the world’s first nursing school, used the relatively new science of statistics to improve health care outcomes and redesigned hospitals. She was also one of Western history’s first advocates of health care for all.

Over the five years I spent researching and writing my biographical novel about Nightingale, “Flight of the Wild Swan,” published March 12, 2024, my vaguely sentimental notions about her were replaced by respect for her visionary achievements. I resolved to bring into sharper focus this woman who, along with her legendary work as a war nurse, spent half a century pioneering advances in health care.

The 19th century ushered in a series of revolutionary medical advancements. Nightingale’s contributions were a significant part of this era.

Memorial statue of Florence Nightingale against a blue sky.
A statue of Nightingale erected in London’s Waterloo Place celebrates her life and contributions to health care. Tony Baggett/iStock via Getty Images

Called to serve the suffering

Florence Nightingale was born in Florence, Italy, on May 12, 1820, to William and Frances Nightingale, a wealthy British couple. The Nightingales raised their two daughters, Florence and her sister Parthenope, on two estates in England. William homeschooled the girls, giving them the equivalent of his own Cambridge University education.

From an early age, Nightingale displayed a formidable intellect, with a particular interest in mathematics. At 16, she experienced a transcendent call to serve the suffering, a call that eventually coalesced into her determination to become a nurse. Her family objected, however, because nursing was an unsuitable occupation for young Victorian women of privilege. It was considered disreputable work with a status even lower than that of servants.

But Nightingale gradually overcame her family’s objections, receiving training in Germany and France. In 1853, she became the superintendent of a small hospital in London for “distressed gentlewomen.” The majority of her patients were educated, unmarried governesses whose health had broken down under the strain of long hours of work and negligible pay.

A little over a year later, she was on her way to the Crimean War.

Portrait of Florence Nightingale
Florence Nightingale set the standards for modern-day nursing. National Library of Medicine

Bringing sanitation to medicine

In October 1854, Nightingale brought 38 female nurses under her supervision to Scutari Barrack in Constantinople – today’s Istanbul. Originally a gargantuan stone barracks for the Turkish army, Scutari was now a British hospital housing thousands of wounded English and Irish soldiers.

At Scutari, she and her nurses found few provisions, little medicine or edible food, and overcrowded hospital wards full of rats, lice and raw sewage. More soldiers were dying of cholera and other infectious diseases than of battle wounds. Nightingale and her nurses set to work cleaning and procuring food, soap, bandages, medicine, clean bedding and clothes for patients. As living standards improved, Scutari’s appalling death rate began to decline.

It was there that Nightingale’s reputation as the “Angel of the Crimea” and the “Lady with the Lamp” began. Wartime journalists telegraphed their newspapers with dramatic accounts of her work. These stories ignited the public’s imagination and created the indelible image of a slight, feminine figure carrying her lamp through hospital wards at night.

In January 1855, British Prime Minister Henry John Temple, 3rd Viscount Palmerston, dispatched a newly formed Sanitary Commission to the Crimea to investigate high mortality rates in the military hospital. Nightingale observed firsthand the dramatic decline in death rates as the commission cleaned out the hospital’s befouled sewer systems, limewashed its walls – in effect killing surface bacteria – and made numerous other sanitation improvements.

Nightingale was already a proponent of hygiene, fresh air and proper diet in medical care; this experience made her a committed sanitarian.

When the war ended in 1856, Nightingale returned home, permanently bedridden with chronic brucellosis, then called “Crimean fever.” This didn’t stop her from spending the rest of her life applying herself to improving health care systems in Great Britain and other countries.

To celebrate her 200th birthday in 2020, the Florence Nightingale Museum in London produced this film about her life, including her struggles to become a nurse despite her family’s disapproval.

Using numbers to cure

Statistics was a relatively new science in Nightingale’s time, but it aligned with her early interest in mathematics. Ultimately, Nightingale would come to believe that statistics used to help reduce mortality rates were “the true measure of God’s purpose.”

Collaborating with William Farr, a leading figure in applying statistics to epidemiology, Nightingale analyzed extensive data on army mortality rates during the Crimean War, proving that most deaths were attributable to preventable diseases rather than battlefield injuries. She was particularly innovative in her use of graphic diagrams such as her famous “rose,” or “coxcomb,” diagram, rightly believing that attractive visuals were more impactful than the dry numbers tables favored by the era’s statisticians.

Nightingale used statistical data to create her famous ‘rose chart’ – one of the first pie charts ever created – showing that the vast majority of deaths among British soldiers during the Crimean War were from preventable diseases, not battle wounds. Wikimedia Commons/Public Domain

As a result, in 1858, in recognition of her use of the statistical method in army sanitary reform, Nightingale was inducted into the Royal Statistical Society as the organizations’s first female fellow. In 2020, the Royal Statistical Society established an annual Florence Nightingale Award for Excellence in Health and Care Analytics.

In a revolutionary step, Nightingale extended her statistical methods and data visualization to other areas, ranging from hospital administration and health care management to public sanitary reform and the sources of preventable diseases. These analyses further exposed the causes of both military and civilian mortality.

Educating future nurses

In 1860, seeking to elevate nursing into both a science and an art, Nightingale founded the world’s first school of nursing: the Nightingale Training School for Nurses at St. Thomas’ Hospital, London.

The female students – numbering 20 to 30 at a time – lived at school and wore nurses’ uniforms to rigorous classes on anatomy, surgical nursing, physiology, chemistry, sanitation and ethics. By the 1880s, Nightingale had accepted the newer “germ theory” of disease spread, and this became part of the curriculum.

At the conclusion of the one-year program, Nightingale sent her nurses into the world as certified and paid health professionals.

By the turn of the century, the school had graduated nearly 2,000 certified nurses. Known as “Nightingales,” they fanned out across Great Britain to practice skilled patient care, develop nursing care systems, teach, train and mentor.

The Nightingale Training School became a pioneering model for nursing education throughout Great Britain. Similar schools would be established in Africa, America, Australia, Canada and other countries.

Nightingale also wrote a bestselling book, 1859’s “Notes on Nursing,” that guided Victorian wives in keeping members of their households healthy.

Advocating for public health

Nightingale’s long, ultimately successful effort to bring trained nurses and midwives into England’s and Ireland’s notorious workhouses has gone largely unacknowledged.

During Victorian times, paupers in workhouses who became ill could be cared for only by other destitute workhouse residents. Nightingale wrote numerous articles emphasizing the need for public health nurses to care of the sick in these institutions, and during the 1860s she called for the abolition of England’s harsh poor laws.

As a result of these efforts, workhouse nursing reforms gradually spread across England.

I believe that a more fully realized understanding of Nightingale’s life and achievements beyond being “the lady with the lamp” can provide an inspirational role model for those considering careers in nursing, medical science and public health today.The Conversation

Melissa Pritchard, Professor Emeritus of English and Women’s Studies, Arizona State University

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Black holes are mysterious, yet also deceptively simple − a new space mission may help physicists answer hairy questions about these astronomical objects

An illustration of a supermassive black hole. NASA/JPL
Gaurav Khanna, University of Rhode Island

Physicists consider black holes one of the most mysterious objects that exist. Ironically, they’re also considered one of the simplest. For years, physicists like me have been looking to prove that black holes are more complex than they seem. And a newly approved European space mission called LISA will help us with this hunt.

Research from the 1970s suggests that you can comprehensively describe a black hole using only three physical attributes – their mass, charge and spin. All the other properties of these massive dying stars, like their detailed composition, density and temperature profiles, disappear as they transform into a black hole. That is how simple they are.

The idea that black holes have only three attributes is called the “no-hair” theorem, implying that they don’t have any “hairy” details that make them complicated.

Black holes are massive, mysterious astronomical objects.

Hairy black holes?

For decades, researchers in the astrophysics community have exploited loopholes or work-arounds within the no-hair theorem’s assumptions to come up with potential hairy black hole scenarios. A hairy black hole has a physical property that scientists can measure – in principle – that’s beyond its mass, charge or spin. This property has to be a permanent part of its structure.

About a decade ago, Stefanos Aretakis, a physicist currently at the University of Toronto, showed mathematically that a black hole containing the maximum charge it could hold – called an extremal charged black hole – would develop “hair” at its horizon. A black hole’s horizon is the boundary where anything that crosses it, even light, can’t escape.

Aretakis’ analysis was more of a thought experiment using a highly simplified physical scenario, so it’s not something scientists expect to observe astrophysically. But supercharged black holes might not be the only kind that could have hair.

Since astrophysical objects such as stars and planets are known to spin, scientists expect that black holes would spin as well, based on how they form. Astronomical evidence has shown that black holes do have spin, though researchers don’t know what the typical spin value is for an astrophysical black hole.

Using computer simulations, my team has recently discovered similar types of hair in black holes that are spinning at the maximum rate. This hair has to do with the rate of change, or the gradient, of space-time’s curvature at the horizon. We also discovered that a black hole wouldn’t actually have to be maximally spinning to have hair, which is significant because these maximally spinning black holes probably don’t form in nature.

Detecting and measuring hair

My team wanted to develop a way to potentially measure this hair – a new fixed property that might characterize a black hole beyond its mass, spin and charge. We started looking into how such a new property might leave a signature on a gravitational wave emitted from a fast-spinning black hole.

A gravitational wave is a tiny disturbance in space-time typically caused by violent astrophysical events in the universe. The collisions of compact astrophysical objects such as black holes and neutron stars emit strong gravitational waves. An international network of gravitational observatories, including the Laser Interferometer Gravitational-wave Observatory in the United States, routinely detects these waves.

Our recent studies suggest that one can measure these hairy attributes from gravitational wave data for fast-spinning black holes. Looking at the gravitational wave data offers an opportunity for a signature of sorts that could indicate whether the black hole has this type of hair.

Our ongoing studies and recent progress made by Som Bishoyi, a student on the team, are based on a blend of theoretical and computational models of fast-spinning black holes. Our findings have not been tested in the field yet or observed in real black holes out in space. But we hope that will soon change.

LISA gets a go-ahead

In January 2024, the European Space Agency formally adopted the space-based Laser Interferometer Space Antenna, or LISA, mission. LISA will look for gravitational waves, and the data from the mission could help my team with our hairy black hole questions.

Three spacecrafts spaced apart sending light beams towards each other while orbiting the Sun
The LISA spacecrafts observing gravitational waves from a distant source while orbiting the Sun. Simon Barke/Univ. Florida, CC BY

Formal adoption means that the project has the go-ahead to move to the construction phase, with a planned 2035 launch. LISA consists of three spacecrafts configured in a perfect equilateral triangle that will trail behind the Earth around the Sun. The spacecrafts will each be 1.6 million miles (2.5 million kilometers) apart, and they will exchange laser beams to measure the distance between each other down to about a billionth of an inch.

LISA will detect gravitational waves from supermassive black holes that are millions or even billions of times more massive than our Sun. It will build a map of the space-time around rotating black holes, which will help physicists understand how gravity works in the close vicinity of black holes to an unprecedented level of accuracy. Physicists hope that LISA will also be able to measure any hairy attributes that black holes might have.

With LIGO making new observations every day and LISA to offer a glimpse into the space-time around black holes, now is one of the most exciting times to be a black hole physicist.The Conversation

Gaurav Khanna, Professor of Physics, University of Rhode Island

This article is republished from The Conversation under a Creative Commons license. Read the original article.

‘Dancing’ raisins − a simple kitchen experiment reveals how objects can extract energy from their environment and come to life

Surface bubble growth can lift objects upward against gravity. Saverio Spagnolie
Saverio Eric Spagnolie, University of Wisconsin-Madison

Scientific discovery doesn’t always require a high-tech laboratory or a hefty budget. Many people have a first-rate lab right in their own homes – their kitchen.

The kitchen offers plenty of opportunities to view and explore what physicists call soft matter and complex fluids. Everyday phenomena, such as Cheerios clustering in milk or rings left when drops of coffee evaporate, have led to discoveries at the intersection of physics and chemistry and other tasteful collaborations between food scientists and physicists.

Two students, Sam Christianson and Carsen Grote, and I published a new study in Nature Communications in May 2024 that dives into another kitchen observation. We studied how objects can levitate in carbonated fluids, a phenomenon that’s whimsically referred to as dancing raisins.

The study explored how objects like raisins can rhythmically move up and down in carbonated fluids for several minutes, even up to an hour.

An accompanying Twitter thread about our research went viral, amassing over half a million views in just two days. Why did this particular experiment catch the imaginations of so many?

Bubbling physics

Sparkling water and other carbonated beverages fizz with bubbles because they contain more gas than the fluid can support – they’re “supersaturated” with gas. When you open a bottle of champagne or a soft drink, the fluid pressure drops and CO₂ molecules begin to make their escape to the surrounding air.

Bubbles do not usually form spontaneously in a fluid. A fluid is composed of molecules that like to stick together, so molecules at the fluid boundary are a bit unhappy. This results in surface tension, a force which seeks to reduce the surface area. Since bubbles add surface area, surface tension and fluid pressure normally squeeze any forming bubbles right back out of existence.

But rough patches on a container’s surface, like the etchings in some champagne glasses, can protect new bubbles from the crushing effects of surface tension, offering them a chance to form and grow.

Bubbles also form inside the microscopic, tubelike cloth fibers left behind after wiping a glass with a towel. The bubbles grow steadily in these tubes and, once they’re big enough, detach and float upward, carrying gas out of the container.

But as many champagne enthusiasts who put fruits in their glasses know, surface etchings and little cloth fibers aren’t the only places where bubbles can form. Adding a small object like a raisin or a peanut to a sparkling drink also enables bubble growth. These immersed objects act as alluring new surfaces for opportunistic molecules like CO₂ to accumulate and form bubbles.

And once enough bubbles have grown on the object, a levitation act may be performed. Together, the bubbles can lift the object up to the surface of the liquid. Once at the surface, the bubbles pop, dropping the object back down. The process then begins again, in a periodic vertical dancing motion.

Dancing raisins

Raisins are particularly good dancers. It takes only a few seconds for enough bubbles to form on a raisin’s wrinkly surface before it starts to rise upward – bubbles have a harder time forming on smoother surfaces. When dropped into just-opened sparkling water, a raisin can dance a vigorous tango for 20 minutes, and then a slower waltz for another hour or so.

Anyone with a few kitchen staples can do their own dancing raisins experiment.

We found that rotation, or spinning, was critically important for coaxing large objects to dance. Bubbles that cling to the bottom of an object can keep it aloft even after the top bubbles pop. But if the object starts to spin even a little bit, the bubbles underneath make the body spin even faster, which results in even more bubbles popping at the surface. And the sooner those bubbles are removed, the sooner the object can get back to its vertical dancing.

Small objects like raisins do not rotate as much as larger objects, but instead they do the twist, rapidly wobbling back and forth.

Modeling the bubbly flamenco

In the paper, we developed a mathematical model to predict how many trips to the surface we would expect an object like a raisin to make. In one experiment, we placed a 3D-printed sphere that acted as a model raisin in a glass of just-opened sparkling water. The sphere traveled from the bottom of the container to the top over 750 times in one hour.

The model incorporated the rate of bubble growth as well as the object’s shape, size and surface roughness. It also took into account how quickly the fluid loses carbonation based on the container’s geometry, and especially the flow created by all that bubbly activity.

Small objects covered in bubbles in carbonated water move upwards towards the surface and back down.
Bubble-coated raisins ‘dance’ to the surface and plummet once their lifting agents have popped. Saverio Spagnolie

The mathematical model helped us determine which forces influence the object’s dancing the most. For example, the fluid drag on the object turned out to be relatively unimportant, but the ratio of the object’s surface area to its volume was critical.

Looking to the future, the model also provides a way to determine some hard to measure quantities using more easily measured ones. For example, just by observing an object’s dancing frequency, we can learn a lot about its surface at the microscopic level without having to see those details directly.

Different dances in different theaters

These results aren’t just interesting for carbonated beverage lovers, though. Supersaturated fluids exist in nature, too – magma is one example.

As magma in a volcano rises closer to the Earth’s surface, it rapidly depressurizes, and dissolved gases from inside the volcano make a dash for the exit, just like the CO₂ in carbonated water. These escaping gases can form into large, high-pressure bubbles and emerge with such force that a volcanic eruption ensues.

The particulate matter in magma may not dance in the same way raisins do in soda water, but tiny objects in the magma may affect how these explosive events play out.

The past decades have also seen an eruption of a different kind – thousands of scientific studies devoted to active matter in fluids. These studies look at things such as swimming microorganisms and the insides of our fluid-filled cells.

Most of these active systems do not exist in water but instead in more complicated biological fluids that contain the energy necessary to produce activity. Microorganisms absorb nutrients from the fluid around them to continue swimming. Molecular motors carry cargo along a superhighway in our cells by pulling nearby energy in the form of ATP from the environment.

Studying these systems can help scientists learn more about how the cells and bacteria in the human body function, and how life on this planet has evolved to its current state.

Meanwhile, a fluid itself can behave strangely because of a diverse molecular composition and bodies moving around inside it. Many new studies have addressed the behavior of microorganisms in such fluids as mucus, for instance, which behaves like both a viscous fluid and an elastic gel. Scientists still have much to learn about these highly complex systems.

While raisins in soda water seem fairly simple when compared with microorganisms swimming through biological fluids, they offer an accessible way to study generic features in those more challenging settings. In both cases, bodies extract energy from their complex fluid environment while also affecting it, and fascinating behaviors ensue.

New insights about the physical world, from geophysics to biology, will continue to emerge from tabletop-scale experiments – and perhaps from right in the kitchen.The Conversation

Saverio Eric Spagnolie, Professor of Mathematics, University of Wisconsin-Madison

This article is republished from The Conversation under a Creative Commons license. Read the original article.

‘Hidden mother’ photos don’t erase moms − rather, they reveal the labor and love that support the child

While the mother’s face isn’t fully visible, the supportive arms encircling her child are. © Andrea Kaston Tange. All images are from the author’s private collection
Andrea Kaston Tange, Macalester College

Collectors relish so-called “hidden mother photographs” as historical oddities.

These 19th-century images contain very young children held still by half-obscured adults who crouch behind chairs or lurk at the margins of pictures, their protective arms stabilizing babies. The heads and shoulders of the adults are sometimes draped in textiles or summarily cut off, or their bodies are partially tucked behind decorative mats that frame the centered child.

The startling realization that Victorian infants were not reclining on cozy blankets but on comfortable laps fuels breathless online attention. Eager resellers of flea-market finds advertise hidden mother photographs using terms like “spooky wonderful,” “cutie creepy” and “bizarre.” Articles about them tend to imply a treasure hunt for hiddenness – for adult knees or noses, poised hands, bosoms, hat brims and skirts.

But this common framing reduces their cultural importance to sensationalism: Look at how kooky our ancestors were!

Sepia photo of young child in a dress, held in the lap of an adult whose face is covered by a black box
The draped ‘mother’ in this carte-de-visite is probably a man, based on the visible adult hand and sleeve. The head of the adult was removed by a smear on the developing plate. JNO. W. Minner’s City Gallery, Sparta, Illinois. (c. 1862–64) © Andrea Kaston Tange. All images are from the author’s private collection.

As someone who has studied the history of these photos, I find myself drawing an unlikely connection between these stiff, sepia portraits and modern candid snapshots of mischievous children delighting their adoring mothers. Both are part of the tradition of sentimental image-making that surrounds the iconic figure of mother and child.

Exposure times in 19th-century photography were very long by current standards – 20 to 60 seconds – which helps explain why trusted adults were needed to soothe infant subjects into the stillness necessary to take a portrait. But this technological limitation doesn’t explain why their mothers were half-erased from these photos, which has led scholars to argue that Victorian women were effaced by their culture, and casual viewers to assume that the photographers who produced these visual gaffes were hilariously bad at their craft.

But my research has shown that Victorian photographers were documenting children at a moment of widespread desire to focus cultural attention – and therefore camera lenses – on childhood as a precious time that ought to be protected. And the partial obfuscation of mothers was not inconsistent with images of beloved children, because to cherish is to hold.

These are, in short, images of care.

Sepia photograph of toddler in dress sitting in lap of adult with cut off head and legs
A well-dressed toddler girl sits on the lap of an elaborately clothed woman, whose head and lower legs have been removed with a vignette filter, circa 1871–74. © Andrea Kaston Tange. All images are from the author’s private collection.

Evolving photographic forms

Photography was a new technology in the 19th century. Early photographers coated thin metal plates with light-sensitive material, exposed them behind the camera’s lens and developed the plates through precise chemical processes. Each exposure yielded a unique and unreproducible picture directly on the metal.

The fragile daguerreotypes of the early 1840s launched a period of constant experimentation. Photographers eventually perfected sturdier tintypes – also unreproducible images on metal plates – and later revolutionized the medium with glass negatives that enabled multiple prints of the same image. These prints required special paper made light sensitive with a coating of ammonium chloride stabilized in albumen, or egg white. With this process, photography became widely viable as a profession, a hobby and an art. In the 1880s, at the height of its production, the Dresden Albumenizing Company required 60,000 eggs a day to meet worldwide demand for its high-quality photographic paper.

Comparing an 1860s tintype with an 1890s gelatin silver studio print shows the evolution of photographic processes.

Two images side by side: a sepia photograph of toddler held in lap of adult with half of head cut off, and a black and white photograph of a toddler sitting in a draped chair
Plain clothing and lack of studio props in the photo on the left suggests this baby boy sits on his working-class mother’s lap, circa 1860. Conversely, the photo on the right features sophisticated lighting and fine detail in a late portrait of a baby boy perched in a draped chair, with his mother tucked behind, circa 1890s. © Andrea Kaston Tange. All images from the author’s private collection.

The studio portrait is characterized by crisp focus, strong contrast between lights and darks, beautiful mid-tones to contour the baby’s cheek, and artful studio lighting to capture alert infant eyes and the gleam of a mother’s cuff button. The tintype is its opposite in every aspect: Its flattened quality and narrower tonal range are hallmarks of this less technically advanced photographic process.

But in both portraits, the sturdy hands of the loving mother stabilize the child.

Picturing tender connections

Scholars don’t know who was first to use the term hidden mother, although some think it emerged around 2008. A photography exhibit at the Venice Biennale by Linda Fregni Nagler and a lyric photo essay by Laura Larson, both published in 2013 and titled “Hidden Mother,” cemented the moniker, which ironically erases the children who are the focal point of these portraits.

One baby picture in particular – a tintype from the 1850s – tells a story about the development of photographic technology and its role in documenting the fleeting, tender moments of childhood.

The baby’s softness is enhanced by comparison with her mother’s strong jawline. The child’s contemplative gaze suggests deep comfort, snuggled as she is against her mother’s side. The contrast between soft and sharp focus is not just one of emotion but the effect of the little one’s slight movement during the necessarily long exposure time.

The baby’s placidity is partly attributable to the presence of a third figure in this photo. This child appears to be a twin: One of her tiny hands is covered protectively by another, equally small, at the end of another arm clad in an identical dress with braided trim. Grounded in their mother’s lap, these babies exist in a triangulated embrace that memorializes the intimacy of family connections.

Putting the original mat, with its oval cutout, back on the photo makes the baby seem to float, removing the embraces that support her. It also suggests where the moniker for these images, hidden mother, came from. But hands, bodies and the power of touch are central to such images.

Valuing the mother-child bond

Modern viewers often assume that 19th-century customs consigned mothering to the margins. But I argue that this is a projection of ahistorical ideas.

It is a strikingly modern tendency to celebrate women’s ability to have both children and careers, without accounting for how one person will then manage two full-time jobs. Such celebration obscures the labor and time parenting requires in favor of the platitude that if we do what we love, for those we love, it is not work.

Contemporary biases, I suggest, may hide mothers far more than did 19th-century portrait conventions. These images remind thoughtful viewers that babies are held and nursed, soothed and protected, nurtured and guided into independence not by abstract notions of being the right kind of mother, not by oddities, but by embodied human beings.

The historical phenomenon of hidden mothers might be productively renamed “cherished child photographs.” This label more accurately identifies their child subjects and centers the relationship, the cherishing, that is at their heart. It also offers a fruitful avenue for tender contemplation of mothers, children, and the myriad forms of motherwork and bodies who perform them, on Mother’s Day and beyond.The Conversation

Andrea Kaston Tange, Professor of English, Macalester College

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Small but mighty, plankton are some of the most powerful creatures on Earth

Choksawatdikorn/Shutterstock
Abigail McQuatters-Gollop, University of Plymouth

If you go to the beach and dip a bucket in the sea, you might at first think it contains lifeless water. But examine that water under a microscope and you will see your bucket contains a universe of microscopic life, in the form of beautiful and fascinating plankton.

Plankton are mostly microscopic algae and animals found throughout Earth’s oceans, seas and lakes, although a few species are visible to humans. Unlike fish, plankton can’t swim against the current. Instead, they drift through the water, floating at the will of the waves and tides. Plankton are critical to marine ecosystems and to humans, but often glide under the radar of our interest.

As a plankton ecologist who has worked to raise their profile globally, I hope I can convince you that these creatures deserve your attention.

Phytoplankton, the algae plankton, are single-celled organisms. Many of them have chlorophyll, a green pigment (like land plants) they use for photosynthesis to produce the oxygen we breathe. Throughout time, phytoplankton have produced roughly half of Earth’s oxygen, making our atmosphere inhabitable today.

Like land plants, phytoplankton form the base of the marine food web. While cows graze grass on land, zooplankton, tiny marine animals, eat phytoplankton.

Zooplankton include one of Earth’s most abundant animals, the copepod: a microscopic crustacean ranging in size from 0.5 to 15mm. Large copepods are eaten by larval fish, which scientists also classify as plankton since they are too weak and small to swim against the ocean currents. These larvae grow into fish that are eaten by animals higher up the food web, such as sharks, birds and humans.

Tiny creature with two egg sacks attached on either side.
Copepod with eggs. Lebendkulturen.de/Shutterstock

Planktonic krill, a shrimp-like crustacean up to 5cm in size, make up most of the diet of the largest vertebrate to ever live on Earth, the blue whale. Blue whales eat by filtering seawater through their comb-like baleen, pushing out water while keeping the plankton in their mouth.

Unlike most sharks, basking sharks and whale sharks don’t have teeth, and eat copepods, krill and other plankton. It’s amazing to think that microscopic animals are the diet of such huge creatures.

Life cycles

Some zooplankton, like copepods and krill, spend their entire lives in the water column between the surface and bottom of the sea, rather than on the seafloor. Other zooplankton only live in the water column during their larval stages, before maturing and settling to the sea floor or, like larval fish, developing the ability to swim against the currents.

In spring, the sea is full of planktonic crab larvae, flicking their tails to swim as they hunt small copepods and other plankton. Crab larvae don’t look like adult crabs: they have huge spines on the tops and bottoms of their heads, and are long and thin rather than round with pincers. As crab larvae grow through their life stages, they look more and more like their adult selves until, finally, they drop to the sea bottom.

Lobsters, mussels, limpets and barnacles also live as plankton in their larvae stages.

Tiny animal with spine much larger than its body.
Crab larvae have huge spines. Chris Moody/Shutterstock

Astonishing diversity

Scientists estimate there are around 100,000 plankton species in the sea. Plankton communities vary throughout the Earth’s seas and oceans, particularly with latitude. Warmer waters generally have lower plankton biomass and abundance, and consist of species with smaller body sizes.

Jellyfish, my favourite type of zooplankton, are among the biggest plankton. Despite their large size (up to 120 metres long in the case of the Lion’s Mane jellyfish), jellyfish are still considered plankton because they can’t swim against the currents and tides. Instead, they pulse through the water.

There are other types of plankton which are much smaller. These are the pico- and nano-plankton that are too small to see with a classic microscope. These tiny plankton absorb nutrients from, and help decompose, waste such as faeces, dead organisms and other biological material from other parts of the food web. This microbial loop wasn’t discovered until the 1980s.

There is so much about plankton that we still don’t know, and there are thousands of species yet to be discovered.

Climate change canaries

Plankton are extremely sensitive to changes in their environment, which means they respond quickly to alterations in sea temperature and acidity. As sea temperatures rise, warm water plankton communities are shifting away from the equator, into newly temperate environments, while cold water plankton communities are being squeezed poleward.

In the North-east Atlantic ocean, for example, plankton have shifted 1,000 miles northward since the 1960s. But these aren’t the same individuals moving – this is the whole plankton community shifting, over millions of individual lifespans.

Some plankton groups use calcium carbonate, or chalk, to form their shells. As the oceans acidify, plankton that depend on calcium carbonate struggle to form their shells, which protect them from predators and give their bodies structure.

Coccolithophores, a phytoplankton group covered in calcium carbonate liths (external plates), developed malformations in laboratory experiments that manipulated seawater pH. We are not yet sure of the extent that wild populations of coccolithophores are affected by pH change, but they are certainly important to both marine food webs and the removal of atmospheric carbon.

Plankton may be tiny but phytoplankton blooms, which are dense aggregations of microscopic single-celled phytoplankton, can span hundreds of kilometres across the ocean’s surface, and are visible from space using satellites.

Turquoise swirl in the sea next to land mass.
Phytoplankton bloom off South Island, New Zealand. Best-Backgrounds/Shutterstock

These huge blooms sink to the sea floor when the plankton die, transporting carbon to the deep sea and helping to fight climate change.

While plankton blooms like this are usually natural phenomena, they may also occur due to excess nutrients from farming or sewage. If blooms are too big or too concentrated due to excess nutrients, they can cause hypoxic (no oxygen) dead zones on the seafloor. These kill everything that lives there, including animals that can’t escape this deadzone quickly.

There are few groups that are so biodiverse and important for how our oceans, indeed our entire planet, function. The next time you are on a boat or at the beach and look out at the sea, remember that each drop of water is full of microscopic life that makes our planet what it is.The Conversation

Abigail McQuatters-Gollop, Associate Professor of Marine Conservation, University of Plymouth

This article is republished from The Conversation under a Creative Commons license. Read the original article.

book of the month - may 2024: i can jump puddles by alan marshall

Alan Marshall AM, (2 May 1902 – 21 January 1984) was an Australian writer, story teller, humanist and social documenter.

He received the Australian Literature Society Short Story Award three times, the first in 1933. His best known book, I Can Jump Puddles (1955) is the first of a three-part autobiography. The other two volumes are This is the Grass (1962) and In Mine Own Heart (1963).

Marshall was born in Noorat, Victoria. At six years old he contracted polio, which left him with a physical disability that grew worse as he grew older.[2] From an early age, he resolved to be a writer and, in I Can Jump Puddles, he demonstrated an almost total recall of his childhood in Noorat. The characters and places of his book are thinly disguised from real life: "Mount Turalla" is Mount Noorat, "Lake Turalla" is Lake Keilambete, the "Curruthers" are the Blacks, "Mrs. Conlon" is Mary Conlon of Dixie, Terang, and his best friend, "Joe", is Leo Carmody.

During the early 1930s. Marshall worked as an accountant at the Trueform Boot and Shoe Company, Clifton Hill, and later wrote about life in the factory in his novel How Beautiful are Thy Feet (1949).

Marshall wrote numerous short stories, mainly set in the bush, and also wrote newspaper columns and magazine articles. He also collected and published Indigenous Australian stories and legends. He travelled widely in Australia and overseas.

The world at your finger tips: Online

With current advice to stay at home and self-isolate, when you come in out of the garden, have had your fill of watching movies and want to explore something new, there's a whole world of books you can download, films you can watch and art galleries you can stroll through - all from at home and via the internet. This week a few suggestions of some of the resources available for you to explore and enjoy. For those who have a passion for Art - this month's Artist of the Month is the Online Australian Art Galleries and State Libraries where you can see great works of art from all over the world  and here - both older works and contemporary works.

Also remember the Project Gutenberg Australia - link here- has heaps of great books, not just focused on Australian subjects but fiction works by popular authors as well. Well worth a look at.

Short Stories for Teenagers you can read for free online

StoryStar is an online resource where you can access and read short stories for teenagers

About

Storystar is a totally FREE short stories site featuring some of the best short stories online, written by/for kids, teens, and adults of all ages around the world, where short story writers are the stars, and everyone is free to shine! Storystar is dedicated to providing a free place where everyone can share their stories. Stories can entertain us, enlighten us, and change us. Our lives are full of stories; stories of joy and sorrow, triumph and tragedy, success and failure. The stories of our lives matter. Share them. Sharing stories with each other can bring us closer together and help us get to know one another better. Please invite your friends and family to visit Storystar to read, rate and share all the short stories that have been published here, and to tell their stories too.

StoryStar headquarters are located on the central Oregon coast.

NFSA - National Film and Sound Archive of Australia

The doors may be temporarily closed but when it comes to the NFSA, we are always open online. We have content for Kids, Animal Lovers, Music fans, Film buffs & lots more.

You can explore what’s available online at the NFSA, see more in the link below.

https://bit.ly/2U8ORjH


NLA Ebooks - Free To Download

The National Library of Australia provides access to thousands of ebooks through its website, catalogue and eResources service. These include our own publications and digitised historical books from our collections as well as subscriptions to collections such as Chinese eResources, Early English Books Online and Ebsco ebooks.

What are ebooks?
Ebooks are books published in an electronic format. They can be read by using a personal computer or an ebook reader.

This guide will help you find and view different types of ebooks in the National Library collections.

Peruse the NLA's online ebooks, ready to download - HERE

The Internet Archive and Digital Library

The Internet Archive is an American digital library with the stated mission of "universal access to all knowledge." It provides free public access to collections of digitised materials, including websites, software applications/games, music, movies, videos, moving images, and millions of public-domain books. There's lots of Australian materials amongst the millions of works on offer.

Visit:  https://archive.org/


Avalon Youth Hub: More Meditation Spots

Due to popular demand our meditation evenings have EXPANDED. Two sessions will now be run every Wednesday evening at the Hub. Both sessions will be facilitated by Merryn at Soul Safaris.

6-7pm - 12 - 15 year olds welcome
7-8pm - 16 - 25 year olds welcome

No experience needed. Learn and develop your mindfulness and practice meditation in a group setting.

For all enquires, message us via facebook or email help@avalonyouthhub.org.au

BIG THANKS The Burdekin Association for funding these sessions!

Green Team Beach Cleans 

Hosted by The Green Team
It has been estimated that we will have more plastic than fish in the ocean by 2050...These beach cleans are aimed at reducing the vast amounts of plastic from entering our oceans before they harm marine life. 

Anyone and everyone is welcome! If you would like to come along, please bring a bucket, gloves and hat. Kids of all ages are also welcome! 

We will meet in front of the surf club. 
Hope to see you there!

The Green Team is a Youth-run, volunteer-based environment initiative from Avalon, Sydney. Keeping our area green and clean.

 The Project Gutenberg Library of Australiana

Australian writers, works about Australia and works which may be of interest to Australians.This Australiana page boasts many ebooks by Australian writers, or books about Australia. There is a diverse range; from the journals of the land and sea explorers; to the early accounts of white settlement in Australia; to the fiction of 'Banjo' Paterson, Henry Lawson and many other Australian writers.

The list of titles form part of the huge collection of ebooks freely downloadable from Project Gutenberg Australia. Follow the links to read more about the authors and titles and to read and/or download the ebooks. 

Profile: Ingleside Riders Group

Ingleside Riders Group Inc. (IRG) is a not for profit incorporated association and is run solely by volunteers. It was formed in 2003 and provides a facility known as “Ingleside Equestrian Park” which is approximately 9 acres of land between Wattle St and McLean St, Ingleside. IRG has a licence agreement with the Minister of Education to use this land. This facility is very valuable as it is the only designated area solely for equestrian use in the Pittwater District.  IRG promotes equal rights and the respect of one another and our list of rules that all members must sign reflect this.

Cyberbullying

Research shows that one in five Australian children aged 8 to 17 has been the target of cyberbullying in the past year. The Office of the Children’s eSafety Commissioner can help you make a complaint, find someone to talk to and provide advice and strategies for dealing with these issues.

Make a Complaint 

The Enhancing Online Safety for Children Act 2015 gives the power to provide assistance in relation to serious cyberbullying material. That is, material that is directed at a particular child with the intention to seriously embarrass, harass, threaten or humiliate.

IMPORTANT INFORMATION 

Before you make a complaint you need to have:

  • copies of the cyberbullying material to upload (eg screenshots or photos)
  • reported the material to the social media service (if possible) at least 48 hours ago
  • at hand as much information as possible about where the material is located
  • 15-20 minutes to complete the form

Visit: esafety.gov.au/complaints-and-reporting/cyberbullying

Our mission

The Office of the Children’s eSafety Commissioner is Australia's leader in online safety. The Office is committed to helping young people have safe, positive experiences online and encouraging behavioural change, where a generation of Australian children act responsibly online—just as they would offline.

We provide online safety education for Australian children and young people, a complaints service for young Australians who experience serious cyberbullying, and address illegal online content through the Online Content Scheme.

Our goal is to empower all Australians to explore the online world—safely.

Visit: esafety.gov.au/about-the-office 

The Green Team

Profile
This Youth-run, volunteer-based environment initiative has been attracting high praise from the founders of Living Ocean as much as other local environment groups recently. 
Creating Beach Cleans events, starting their own, sustainability days - ‘action speaks louder than words’ ethos is at the core of this group. 

National Training Complaints Hotline – 13 38 73

The National Training Complaints Hotline is accessible on 13 38 73 (Monday to Friday from 8am to 6pm nationally) or via email at skilling@education.gov.au.

Sync Your Breathing with this - to help you Relax

Send In Your Stuff

Pittwater Online News is not only For and About you, it is also BY you.  
We will not publish swearing or the gossip about others. BUT: If you have a poem, story or something you want to see addressed, let us know or send to: pittwateronlinenews@live.com.au

All Are Welcome, All Belong!

Youth Source: Northern Sydney Region

A directory of services and resources relevant to young people and those who work, play and live alongside them.

The YouthSource directory has listings from the following types of service providers: Aboriginal, Accommodation, Alcohol & Other Drugs, Community Service, Counselling, Disability, Education & Training, Emergency Information, Employment, Financial, Gambling,  General Health & Wellbeing, Government Agency, Hospital & GP, Legal & Justice, Library, Mental Health, Multicultural, Nutrition & Eating Disorders, Parenting, Relationships, Sexual Health, University, Youth Centre

Driver Knowledge Test (DKT) Practice run Online

Did you know you can do a practice run of the DKT online on the RMS site? - check out the base of this page, and the rest on the webpage, it's loaded with information for you!

The DKT Practice test is designed to help you become familiar with the test, and decide if you’re ready to attempt the test for real.  Experienced drivers can also take the practice test to check their knowledge of the road rules. Unlike the real test, the practice DKT allows you to finish all 45 questions, regardless of how many you get wrong. At the end of the practice test, you’ll be advised whether you passed or failed.

Fined Out: Practical guide for people having problems with fines

Legal Aid NSW has just published an updated version of its 'Fined Out' booklet, produced in collaboration with Inner City Legal Centre and Redfern Legal Centre.

Fined Out is a practical guide to the NSW fines system. It provides information about how to deal with fines and contact information for services that can help people with their fines.

A fine is a financial penalty for breaking the law. The Fines Act 1996 (NSW) and Regulations sets out the rules about fines.

The 5th edition of 'Fined Out' includes information on the different types of fines and chapters on the various options to deal with fines at different stages of the fine lifecycle, including court options and pathways to seek a review, a 50% reduction, a write-off, plan, or a Work and Development Order (WDO).

The resource features links to self-help legal tools for people with NSW fines, traffic offence fines and court attendance notices (CANs) and also explains the role of Revenue NSW in administering and enforcing fines.

Other sections of the booklet include information specific to Aboriginal and Torres Strait Islander people, young people and driving offences, as well as a series of template letters to assist people to self-advocate.

Hard copies will soon be available to be ordered online through the Publications tab on the Legal Aid NSW website.

Hard copies will also be made available in all public and prison libraries throughout NSW.

Read the resource online, or download the PDF.

Apprenticeships and traineeships info

Are you going to leave school this year?
Looking for an apprenticeship or traineeship to get you started?
This website, Training Services NSW, has stacks of info for you;

It lists the group training organisations (GTOs) that are currently registered in NSW under the Apprenticeship and Traineeship Act 2001. These GTOs have been audited by independent auditors and are compliant with the National Standards for Group Training Organisations.

If you are interested in using the services of a registered GTO, please contact any of the organisations listed here: https://www.training.nsw.gov.au/gto/contacts.html

There are also some great websites, like 1300apprentice, which list what kind of apprenticeships and traineeships they can guide you to securing as well as listing work available right now.

Profile Bayview Yacht Racing Association (BYRA)
1842 Pittwater Rd, Bayview
Website: www.byra.org.au

BYRA has a passion for sharing the great waters of Pittwater and a love of sailing with everyone aged 8 to 80 or over!

 headspace Brookvale

headspace Brookvale provides services to young people aged 12-25. If you are a young person looking for health advice, support and/or information,headspace Brookvale can help you with:

• Mental health • Physical/sexual health • Alcohol and other drug services • Education and employment services

If you ever feel that you are:

• Alone and confused • Down, depressed or anxious • Worried about your use of alcohol and/or other drugs • Not coping at home, school or work • Being bullied, hurt or harassed • Wanting to hurt yourself • Concerned about your sexual health • Struggling with housing or accommodation • Having relationship problems • Finding it hard to get a job

Or if you just need someone to talk to… headspace Brookvale can help! The best part is our service is free, confidential and youth friendly.

headspace Brookvale is open from Monday to Friday 9:00am-5:30pm so if you want to talk or make an appointment give us a call on (02) 9937 6500. If you're not feeling up to contacting us yourself, feel free to ask your family, friend, teacher, doctor or someone close to you to make a referral on your behalf.

When you first come to headspace Brookvale you will be greeted by one of our friendly staff. You will then talk with a member of our headspace Brookvale Youth Access Team. The headspace Brookvale Youth Access Team consists of three workers, who will work with you around whatever problems you are facing. Depending on what's happening for you, you may meet with your Youth Access Worker a number of times or you may be referred on to a more appropriate service provider.

A number of service providers are operating out of headspace Brookvale including Psychologists, Drug & Alcohol Workers, Sexual Health Workers, Employment Services and more! If we can't find a service operating withinheadspace Brookvale that best suits you, the Youth Access Team can also refer you to other services in the Sydney area.

eheadspace provides online and telephone support for young people aged 12-25. It is a confidential, free, secure space where you can chat, email or talk on the phone to qualified youth mental health professionals.

Click here to go to eheadspace

For urgent mental health assistance or if you are in a crisis please call the Northern Sydney 24 hour Mental Health Access Line on 1800 011 511

Need Help Right NOW??

kids help line: 1800 55 1800 - www.kidshelpline.com.au

lifeline australia - 13 11 14 - www.lifeline.org.au

headspace Brookvale is located at Level 2 Brookvale House, 1A Cross Street Brookvale NSW 2100 (Old Medical Centre at Warringah Mall). We are nearby Brookvale Westfield's bus stop on Pittwater road, and have plenty of parking under the building opposite Bunnings. More at: www.headspace.org.au/headspace-centres/headspace-brookvale

Profile: Avalon Soccer Club
Avalon Soccer Club is an amateur club situated at the northern end of Sydney’s Northern Beaches. As a club we pride ourselves on our friendly, family club environment. The club is comprised of over a thousand players aged from 5 to 70 who enjoy playing the beautiful game at a variety of levels and is entirely run by a group of dedicated volunteers. 
Profile: Pittwater Baseball Club

Their Mission: Share a community spirit through the joy of our children engaging in baseball.

Year 13

Year13 is an online resource for post school options that specialises in providing information and services on Apprenticeships, Gap Year Programs, Job Vacancies, Studying, Money Advice, Internships and the fun of life after school. Partnering with leading companies across Australia Year13 helps facilitate positive choices for young Australians when finishing school.

NCYLC is a community legal centre dedicated to providing advice to children and young people. NCYLC has developed a Cyber Project called Lawmail, which allows young people to easily access free legal advice from anywhere in Australia, at any time.

NCYLC was set up to ensure children’s rights are not marginalised or ignored. NCYLC helps children across Australia with their problems, including abuse and neglect. The AGD, UNSW, KWM, Telstra and ASIC collaborate by providing financial, in-kind and/or pro bono volunteer resources to NCYLC to operate Lawmail and/or Lawstuff.

Kids Helpline

If you’re aged 5-25 the Kids Helpline provides free and confidential online and phone counselling 24 hours a day, seven days a week on 1800 55 1800. You can chat with us about anything… What’s going on at home, stuff with friends. Something at school or feeling sad, angry or worried. You don’t have to tell us your name if you don’t want to.

You can Webchat, email or phone. Always remember - Everyone deserves to be safe and happy. You’re important and we are here to help you. Visit: https://kidshelpline.com.au/kids/