The impact of climate change: How longer Earth days will affect our planet

The impacts of climate change are widespread, ranging from biodiversity loss to extreme weather events, rising sea levels, wildfires, and mass human migrations. Each year reveals more about our impact on the environment, with some discoveries more surprising than others.

One of the most shocking revelations to join this list is the recent discovery that our greenhouse gas emissions are altering the Earth’s rotation.

As a result, Earth days are gradually becoming longer, potentially leading to significant changes in how we experience time in the future.

“It’s fascinating how our actions as humans can have such a profound impact on the entire planet through the extensive climate change we’ve triggered over the last century,” says Professor Benedict Soja, a scientist at ETH Zurich who contributed to uncovering this concerning trend.

“This effect may surpass previous significant influences on Earth’s rotation.”

Could we see more hours in a day?

We are familiar with the greenhouse effect, where gases like carbon dioxide trap heat in the Earth’s atmosphere, leading to a rise in temperatures.

Last year, global temperatures were 1.18 degrees Celsius above the 20th-century average, approaching the 1.5 degrees Celsius target set in 2015 as a limit to avoid the worst consequences of climate change.

Record melting of Swiss glaciers in 2022 – Credit: Getty Images

The primary consequence of this warming is the melting of large ice areas in the Arctic and Antarctic, with Switzerland losing 10% of its glacier mass in the last two years, Antarctica shedding 150 billion tons of ice annually, and Greenland losing 270 billion tons.

While many are concerned about the impact of this melting on coastal areas, Soja and his team posed a different question: Will this significant mass redistribution likely prevail? What will be its broad-scale impact on the planet? In a recent study published in the journal Proceedings of the National Academy of Sciences (PNAS), they provided an answer.

“As the ice melts, the Earth’s mass shifts from the polar regions to the oceans,” Soja explained. “This results in the Earth becoming flatter and more oblate, with its mass moving further from the rotation axis.”

Understanding the Mechanism

Similar to any rotating object, the Earth adheres to the law of momentum conservation. Simply put, momentum must be preserved, and it depends on the moment of inertia and rotational speed. As mass moves away from the rotation axis due to melting ice, the moment of inertia increases.

Therefore, to uphold its momentum despite ice melting, the Earth’s rotation slows down, elongating our days.

Soja likens this concept to a figure skater performing a spin, where extending the arms slows down the rotation, while pulling them in speeds it up.

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The effect of changing the distance between the mass and the axis of rotation is seen when figure skaters use their arms to change the speed of rotation.

The study indicated that from 1900 to 2000, the climate’s impact on the length of Earth’s day ranged from 0.3 to 1.0 milliseconds per century. Since 2000, accelerated melting has raised this rate to 1.3 milliseconds per century, with a potential increase to 2.6 milliseconds per century by 2100 if emissions remain unchecked.

While these changes may seem small in our daily lives, they could have significant effects on a globally synchronized technological network.

Considerations on Time Management

Three main timescales play crucial roles in timekeeping: International Atomic Time (TAI), Universal Time (UT1), and Coordinated Universal Time (UTC). TAI relies on atomic clocks, UT1 is determined by Earth’s rotation, and UTC synchronizes the two.

Leap seconds were introduced in 1972 to align UTC with UT1 within 0.9 seconds.

Unlike predictable leap years, leap seconds are added irregularly as needed. Since 1972, 27 leap seconds have been added, with the most recent in 2016. Disruptions from leap seconds have caused issues in the digital age, impacting technology companies striving for synchronization.

Atomic clock made in Germany – Credit: Alamy

The recent discovery of Earth’s core slowing down further complicates matters. If the planet’s rotation continues to accelerate, a negative leap second may need to be introduced to UTC. This unprecedented situation poses substantial challenges as systems are unprepared for negative adjustments.

“This has never occurred before, and frankly, I don’t think anyone anticipated it,” Agnew remarked. He compares this scenario to the Y2K scare when concerns about potential computer errors surfaced at the end of the 20th century.

“The critical aspect is that we don’t know the consequences of introducing a negative leap second,” he cautioned. “The negative impacts could be unforeseen.”

According to Agnew, if the effects of climate change had not slowed down, a negative leap second would have been necessary in 2026. “Global warming might postpone negative leap seconds and eliminate their need entirely,” he noted.

While this discovery regarding climate change may offer a positive effect, considering less necessity for negative leap seconds, the implications of further greenhouse gas emissions outweigh any potential benefits. As the situation stands, negative leap seconds may still be required in 2029.

Perhaps it’s time to reconsider the current system?

Agnew proposed a solution to reduce the required precision between timescales, eliminating the need for negative leap seconds and allowing for more predictable positive adjustments.

“It could resemble a leap year. You add a fixed number of seconds at a specific time and accept that it may not be exact but is tolerable,” suggested Agnew.

This proposition aligns with the dominance of slowing over longer timescales, rather than the complex interactions involving Earth’s core or ice melting.

Efforts are reportedly underway to implement this system, with a target to eliminate the need for leap seconds by 2035. However, international agreement hurdles must be overcome. Failure to adapt before requiring a negative leap second could lead to unprecedented chaos, highlighting the urgency of the situation.


Meet the Experts

Benedict Soja: Assistant Professor in the Department of Civil, Environmental, and Geoengineering at ETH Zurich.

Duncan Agnew: Professor Emeritus at Scripps Institution of Oceanography, specializing in crustal deformation measurement and geophysical data analysis.

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Source: www.sciencefocus.com

Wasps have a unique ability to store alcohol that surpasses any other animal on the planet.

Oriental hornet (Vespa orientalis) may drink you under the table

Vladimir Kazachikov/Shutterstock

One species of wasp, which often eats alcohol-containing foods, can retain alcohol at levels that other known animals cannot tolerate without causing side effects.

‘This is crazy,’ says study author Sofia Bucebuti at Ben-Gurion University in the Negev, Israel.

Oriental wasp diet (vespa orientalis) consists of ripe fruit containing nectar and grapes. This fruit contains sugar, which is converted to ethanol through natural fermentation over time.

While ethanol is highly nutritious for animals, it is also highly intoxicating. Even animals that routinely eat fermented fruit, such as fruit flies and shrews, cannot have more than 4% ethanol in their diet, Bucebuti and his colleagues say.

But when Bucebuti’s team fed the hornets nothing for a week other than various sugar solutions containing varying amounts of ethanol from 1 to 80 percent, the hornets seemed unaffected. Neither their behavior nor their lifespans changed. What makes this particularly surprising is that a solution containing 80% ethanol contains four times the alcohol content of what occurs in nature.

“We initially experimented with only 20%. [ethanol] And we are already surprised,” say study authors Elan Levin At Tel Aviv University, Israel. The 80% ethanol figure is “even more incredible.”

Analysis of the genomes of several wasp species suggests that the insects have two to four copies of the gene that produces NADP+, which helps break down alcohol. Researchers think this may help explain why the oriental hornet, and perhaps other wasp species, can process such large amounts of alcohol.

These findings “remind us that we’re not the only ones who like alcohol.” james fry at the University of Rochester in New York. However, because data from other animal studies are difficult to compare, researchers are not convinced that wasps are the only organisms that can process such large amounts of alcohol.

Wasps’ love of alcohol may give them a competitive advantage when it comes to eating nutritious, highly fermented foods, researchers say. Irene Stefanini At the University of Turin, Italy. She believes that the wasp’s resistance is probably related to the mutualistic relationship between the animal and fermenting brewer’s yeast. budding yeastWhich her study They have been shown to live in the intestines of wasps, survive, and even mate. Perhaps the wasp helps the yeast move from fruit to fruit, and the yeast helps the wasp find energy-rich food.

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  • insect/
  • drugs and alcohol

Source: www.newscientist.com

The Impending Collapse of Atlantic Currents: The Impact on our Planet

The frozen River Thames is being hit by cold winds, the Mersey docks are blocked by ice floes, and crops are failing in the UK. Meanwhile, rising sea levels are flooding the east coast of the United States, and the Amazon ecosystem is experiencing disruptions due to changing seasons. The world has undergone significant changes. What has caused this?

These events may seem like scenes from a disaster movie, but a recent scientific study focusing on the Atlantic Meridional Overturning Circulation (AMOC) warns that these scenarios could become a reality as early as 2050. Learn more.


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What is AMOC, why is it vital, and what changes can we expect? Will disruptions lead to catastrophic events, and how can we address the situation?

The Importance of AMOC and Expected Changes

The AMOC, also known as the “Great Ocean Conveyor,” is a vast ocean current system that includes the Gulf Stream. It transports warm, salty water from the tropics northward into the North Atlantic Ocean. As this water cools and becomes denser, it sinks, flows back southward at depth, and eventually rises to the surface, creating a continuous circulation loop.

This circulation system moves significant amounts of heat around the Atlantic Ocean, equivalent to boiling approximately 100 billion kettles. The AMOC plays a crucial role in distributing heat input to the Northern Hemisphere and affects climate zones worldwide. Any weakening of the AMOC could lead to shifts in global climate patterns, impacting various regions.

Changes in wind patterns can also influence AMOC. Stronger winds during ice ages bolstered parts of the Gulf Stream, while in a warmer future world, wind effects might weaken the AMOC.

Evidences of AMOC Changes

Direct measurements of AMOC strength started in 2004 using the RAPID array across the Atlantic Ocean. Observations indicate a 10% decline in intensity over nearly two decades, but year-to-year variations pose challenges in determining a clear long-term trend.

Past indirect measures, such as cooling trends in southern Greenland, suggest a weakening AMOC. Salt accumulation in the South Atlantic further supports the notion of reduced heat and salt transport due to system weakening.

By studying marine sediment cores and ancient shells, paleoclimatologists have discovered that the current AMOC weakening is unparalleled in the last 1,600 years, indicating a potential 15% decline in the system’s strength.

Future Outlook for AMOC

Climate models predict a 30-50% weakening of AMOC by the end of the century if greenhouse gas emissions continue. This could result in altered weather patterns, increased extreme events, and sea level rise along certain coastlines.

A small increase in global temperatures might trigger a swift shutdown of the AMOC, leading to severe climate impacts. Understanding the potential collapse mechanisms, such as “salt feedback,” highlights the need for immediate climate action to prevent such scenarios.

Managing AMOC Risk

To mitigate the risks associated with AMOC collapse, we must urgently reduce greenhouse gas emissions, enhance climate resilience, and prepare for potential disruptions in food and water supplies. Addressing the root cause of global warming and implementing sustainable practices are crucial in safeguarding the stability of the Earth’s climate system.

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Source: www.sciencefocus.com

Newly Found Planet Orbiting Barnard’s Star Only 6 Light Years from Earth

Artist’s impression of Barnard’s b, a planet orbiting around Barnard’s star

ESO/M.Kornmesser

Barnard’s star, one of the Sun’s closest neighbors, appears to have at least one planet orbiting around it, and possibly three more that require further confirmation.

Astronomers have been searching for planets around Barnard’s star, 5.96 light-years away, since the 1960s. Barnard’s star is the next closest star to us after the three stars in the Alpha Centauri star system.

In 2018, researchers claimed to have discovered a planet at least three times the size of Earth called Barnard Star B, but subsequent analysis revealed that the apparent planet’s signal was actually a larger-than-expected star. Turns out it was caused by activity. .

now, Jonay González Hernández Researchers at the Canary Islands Institute of Astrophysics have announced the discovery of a new Barnard star b, which has about 40 percent the mass of Earth.

The planet is much closer to its star than any other planet in our solar system, completing an orbit in just over three Earth days. This also means that its surface temperature is around 125°C (257°F), too hot for liquid water or life to exist.

Using an instrument called Espresso on the European Southern Observatory’s Very Large Telescope in Chile, González Hernández and his team observed tiny wobbles in Barnard’s star’s position caused by the orbiting planet’s gravity. I discovered this star.

They also found evidence of three more planets orbiting the star. However, the signal wasn’t strong enough to be certain, so more observations will be needed to confirm that.

“These detections are very tricky and always difficult because there is stellar activity, the magnetic field of the star that rotates with the star,” he says. Rodrigo Fernando Diaz at the National University of San Martin, Argentina. González Hernández and his team have thoroughly checked whether the observations are from a planet, but there could always be “unknown unknowns,” Fernando Díaz said. says. To really confirm this, he says, data from other telescopes is needed, which could take years of observations.

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Source: www.newscientist.com

JWST finds a solitary world challenging the distinction between star and planet

Star cluster NGC 1333 contains many brown dwarfs

NASA/CXC/JPL-Caltech/NOAO/DSS

Astronomers have discovered six new worlds that look like planets but formed like stars. These so-called “rogue worlds” are between five and 15 times the mass of Jupiter, and one of them may even host the beginnings of a miniature solar system.

Ray Jayawardene Using the James Webb Space Telescope, a researcher from Johns Hopkins University in Maryland and his colleagues discovered these strange worlds in the NGC 1333 star cluster. Despite being planet-sized, none of these worlds orbit a star. This indicates that they likely formed by the collapse of a cloud of dust and gas, similar to how stars like our Sun are born. These objects that form like stars but are not massive enough to sustain the fusion of hydrogen are called brown dwarfs, or failed stars.

“In some ways, the most shocking thing is what we didn't find,” Jayawardene says. “Even though we had the sensitivity to do so, we couldn't find anything with a mass less than five times that of Jupiter.” This may indicate that brown dwarfs can't form at lower masses — that is, they are the smallest objects that can form like stars.

From their observations, the researchers found that about 10 percent of the objects in NGC 1333 are made up of brown dwarfs — a much higher number than expected based on star formation models — and that additional processes, such as turbulence, may be driving the formation of these nomadic planets.

One of the brown dwarfs is particularly unusual, with a ring of dust around it similar to the ones that formed the planets in our solar system. At about five times the mass of Jupiter, it's the smallest planet with such a ring ever found and may mark the beginning of a strange, shrunken planetary system around a dysfunctional star.

“From the miniature world around these objects, [brown dwarf] “It will glow mostly in the infrared, with a very reddish glow, and over hundreds of millions of years it will gradually fade away and become invisible,” Jayawardene says. As the brown dwarf fades, any planets that form around it will freeze out completely, darkening the entire system and making it a less than promising world for searching for life.

Journal References: Astronomical Journal, Printing

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Source: www.newscientist.com

Searching for the exomoon: Investigating a moon orbiting a distant planet

Many years ago, at that time david kipping When he lived in London, he would walk home through the city and look up at the moon. For astronomers, its dimly glowing presence was a nightly source of inspiration. “It reminded us that satellites are waiting for us around exoplanets,” he says. “It made sense that we should look for them.”

It would be exciting to discover an exomoon, a natural satellite of a world outside our solar system. First, the moon may play a key role in determining the habitability of its host planet by dampening its wobble and promoting a stable climate, in the same way it did for Earth. there is. There may also be strange and wonderful configurations, such as a lunar ring or a moon with its own moon. But the most interesting thing is that some of them may be more suitable for life than exoplanets.

Kipping, now at Cornell University in New York, is part of a small community of astronomers exploring solar moons. At least statistics are on your side. About 5,500 exoplanets have been discovered so far, some of which may have dozens of moons. The problem is that it’s not easy to prove its existence. Two previous sightings of Kipping have been hotly debated.

But now there’s hope on the horizon, with many new ways to explore these objects, from monitoring rogue planets that have abandoned their stars to monitoring exoplanets’ gravitational wobbles. Armed with these new technologies, and new telescopes also in development, the Moon will…

Source: www.newscientist.com

Bizarre White Dwarf Leaves Metallic Marks Following Consumption of Planet

Artist’s impression of WD 0816-310. Astronomers have discovered scars imprinted on the surface left when a star swallows a planet.

ESO/L. Calzada

Astronomers have discovered a white dwarf star with strange metallic scars on its surface. The scar likely formed when the star tore apart and ate a small planet in its orbit.

Researchers often find white dwarfs with traces of metal in their atmospheres that came from planets that fell into the star. It has long been thought that metals should be evenly distributed across the surfaces of these so-called contaminated white dwarfs; Jay Farihi Researchers at University College London have discovered a strange concentration of metal debris.

Researchers monitored the star, called WD 0816-310, for two months using the Very Large Telescope in Chile. They discovered that the white dwarf had an opaque piece of metal on top of one of its magnetic poles, blocking some of the star’s light as it rotated. This position indicates that material may have been funneled into the star by its magnetic field. “This is the same process that causes auroras on Earth: charged particles follow magnetic fields to the surface,” Farihi said.

The planet that WD 0816-310 destroyed was small, probably about the same size as the solar system’s asteroid Vesta, which is about 525 kilometers in diameter. Its interior is now prominently displayed on its host star, which could make it relatively easy to study what its geochemistry was like before it was engulfed. Such studies may even be one of the best ways to observe small worlds outside our solar system, even after they disappear.

And there may be many other stars that have been similarly damaged. “When we find something outlandish, it’s often because they all looked that way and we just weren’t asking the right questions,” Farihi says. “This is the first, but it probably won’t be the last.” In fact, researchers have already discovered two white dwarfs that appear to have similar scars. If we go back and observe similar stars over and over again, we may discover even more stars.

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Source: www.newscientist.com

Exploring a Hidden Deep-Sea Oasis: Witnessing the Birth of 20,000 Octopuses on Planet Earth 3

Its mauve, suction cup-covered arms gently unfold to grab an egg shaped like an elongated ping-pong ball. A jet of water from a siphon next to the octopus's head ensures that the unhatched cubs get enough oxygen.

From a distance, she is surrounded by hundreds of females, living up to her nickname. The pearl octopus (Muusoctopus robotus) resembles a spherical gem that sits on the ocean floor. This is the largest known assemblage of eight-armed molluscs on Earth, numbering approximately 20,000 individuals, and has been witnessed by people all over the world in astonishingly high resolution. “Oceans” episode BBC series Planet Earth III.

This view would have been amazing enough even if it were from shallow water, including tropical coral reefs and kelp forests. But these octopus mothers tend to their eggs in freezing cold and darkness, about 2 miles below the surface. of the deep sea.

“The fact that there is life there is amazing in itself,” says the producer and director. Will Ridgeon They spent two years photographing the octopus, collaborating with scientists and technicians at California's Monterey Bay Aquarium Research Institute (MBARI).

The aptly named pearl octopus rears its eggs in an octopus garden surrounded by flower-like anemones. – Credit: Monterey Bay Aquarium Research Institute

The octopus farm, as the site is now known, is located on a hill in the eastern Pacific Ocean, 160 km (100 miles) southwest of Monterey Bay, near a giant underwater mountain called Davidson Seamount. This place was discovered during his expedition in 2018. live streamed over the internet.

It was the first time I had ever seen so many creatures in one place, let alone in the deep sea. (Octopuses are notoriously solitary animals and tend to be cannibalistic when kept together in captivity.) ).

Ridgeon watched the livestream of the discovery and immediately knew it was a story to be filmed in a new BBC series.he teamed up with Dr. Jim Barrya senior scientist at MBARI, began regularly visiting octopus farms in 2019 to learn more about why so many octopuses congregate in certain areas.

“The question is, why is it there?” Barry says. Barry and his colleagues gathered specialized tools and began a series of detailed studies. They created a photomosaic of his 2.5-hectare (about 27,000 square feet2) portion of the property and stitched together high-resolution images that allowed them to count the octopus population.

They also installed time-lapse cameras on the ocean floor, taking close-up photos every 20 minutes at a time for months to show what the octopuses were doing, and Barry's team gradually expanded the octopus park's largest began to unravel some of the mysteries.

Octopus farm location. – Image credit: MBARI

work remotely

Ridgeon took part in an expedition to an octopus farm early on. Initially, filming took place during lockdown, so he participated via live video link from his bedroom in Bristol, England (with occasional interruptions from his five-year-old daughter).

Once COVID-19 restrictions allowed, Ridgeon joined Barry and his team aboard MBARI's vessel, the research vessel Western Flyer. However, no one visited the octopus farm directly. All surveys and filming were done using a car-sized remotely operated vehicle (ROV) equipped with a camera and a robotic arm.

The dive began around 6 a.m., and the ROV was lowered into the ocean through a hole in the Western Flyer's hull called the moonpool. “It's very James Bond,” Ridgeon says. The descent to the octopus garden can take up to two hours, and the ROV will remain there all day.

The pilot controls the ROV via a cable connected to a control room on the ship on the ground, and everyone watches the video feed to see what's happening below.

Researchers survey the octopus farm from the Western Flyer's ROV control room. – Credit: Monterey Bay Aquarium Research Institute

“You forget you're looking at a screen,” Ridgeon says. “You think you're there,” says the MBARI engineer. He worked with the BBC to find the ideal camera setup to photograph the octopus garden. It was not possible to use footage from a camera fixed to the ROV due to too much vibration.

“I think the BBC will do a little bit about that.” [shivering]“But not as much as we had,” Barry says. ROVs “shudder” not because of the cold temperatures of the deep ocean, but because the thrusters must be activated constantly to ensure they stay close to the ocean floor (ROVs are positively buoyant, so if they fail they will ). .

To get around this, Barry and Ridgeon used a separate 4K camera mounted on a specially designed stand that could be placed on the ocean floor.

“I think that's the secret behind the images,” Ridgeon says. Unlike the ROV cameras used by scientists, which can only reach within a few meters of objects on the ocean floor, the 4K camera's focal length of about 20 centimeters (7 to 8 inches) allows it to precisely navigate between octopuses. can be captured.

But it was difficult to use. It took up to 40 minutes to get into position, and the team had to hope it wouldn't fall over and the action would happen in front of it. Ridgeon operated the camera from the ship using his PlayStation controller, which MBARI engineers adapted for the job. “At first it's like trying to film him with his hands tied behind his back,” Ridgeon said.

Another challenge with deep-sea photography is light. “Put the light as far away from the camera as possible, ideally around the sides so it’s three-quarters backlit. [the scene]That way, there are no reflections from any debris in the water,” explains Ridgeon.

The octopus garden provides insight into the life and reproduction of molluscs. – Credit: Monterey Bay Aquarium Research Institute

Those “fragments” are marine snow. These are organic particles that constantly rain down from the shallow ocean above. Marine snow is made up of dead plankton and their feces stuck together by microbial glue, and is the main food source for deep-sea animals. However, it makes filming difficult as the movie can look like it was shot in a snowstorm.

To see through the snowstorm and achieve the desired three-quarters backlighting effect, the MBARI team built a lighting system that the ROV could hold on its side, away from the camera. “That's how we got some really great shots,” Barry says.

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Accelerate development

As Barry's investigation and BBC filming progressed, the team made some surprising discoveries. First, no medium-sized octopus ever visited this location, and there were no signs of it feeding. It was only a fully grown adult octopus.

They were here to breed and for no other purpose. It may be called an octopus farm, but this place is definitely an octopus farm. The researchers also collected evidence that incubating females use on-site hot springs to speed up the development of their offspring.

For octopuses, there is a strong relationship between temperature and hatching time. The colder it is, the longer it will take and the more dangerous it will be. This is because there are scavengers that prey on unborn, unprotected octopus eggs.

Temperature studies have shown that the seawater surrounding each octopus nest can reach 10°C (50°F), much warmer than the 1.6°C (34°F) seawater just a few meters away. It was shown. By observing specific octopuses (identifiable by scratch and scar patterns) in the field, Barry and his colleagues determined that their eggs take an average of 1.8 years to hatch.

During this time, the female does not move but is constantly fighting off predators and guarding her approximately 60 eggs. “Once you plant an egg on a rock, that's it. You can't leave that spot,” Barry says. At just under two years, it's not the longest parenting period for an octopus. This record is given to another species that other MBARI scientists discovered nearby, Graneledon boreopafica, clinging to the sides of Monterey She Canyon 1.4 km (just under a mile) deep. I did.

Researchers watched one female incubate her eggs for four and a half years, longer than any other recorded animal. However, she was growing her eggs in water that was much warmer than the octopus park's ambient temperature of 1.6 degrees Celsius. Without the hot springs, the eggs in the octopus garden would take more than 10 years to hatch. When this site was discovered, biologists were surprised to find octopuses nesting there.

But geologists were fascinated by warm water seeping through the ocean floor, something they had never seen before. These springs are much cooler than the red-hot hydrothermal vents that form at the edges of tectonic plates where new molten ocean floors are created.

Although the enormous pressure will not cause the water to boil, the temperature around the vent can reach hundreds of degrees. These were first discovered in his 1970s, and plumes of hydrothermal water rise up to hundreds of meters in the water column, making them relatively easy to detect with temperature probes. In contrast, hot springs are more difficult to find because they form away from these tectonically active regions and have much cooler temperatures.

But geologists believe they could exist in the thousands and are highly stable, likely remaining in the same location for hundreds or even thousands of years. Therefore, biologists believe that more octopus farms may be established around these springs.

birth and death

In the final scene of the “Octopus Garden” episode Planet Earth III, a cluster of tiny sucker-like arms appears beneath the brooding female, then a wobbling young octopus swims away into the darkness like a mini-umbrella. More chicks follow and begin life at sea.

No one knows where they're going…yet. “That's what I want to understand next,” Barry says. The hatchlings are large for a newborn octopus, at about 6 cm (2 inches), so they have the best chance of survival. But as anyone who has seen the Octopus documentary knows, this comes at a heavy cost to mothers.

“These mothers are trying so hard to protect their bloodlines, and they're just dying out,” Barry says. Her father died a few years ago, shortly after mating. On the screen, we see the women's eyes cloudy and their bodies wrinkled. Ridgeon saw what happened next, but she decided it was not suitable for an evening television audience.

Dead octopuses are quickly attacked by scavengers such as fish, snails, sea anemones, and shrimp. For Barry, this is another important part of his discovery at the octopus farm. The nesting season is asynchronous, with octopuses hatching and mothers dying throughout the year. Approximately 9 each day. The female octopus' body nourishes the rest of the ecosystem and helps supplement the energy input from marine snow by 72 percent.

Graneledon boreopafica (a species of octopus that incubates eggs in cold water) has a 4.5 year rearing period, which holds the record for the longest rearing period of any animal. – Credit: Alamy

“This is clearly a huge food subsidy for the local ecosystem,” Barry says. “That wouldn't happen in shallow water,” he added. Because there is a lot of food around. But in the more barren depths, nothing goes to waste.

The BBC has finished filming at the octopus farm, but Barry's research continues. One of the things he wants to know is the age of the sea anemone. These are giant orange flower-like animals that make the octopus garden look like a real garden.

Barry studies sea anemones, which live for decades in shallow coastal waters, and finds that deep-sea species can survive for centuries, in contrast to octopuses, which are relatively short-lived. That's what I'm thinking.

“They're like sentinels that just sit there while the octopus cycles,” he says. There are many more questions Barry would like to answer. “Are octopuses confined to this breeding form in warm areas, or are they able to breed elsewhere with cooler ambient temperatures? Is there fidelity to specific nest sites? ?Will they return to their place of birth?'' he asks.

No one knows how far the octopuses travel before they reach the garden or how they found them, but Barry said he was surprised by the large number of dead and dying octopuses floating around. I suspect I smelled it. “We'll definitely be back,” he says.

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Source: www.sciencefocus.com

Strange Alien Planet Indicates Earth’s Survival After Sun’s Demise

Mark Garlick/Science Photo Library

When I found out the date of the end of the Earth, everything seemed so simple. Five billion years from now, the solar system will have changed dramatically. Instead of the gentle presence we are accustomed to, the sun will become a behemoth, hundreds of times larger than it is today. In the process, it will wipe out the rocky inner planets, including our own.

Or will it be? We recently witnessed the death stages of another star for the first time. And miraculously, it seems some planets will be able to survive this apocalyptic era. Observations like these call into question the story of how the Earth will die, and give us hope that somehow the Earth may outlast the Sun. Even if it doesn’t, all is not lost. The study also provides clues as to where humans might best seek refuge.

How does the sun die?

The sun is powered by nuclear fusion. In nuclear fusion, hydrogen atoms fuse into helium, releasing a huge amount of energy in the process. However, the fate of our star is determined by one fact. This means that the supply of hydrogen is limited. As this energy begins to deplete, in about another 5 billion years, the Sun’s internal structure will change and it will expand to about 200 times its current size. It will change from the current yellow dwarf to a red giant. After another billion years, the star shrinks and expands again, before disappearing and becoming a stellar corpse called a white dwarf.

As it grows…

Source: www.newscientist.com

Astronomers make breakthrough discovery in planet formation, conflicting with theoretical predictions

Recent observations of the young star DG Taurus reveal a smooth protoplanetary disk in which no planets have yet formed, suggesting that it is on the brink of this process. The findings show unexpected dust grain growth patterns and provide new insights into the early stages of planet formation. Credit: SciTechDaily.com

Astronomers have become very good at finding signs of planet formation around stars. However, to fully understand planet formation, it is important to examine cases where this process has not yet begun.

Looking for something and not finding it can sometimes be even more difficult than finding it, but new detailed observations of the young star DG Taurus reveal that the planet is a smooth protoplanet with no signs of planet formation. It was shown that it has a system disk. This lack of detected planet formation may indicate that DG Taurus is on the eve of planet formation.

Image of radio radiation intensity from a disk near DG Taurus observed with ALMA. Rings have not yet formed within the disk, suggesting that planets are about to form.Credit: ALMA (ESO/National Astronomical Observatory/NRAO), S. Obashi et al.

Protoplanetary disk and planet growth

Planets form around protostars, which are young stars that are still forming, in disks of gas and dust known as protoplanetary disks. Planets grow so slowly that it is impossible to observe their evolution in situ. Therefore, astronomers observe many protostars at slightly different stages of planet formation to build theoretical understanding.

This time, an international research team led by Satoshi Ohashi of the National Astronomical Observatory of Japan (NAOJ) has developed the Atacama Large Millimeter/Submillimeter Array (alma telescope) will conduct high-resolution observations of the protoplanetary disk surrounding the relatively young protostar DG Taurus, located 410 light-years away in the direction of Taurus. The researchers found that DG Taurus has a smooth protoplanetary disk and no rings that would indicate planet formation. This led the research team to believe that the DG Taurus system could begin forming planets in the future.

Unexpected discoveries and future research

The researchers found that during this pre-planetary stage, dust particles are within 40 astronomical units (about twice the size of Earth’s orbit). Uranus The radius of the central protostar is still small, but beyond this radius the dust particles begin to grow, which is the first step in planet formation. This goes against the theoretical expectation that planet formation begins inside the disk.

These results provide surprising new information about dust distribution and other conditions at the beginning of planet formation. Studying more examples in the future will further deepen our understanding of planet formation.

Reference: “Dust concentration and particle growth in the smooth disk of a DG tau protostar revealed by ALMA triple-band frequency observations” Satoshi Ohashi, Munetake Momose, Akiraka Kataoka, Aya Higuchi E, Takashi Tsukagoshi, Takahiro Ueda, Claudio Codella, Linda Podio, Tomoyuki Hanawa, Nami Sakai, Hiroshi Kobayashi, Satoshi Okuzumi, Hidekazu Tanaka, August 28, 2023, of astrophysical journal.
DOI: 10.3847/1538-4357/ace9b9

This research was funded by the Japan Society for the Promotion of Science, the German Foundation, and the European Union.

Source: scitechdaily.com