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Rare, dusty dying star shown in new JWST image

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Giant stars can be a prime example of the “live fast, die young” principle. Unlike our own Sun, which will shine for billions of years, more massive stars can burn off their fusion fuel in just a few million years before shedding their outer layers and exploding in supernovae.

NASA this week presented a rare image from the James Webb Space Telescope (JWST) of one of these stellar giants, Wolf-Rayet stars in the last, fleeting stages of their lives. Named WR 124, it lies in the constellation Sagittarius and lies about 15,000 light-years from Earth. The dying star has at least 30 times the mass of our Sun, but it is rapidly contracting, expelling hot gas into the cold vacuum of space.

“We caught it before,” explains Anthony Moffat, a retired astrophysicist who previously observed WR 124 with the Hubble Space Telescope and was not involved in the recent JWST measurements. Moffat has been studying Wolf-Rayet stars for decades. “This is the youngest person I know,” he says. The colorful cloud in the image, somewhat erroneously called a planetary nebula, is only a few thousand years old. Now, “the nebula is hugging the star,” he says. But as time passes, it will bloom outward in the form of expanding shells or rings of gas and dust.

Stars are natural fusion reactors, glowing with the energy released when hydrogen is fused to form helium atoms. Once massive stars burn off all their hydrogen, they begin to convert helium into heavier elements through a more energetic fusion reaction, causing powerful stellar winds. Rushing at speeds of more than 150,000 kilometers per hour, these winds carry the outer layers of the star with them, throwing huge volumes of gas and dust into space.

This gas glows with infrared radiation, the same type of light that JWST detects. Astrophysicists have created an impressive image by combining data from two JWST instruments, a near-infrared camera (NIRCam) and a mid-infrared (MIRI) instrument. The Hubble Space Telescope, which predominantly collects light in the optical range, has taken pictures of WR 124 before, but the JWST observations show the star’s growing nebula in stunning new detail.

“Personally, the most exciting part of this image is that we are capturing a rare phenomenon, i.e. a Wolf-Rayet star, at a level of detail that can only be achieved with JWST,” says Macarena Garcia Marin, an astrophysicist. The European Space Agency, which works with MIRI.

Only massive stars can go through the Wolf-Rayet phase, and not all of them. Astronomers have calculated that there are only 1,000 Wolf-Rayet stars in our galaxy—about one in every 100 million. The nearest one is about 1,000 light-years away in the star system Gamma Velorum, visible from the Southern Hemisphere. According to Moffat, Wolf-Rayet stars could be a million times brighter than the Sun. “What they lack in numbers, they make up for in light,” he adds.

“This dust is spreading into space and will eventually create planets. And that’s how we got here, really,” NASA astrophysicist Amber Strone said during a panel discussion at the 2023 South by Southwest conference in Austin, Texas, where the image was first unveiled. “I think this is one of the most beautiful concepts in all of astronomy.”

But while we are all made of stardust, there seems to be a lot more to the universe than scientists can explain with a simple cataloging of obvious sources. “It’s always exciting to be in science when our theories don’t match up with our observations — and that’s where we are right now with the dust,” Strawn says. These detailed pictures of the decoupling of a dying star as it forges heavy elements and produces copious amounts of dust could help scientists refine their understanding of this underlying process.

Someday—thousands or even millions of years from now, but essentially tomorrow on a galactic scale—WR 124 will explode in a spectacular supernova. In addition to a large amount of dust and heavy elements, a black hole may remain after the explosion. But physicists don’t have a good way to predict this with certainty. Moffat suggests that the supernova remnant could instead turn into a neutron star, the last stop before the collapsing star reaches the ultimate oblivion of a black hole. Without a glimpse from some observatory that remains for us in the distant future, we may never know what will happen to WR 124. But in any case, its ultimate fate remains the same, written in stars and planets that are still not formed from his generous gift of cosmic dust.

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Geometric deep optical sounding | The science

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The review discusses the latest developments in the field of optical sensing and imaging.

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A 7,000-year-old cult site in Saudi Arabia has been filled with human remains and animal bones.

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Archaeologists in Saudi Arabia have discovered ancient human remains buried alongside hundreds of scattered animal bones inside a 7,000-year-old desert monument, a ritual site used by a prehistoric cult.

The remains of an adult male around the age of 30 were found inside a mustatil, a structure whose name comes from the Arabic word for rectangle. The ruins are one of more than 1,600 mustatils discovered in Saudi Arabia since the 1970s. The structures, mostly buried in sand, were built when The Arabian desert was a lush meadow where elephants roamed and hippos bathed in lakes.

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Here’s the true story of a massive seaweed “drop” heading towards Florida.

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A free raft of kelp, about twice the width of the United States, is moving slowly across the Caribbean Sea. Currently, buckets of floating algae are washing up on Florida’s east coast beaches earlier than usual, raising scientists’ concerns about what the coming months will bring.

Seaweeds are made up of species of algae of the genus sargassum. These species grow as a mat of clumps of algae that are kept afloat by small air-filled sacs attached to leafy structures. The algae form a belt between the Caribbean Sea and West Africa in the Sargasso Sea in the North Atlantic Ocean and then drift westward with the currents. Scientists say reports of a huge algae crashing into the coastline are exaggerated because sargassum algae are scattered throughout the ocean, and most of the algae will never reach the sandy shores of the coast. But in recent years, researchers have routinely observed larger so-called sargassum blooms. And once the algae starts to wash up on the beaches and rot, it can cause serious problems, locals say.

Among the annual sargassum census in the Atlantic Ocean, “2018 was a record year and we’ve had some big years since then,” says Brian Lapointe, an oceanographer at Florida Atlantic University who has been studying seaweed for decades. “This is the new normal and we will have to adapt to it.”

The “droplet” of algae has been dubbed the Great Atlantic Sargassum Belt, and although it is spread out, the algae in the belt only covers about 0.1 percent of the water’s surface, says Chuangmin Hu, an oceanographer at the University of South Florida who used satellites to study sargassum for nearly 20 years.

Hu and colleagues use data collected by NASA satellites, including Terra and Aqua, to estimate the total mass sargassum in the Atlantic every month, tracking the annual cycle, which usually peaks in June. Last year, seaweed broke the record for the largest amount ever recorded in the Atlantic, with about 22 million metric tons of the substance found throughout the ocean, the team calculated.

Hu says the team has estimated that the Atlantic contains about six million metric tons. sargassum in February and that he is confident that the March mass will be higher. “There should be more this month. There is no doubt,” says Hu. “Even in the first two weeks, I saw an increase in numbers.”

In the ocean, Hu says sargassum is an important habitat for fish and turtles, among other marine life. He calls the belt a “moving ecosystem”. And only a small fraction of the algae present in the Atlantic will ever be washed up on beaches, Hu adds.

But beaches in Fort Lauderdale and the Florida Keys are already reporting sargassum Deposits this year, Lapointe says, and it’s on beaches that algae can be problematic. There, he says, the algae rots and releases chemicals like hydrogen sulfide gas that smells like rotten eggs. If inhaled, the gas can also cause headaches and irritate the eyes, nose, and throat. People with asthma or other breathing problems may be more sensitive to this effect. Florida Department of Health. The early appearance of algae is raising concerns about what this summer could bring.

“It’s pretty early sargassum season to see so much, so I think it’s also fueling some fears about what’s coming next,” says Lapointe.

Hu says that sargassum Volumes cannot be predicted more than two or three months in advance, so this summer’s seasonal peak is still too far away to predict. However, the researchers expected that this year could be rich in algae, because even during the winter calm there were more than average.

And the Atlantic reliably produced much more sargassum in recent decades than historically. Lapointe says it’s high sargassum Levels in recent years are likely due in part to nutrient-rich water flowing off land into rivers and oceans, where it can fertilize seaweed. But understanding and solving the problem remains confusing, he adds.

“This has been going on for over 10 years, and we haven’t made much progress in better understanding all of these factors that affect nutrients and climate,” he says. “That’s what we’re working on as scientists.”

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