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    Don't Miss: Find out about the handshake, humanity's oldest greeting

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    The Handshake is over 7 million years old, says palaeoanthropologist, explorer and comic Ella Al-Shamahi. She will explain the secrets of this most ancient and universal greeting at the Royal Institution, London, at 7pm BST on 21 July.

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    Why Sharks Matter to us, the oceans and the marine economy is a subject of concern for David Shiffman, at the University of Arizona. Saving the imperilled predator will require a serious rethink of its image. Available to buy in the UK from 19 July.
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    The Future of Ageing makes the case … More

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    The most distant rotating galaxy hails from 13.3 billion years ago

    There is a galaxy spinning like a record in the early universe — far earlier than any others have been seen twirling around.  

    Astronomers have spotted signs of rotation in the galaxy MACS1149-JD1, JD1 for short, which sits so far away that its light takes 13.3 billion years to reach Earth. “The galaxy we analyzed, JD1, is the most distant example of a rotational galaxy,” says astronomer Akio Inoue of Waseda University in Tokyo.

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    “The origin of the rotational motion in galaxies is closely related to a question: how galaxies like the Milky Way formed,” Inoue says. “So, it is interesting to find the onset of rotation in the early universe.”

    JD1 was discovered in 2012. Due to its great distance from Earth, its light had been stretched, or redshifted, into longer wavelengths, thanks to the expansion of the universe. That redshifted light revealed that JD1 existed just 500 million years after the Big Bang.

    Astronomers used light from the entire galaxy to make that measurement. Now, using the Atacama Large Millimeter/submillimeter Array in Chile for about two months in 2018, Inoue and colleagues have measured more subtle differences in how that light is shifted across the galaxy’s disk. The new data show that, while all of JD1 is moving away from Earth, its northern part is moving away slower than the southern part. That’s a sign of rotation, the researchers report in the July 1 Astrophysical Journal Letters.

    JD1 spins at about 180,000 kilometers per hour, roughly a quarter the spin speed of the Milky Way. The galaxy is also smaller than modern spiral galaxies. So JD1 may be just starting to spin, Inoue says.

    The James Webb Space Telescope will observe JD1 in the next year to reveal more clues to how that galaxy, and others like ours, formed (SN: 10/6/21). More

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    Here are the James Webb Space Telescope’s stunning first pictures

    We’ve now seen farther, deeper and more clearly into space than ever before.

    A stellar birthplace, a nebula surrounding a dying star, a group of closely interacting galaxies, the first spectrum of an exoplanet’s light. These are some of the first images from the James Webb Space Telescope, released in a NASA news briefing on July 12. This quartet of cosmic scenes follows on the heels of the very first image released from the telescope, a vista of thousands of distant galaxies, presented in a White House briefing on July 11.   

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    “First of all, it’s really gorgeous. And it’s teeming with galaxies,” said JWST Operations Scientist Jane Rigby at the July 12 briefing. “That’s been true of every image we’ve taken with Webb. We can’t take [an image of] blank sky. Everywhere we look, there’s galaxies everywhere.”

    Going deep

    The galaxies captured in the first released image lie behind a cluster of galaxies about 4.6 billion light-years away. The mass from those closer galaxies distorts spacetime in such a way that objects behind the cluster are magnified, giving astronomers a way to peer more than 13 billion years into the early universe.

    Even with that celestial assist, other existing telescopes could never see so far.  But the James Webb Space Telescope, also known as JWST, is incredibly large — at 6.5 meters across, its mirror is nearly three times as wide as that of the Hubble Space Telescope. It also sees in the infrared wavelengths of light where distant galaxies appear. Those features give it an edge over previous observatories.

    “There’s a sharpness and a clarity we’ve never had,” said Rigby, of NASA’s Goddard Space Flight Center in Greenbelt, Md. “You can really zoom in and play around.”

    This composite of images, revealing thousands of galaxies, is the deepest view of the universe ever captured — a record astronomers don’t expect to last long.NASA, ESA, CSA, STScI

    Although that first image represents the deepest view of the cosmos to date, “this is not a record that will stand for very long,” astronomer Klaus Pontoppidan of the Space Telescope Science Institute in Baltimore said in a June 29 news briefing. “Scientists will very quickly beat that record and go even deeper.”

    But JWST wasn’t built only to peer deeper and farther back in time than ever before. The cache of first images and data showcases space scenes both near and far, glimpses of single stars and entire galaxies, and even a peek into the chemical composition of a far-off planet’s atmosphere. 

    “These are pictures just taken over a period of five days. Every five days, we’re getting more data,” European Space Agency science advisor Mark McCaughrean said at the July 12 briefing. (JWST is an international collaboration among NASA, ESA and the Canadian Space Agency.) “It’s a culmination of decades of work, but it’s just the beginning of decades. What we’ve seen today with these images is essentially that we’re ready now.”

    This Hubble Space Telescope image of the galaxy cluster SMACS 0723 shows the same spot of sky as the JWST image above. The visible galaxies are fewer and not as far away.NASA, ESA, HST/STScI/AURA

    Cosmic cliffs

    This image shows the “Cosmic Cliffs,” part of the enormous Carina nebula, a region about 7,600 light-years from Earth where many massive stars are being born. Some of the most famous Hubble Space Telescope images feature this nebula in visible light, but JWST shows it in “infrared fireworks,” Pontoppidan says. JWST’s infrared detectors can see through dust, so the nebula appears especially spangled with stars. 

    Newborn stars sculpt the gas and dust around them in this JWST image of the Cosmic Cliffs in the Carina nebula, a star-forming region in the Milky Way galaxy.NASA, ESA, CSA, STScI

    “We’re seeing brand new stars that were previously completely hidden from our view,” said NASA Goddard astrophysicist Amber Straughn.

    But molecules in the dust itself are glowing too. Energetic winds from baby stars in the top of the image are pushing and sculpting the wall of gas and dust that runs across the middle. “We see examples of bubbles and cavities and jets that are being blown out from newborn stars,” Straughn said. And gas and dust are the raw material for new stars — and new planets.

    “It reminds me that our sun and our planets, and ultimately us, were formed out of this same stuff that we see here,” Straughn said. “We humans really are connected to the universe. We’re made out of the same stuff.”

    This view of young stars sculpting the gas and dust around them in the Carina nebula was captured by the Hubble space telescope in 2010.NASA, ESA, Mario Livio and Hubble 20th Anniversary Team/STScI

    Foamy nebula 

    The Southern Ring nebula is an expanding cloud of gas that surrounds a dying star about 2,000 light-years from Earth. In previous Hubble images, the nebula looks like an oblong swimming pool with a fuzzy orange deck and a bright diamond, a white dwarf star, in the middle. JWST expands the view far beyond that, showing more tendrils and structures in the gas than previous telescopes could see.

    JWST captured an image of the Southern Ring nebula in near-infrared (left) and mid-infrared (right) light, highlighting wispy structures at the nebula’s edge and revealing a second star in the middle.NASA, ESA, CSA, STScI

    “You see this bubbly, almost foamy appearance,” said JWST astronomer Karl Gordon, of the Space Telescope Science Institute. In the left hand image, which captures near-infrared light from JWST’s NIRCam instrument, the foaminess traces molecular hydrogen that formed as dust expanded away from the center. The center appears blue due to hot ionized gas heated by the leftover core of the star. Rays of light escape the nebula like the sun peeking through patchy clouds.

    In the right-hand image, taken by the MIRI mid-infrared camera, the outer rings look blue and trace hydrocarbons forming on the surface of dust grains. The MIRI image also reveals a second star in the nebula’s core.

    “We knew this was a binary star, but we didn’t see much of the actual star that produced this nebula,” Gordon said. “Now in MIRI this star glows red.”

    Hubble took this image of the Southern Ring nebula, a cloud of gas fleeing a dying star, in 2008.NASA, The Hubble Heritage Team/STScI/AURA/NASA

    A galactic quintet 

    Stephan’s Quintet is a group of galaxies about 290 million light-years away that was discovered in 1877. Four of the galaxies are engaged in an intimate gravitational dance, with one member of the group passing through the core of the cluster. (The fifth galaxy is actually much closer to Earth and just appears in a similar spot on the sky.) JWST’s images show off more structure within the galaxies than previous observations did, revealing where stars are being born.

    This composite image of Stephan’s Quintet shows five galaxies in mid- and near-infrared light. Four of the galaxies are bound by each others’ gravity in an endless looping dance. The fifth, the large galaxy to the left, is in the foreground, much closer to Earth than the other four. NASA, ESA, CSA, STScI

    “This is a very important image and area to study,” because it shows the sort of interactions that drive the evolution of galaxies, said JWST scientist Giovanna Giardino of the European Space Agency.

    In an image from the MIRI instrument alone, the galaxies look like wispy skeletons reaching towards each other. Two galaxies are clearly close to merging. And in the top galaxy, evidence of a supermassive black hole comes to light. Material swirling around the black hole is heated to extremely high temperatures and glows in infrared light as it falls into the black hole.

    This Hubble space telescope image of the five galaxies that make up Stephan’s Quintet was released in 2018.G. Bacon, J. DePasquale, F. Summers and Z. Levay/STScI, NASA, ESA

    An exoplanet’s sky

    This “image” is clearly different from the others, but it’s no less scientifically exciting. It shows the spectrum of light from the star WASP 96 as it passes through the atmosphere of its gas giant planet, WASP 96b. 

    “You get a bunch of what looks like bumps and wiggles to some people but it’s actually full of information content,” said NASA exoplanet scientist Knicole Colón. “You’re actually seeing bumps and wiggles that indicate the presence of water vapor in the atmosphere of this exoplanet.”

    The planet is about half the mass of Jupiter and orbits its star every 3.4 days. Previously astronomers thought it had no clouds in its sky, but the new data from JWST show signs of clouds and haze. “There is evidence of clouds and hazes because the water features are not quite as large as we predicted,” Colón said.

    Gas giant planet WASP 96b, shown in this artist’s illustration, orbits its star every 3.4 days.Engine House

    A long time coming

    These first images and data have been a very long time coming. The telescope that would become JWST was first dreamed up in the 1980s, and the planning and construction suffered years of budget issues and delays (SN: 10/6/21).

    The telescope finally launched on December 25. It then had to unfold and assemble itself in space, travel to a gravitationally stable spot about 1.5 million kilometers from Earth, align its insectlike primary mirror made of 18 hexagonal segments and calibrate its science instruments (SN: 1/24/22). There were hundreds of possible points of failure in that process, but the telescope unfurled successfully and got to work.

    “We are so thrilled that it works because there’s so much at risk,” says JWST senior project scientist John Mather of NASA’s Goddard Space Flight Center. “The world has trusted us to put our billions into this and make it go, and it works. So it’s an immense relief.”

    The James Webb Space Telescope (illustrated) spent months unfolding and calibrating its instruments after it launched on December 25. Adriana Manrique Gutierrez/CIL/GSFC/NASA

    In the months following, the telescope team released teasers of imagery from calibration, which already showed hundreds of distant, never-before-seen galaxies. But the images now being released are the first full-color pictures made from the data scientists will use to start unraveling mysteries of the universe.

    “It sees things that I never dreamed were out there,” Mather says.

    For the telescope team, the relief in finally seeing the first images was palpable. “It was like, ‘Oh my god, we made it!’” says image processor Alyssa Pagan, also of Space Telescope Science Institute. “It seems impossible. It’s like the impossible happened.”

    In light of the expected anticipation surrounding the first batch of images, the imaging team was sworn to secrecy.  “I couldn’t even share it with my wife,” says Pontoppidan, leader of the team that produced the first color science images.  

    “You’re looking at the deepest image of the universe yet, and you’re the only one who’s seen that,” he says, of the first picture released July 11. “It’s profoundly lonely.” Soon, though, the team of scientists, image processors and science writers was seeing something new every day for weeks as the telescope downloaded the first images. “It’s a crazy experience,” Pontoppidan says. “Once in a lifetime.”

    For Pagan, the timing is perfect. “It’s a very unifying thing,” she says. “The world is so polarized right now. I think it could use something that’s a little bit more universal and connecting. It’s a good perspective, to be reminded that we’re part of something so much greater and beautiful.” 

    JWST is just getting started as it now begins its first round of full science operations. “There’s lots more science to be done,” Mather says. “The mysteries of the universe will not come to an end anytime soon.”

    [embedded content]
    Exploded stars, colliding galaxies, and beautiful clouds feature in the first space photos released by The James Webb Space Telescope July 12.

    Asa Stahl contributed to this story.  More

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    Sand clouds are common in atmospheres of brown dwarfs

    Clouds of sand can condense, grow and disappear in some extraterrestrial atmospheres. A new look at old data shows that clouds made of hot silicate minerals are common in celestial objects known as brown dwarfs.

    “This is the first full contextual understanding of any cloud outside the solar system,” says astronomer Stanimir Metchev of the University of Western Ontario in London, Canada. Metchev’s colleague Genaro Suárez presented the new work July 4 at the Cool Stars meeting in Toulouse, France.

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    Clouds come in many flavors in our solar system, from Earth’s puffs of water vapor to Jupiter’s bands of ammonia. Astronomers have also inferred the presence of “extrasolar clouds” on planets outside the solar system (SN: 9/11/19).

    But the only extrasolar clouds that have been directly detected were in the skies of brown dwarfs — dim, ruddy orbs that are too large to be planets but too small and cool to be stars. In 2004, astronomers used NASA’s Spitzer Space Telescope to observe brown dwarfs and spotted spectral signatures of sand — more specifically, grains of silicate minerals such as quartz and olivine. A few more tentative examples of sand clouds were spotted in 2006 and 2008.

    Floating in one of these clouds would feel like being in a sandstorm, says planetary scientist Mark Marley of the University of Arizona in Tucson, who was involved in one of those early discoveries. “If you could take a scoop out of it and bring it home, you would have hot sand.”

    Astronomers at the time found six examples of these silicate clouds. “I kind of thought that was it,” Marley says. Theoretically, there should be a lot more than six brown dwarfs with sandy skies. But part of the Spitzer telescope ran out of coolant in 2009 and was no longer able to measure similar clouds’ chemistry.

    While Suárez was looking into archived Spitzer data for a different project, he realized there were unpublished or unanalyzed data on dozens of brown dwarfs. So he analyzed all of the low-mass stars and brown dwarfs that Spitzer had ever observed, 113 objects in total, 68 of which had never been published before, the team reports in the July Monthly Notices of the Royal Astronomical Society.

    “It’s very impressive to me that this was hiding in plain sight,” Marley says.

    Not every brown dwarf in the sample showed strong signs of silicate clouds. But together, the brown dwarfs followed a clear trend. For dwarfs and low-mass stars hotter than about 1700˚ Celsius, silicates exist as a vapor, and the objects show no signs of clouds. But below that temperature, signs of clouds start to appear, becoming thickest around 1300˚ C. Then the signal disappears for brown dwarfs that are cooler than about 1000˚ C, as the clouds sink deep into the atmospheres.

    The finding confirms previous suspicions that silicate clouds are widespread and reveals the conditions under which they form. Because brown dwarfs are born hot and cool down over time, most of them should see each phase of sand cloud evolution as they age. “We are learning how these brown dwarfs live,” Suárez says. Future research can extrapolate the results to better understand atmospheres in planets like Jupiter, he notes.

    The recently launched James Webb Space Telescope will also study atmospheric chemistry in exoplanets and brown dwarfs and will specifically look for clouds (SN: 10/6/21). Marley looks forward to combining the trends from this study with future results from JWST. “It’s really going to be a renaissance in brown dwarf science,” he says. More

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    How to make the best cup of cold-brew coffee

    Cold-brew coffee is on the rise. Enthusiasts say it has a smoother, less acidic taste and new research backs this up, finds Sam Wong, who takes his with ice and milk

    Humans

    6 July 2022

    By Sam Wong
    Jozef Polc/Alamy
    A GOOD cup of coffee is all about balance. Coffee contains more than 1000 flavour compounds, including some that provide the fruity, earthy and chocolatey aromas we detect in our noses and others responsible for the acidity, bitterness and astringency we detect in our mouths.
    The challenge is to extract a rich brew of desirable flavour compounds without overextracting those that make the drink bitter and overpowering. The roasting and grinding of the beans, the temperature of the water, the ratio of ground coffee to water and the time they are in contact all play a part, but different brewing … More

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    Stalking the Atomic City review: An extraordinary window on Chernobyl

    This vivid guide takes us into the exclusion zone around the nuclear power plant that exploded in 1986, revealing a “land of tranquillity and frozen time”

    Humans

    6 July 2022

    By George Bass

    BEFORE 26 April 1986, living near the Vladimir Lenin Nuclear Power Plant in the city of Chernobyl (nicknamed Atomic City) or in the nearby workers’ city of Prypyat was highly desirable. There was a new restaurant, supermarket, large playground and immaculate flats, all of which marked it out as one of the Soviet Union’s more prosperous areas. It was so desirable that newspapers ran adverts … More

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    Brian and Charles review: Can robots transform us, asks fantasy film

    A gentle fantasy about a lonely inventor called Brian, whose world changes completely when a robot he creates comes to life, makes a serious point about the possibilities of personal robots, finds Simon Ings

    Humans

    6 July 2022

    By Simon Ings

    Brian’s life changes after he sees a mannequin’s head in some rubbishCourtesy of Will Davie / Focus Features
    Brian and Charles
    Jim Archer
    On general release in US/UK cinemas

    AMATEUR inventor Brian Gittins has been having a bad time. He is terribly shy, lives alone and has become a favourite target of the local bully, Eddie Tomington (played by Jamie Michie).
    He finds consolation in his “inventions pantry” (“a cowshed, really”), from which emerges one ludicrously misconceived invention after another. His heart is in the right place: his tricycle-powered “flying cuckoo clock”, for instance, is meant as a service to … More

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    NFT fans fall for Snoop Dogg impersonator

    Feedback is our weekly column of bizarre stories, implausible advertising claims, confusing instructions and more

    Humans

    6 July 2022

    Josie Ford
    Should that be Beedfack?
    Feedback’s whirlwind romance with non-fungible tokens took another knock this week on learning that a celebrity impersonator called Doop Snogg and the man who hired him, Isaac Kamlish of NFT start-up Fair.xyz, arrived at a New York NFT festival to a blizzard of business cards hurled by star-struck CEOs who thought, against all available evidence, that Doop Snogg was the real Snoop Dogg.
    Was tulip mania ever this weird, Feedback wonders, putting our autograph book back in our pocket and heading for the West Coast and a bite to eat at NFT-themed burger restaurant Bored & … More