More stories

  • in

    Could we grow endangered plants on other planets? No

    Josie Ford
    Solar system agronomy
    Could we grow endangered plants on other planets? We pause and consider this question. No.
    Still, since this query is the subject line of a PR email from an online flower-delivery service, handed to us by a colleague with a pair of tongs and a disparaging look, we find it worthy of further consideration. Even more so since we are promised conclusions reached “using research and working with a designer”.
    “Today, nearly 40% of the world’s plants are endangered, according to a report from the Royal Botanic Gardens, Kew,” we read. Sad, sad science fact. But never fear, once we have destroyed Earth’s ecosystems, a bright, green future exists elsewhere in the solar system, at least in the world of whirly-eyed PR.Advertisement
    “As the soil on Mars has double the amount of iron than soil on planet earth, leafy green vegetables and microgreens would easily thrive there,” we learn. Dandelions, too, apparently – a species far from endangered on Feedback’s small patch of terra firma. “Hops vine [sic], trees, shrubs and poison ivy might be able to survive the challenging temperatures on this moon”, it opines of Jupiter’s satellite Europa, where days struggle to rise above -135°C and surface radiation levels are around 2000 times those on Earth. “One of the only things that can kill poison ivy is boiling water – so the cold and wet conditions on Europa seem to be the ideal environment for this plant.”
    The outlook is even rosier on Titan, the Saturnian moon where water ice at around -180°C fulfils the function of bedrock, and great surface lakes are filled with liquid natural gas. “Titan’s surface is sculpted by methane and ethane, which only one other planet in the solar system has: Earth. Therefore, tobacco plants should grow on this moon too”, our correspondent concludes, non-sequentially.
    “Please let me know if you have any questions”, the email ends. So, so many, including where we get some of the wacky Europa baccy too. Optimism is a fine, fine thing, but as far as the future of life on Earth is concerned, we fear the rationalist’s counterstatement applies: il faut cultiver notre jardin.
    Bog standards
    “We are all in the gutter, but some of us are looking at the stars”, as one of the usual suspects once wrote. Or we are all in the gutter, sending in responses to our recent item on peculiar toilet signage (31 July).
    “Toilets and viewing area” was an unfortunate juxtaposition that confronted Richard Ellam at an Aberdeen Science Festival some years back, while Chris Evans relays that “A lay-by eatery near where I live (on the A59 between Skipton and Clitheroe) for some years displayed a sign reading ‘Sit-in or take-away toilet’” – neither of which seems particularly practicable or desirable.
    Hazardous fore play
    Our item on the newly introduced crocodile hazard at the Royal Port Moresby Golf Club in Papua New Guinea (14 August) reminds Stuart Reeves in Wake Forest, North Carolina, of playing at the Skukuza Golf Club in Kruger National Park in South Africa – a sentence that exhausts us even typing it.
    Its “local rules” include such gems as “Burrowing animals – Rough/Fairway drop without penalty from holes made by burrowing animals and termites, NOT HOOF MARKS. Burrowing animals include warthogs, moles and termites”.
    Other rules (“formal and informal”) that Stuart has encountered on his travels include “Give way to a herdsman and his cows crossing the fairway; free drop from a hippopotamus footprint; free drop about 3 club lengths if the ball lands in the coils of a snake (no need to be precise); if a monkey steals your ball it is a lost ball”. Strong stuff – and further congratulations on your self-confessed status as a “recovering golfer”.
    Transcendental number
    Mentions in Almost the last word (14 August) of “interesting numbers, numbers with their own Wiki page and the fine-structure constant (approximately 1/137) prompted me to recheck the Wiki page for 137″, writes Mike Sargent, displaying the talent for the tangent that we so admire among Feedback readers. “It has for several years now informed us that ‘Wolfgang Pauli, a pioneer of quantum physics, died in a hospital room numbered 137, a coincidence that disturbed him’.”
    “It is difficult to know which is more surprising, that Pauli’s consciousness transcended death, or that he then contrived to communicate his feelings on his demise to a Wiki page editor,” he continues. We don’t wish to sound too woo, but it is a fundamental tenet of quantum mechanics that information cannot be destroyed, and “Physics might create a backdoor to an afterlife – but don’t bank on it” is the headline of an article we see in our webspace starting from that basis. We would say that’s living proof, but that’s possibly not quite right.
    Last laugh
    Casting our all-seeing eye over our shoulder, we see that our neighbours and friends in Almost the last word (backwards readers: you’ll find it towards the front) are discussing how a photon “knows” to travel at the speed of light.
    With the privilege of having the actual last word, we must give the obvious missing answer: because it is very bright.
    Got a story for Feedback?Send it to feedback@newscientist.com or New Scientist, Northcliffe House, 2 Derry Street, London W8 5TTConsideration of items sent in the post will be delayed
    You can send stories to Feedback by email at feedback@newscientist.com. Please include your home address. This week’s and past Feedbacks can be seen on our website. More

  • in

    Star Trek Lower Decks review: Season 2 is a triumph

    By Swapna Krishna

    In Star Trek: Lower Decks, we see what life is like for low-ranking members of Starfleet2021 CBS Interactive, Inc.
    TV
    Star Trek: Lower Decks
    Amazon Prime Video

    WHEN Star Trek: Lower Decks first premiered in the US last August, it presented a perspective we had rarely seen within the Star Trek universe. While we had traditionally focused on the “upstairs” bridge crew boldly going where no one had gone before, Lower Decks turned its sharp eye towards the “downstairs”: the workers responsible for the least glamorous tasks on the ship. That it was … More

  • in

    Don't Miss: Netflix follows the all-civilian crew of a SpaceX mission

    John Kraus/Courtesy of Netflix
    Watch
    Countdown: Inspiration4 mission to space follows the first all-civilian crew of a SpaceX Dragon. Their three days in orbit later this year will raise funds for a children’s research hospital. On Netflix from 6 September.

    Read
    Five Minds, a speculative thriller by Guy Morpuss, is set in a future where, to solve the planet’s population problem, human bodies play host to multiple minds. But what if you might be sharing a body with a murderer?

    Read
    What’s Eating the Universe? wonders physicist Paul Davies, as he … More

  • in

    The Forgotten City review: It's fun being stuck in a Roman time-loop

    By Jacob Aron

    Don’t break the Golden Rule otherwise statues will come after youDear Villagers
    Game
    The Forgotten City
    Modern Storyteller Multiple consolesAdvertisement

    IF YOU could live today again, would you do anything differently? This theme has been explored in everything from films like Edge of Tomorrow to pretty much every sci-fi TV show of the 1990s looking to produce an episode on the cheap, but time loops are rarer in video games.
    At first, that might seem strange – unlike a film, a time loop running on a computer can be instantly reset, making them easy to produce – until you realise that the best examples of the genre (Groundhog Day, obviously) make heavy use of cuts and rely on the viewer to fill in the repetitive details. That is harder to do in a game, where players are responsible for all of the protagonist’s actions.
    The Forgotten City has a neat solution to this problem, which I will get to in a moment. The game sees you thrown back 2000 years to an underground Roman settlement, where you must attempt to solve a mystery in order to free yourself from living the same day over and over. Only then can you return to your own time.
    The titular city has one very simple law, the Golden Rule: if anyone commits a sin, everyone is punished. Exactly what counts as a sin is one of the themes explored in the game, as no one in the city is exactly sure. All they know is that if someone breaks this rule, the golden statues that are littered all over the place will come to life, attacking everyone they see and turning them into gold.
    “By exploring the consequences of an all-seeing authority, the game critiques modern surveillance systems”
    Thanks to the time loop, you are able to escape this fate – and more importantly, keep any items you have picked up, along with any knowledge of what has happened before.
    This makes for some fun puzzles to solve. Some are simple – can’t get inside a locked door? Steal the key, reset the loop and let yourself in. Some are more complex, such as a woman who seems to have been poisoned, and is about to die, without anyone breaking the Golden Rule.
    Thankfully, once you have solved a puzzle, you don’t have to do it again the next loop around. The first person you meet at the start of every loop, Galerius, will happily, if slightly bewilderedly, follow your instructions to complete tasks on your behalf.
    This frees you up to delve further into the plot, which had me hooked. Although set in ancient Rome, the game serves as a criticism of the panopticon concept invented by 18th-century philosopher Jeremy Bentham, who designed a prison in which everyone could be watched from one location, with the intention being they would be on their best behaviour. By exploring the consequences of an all-seeing authority, it also critiques modern surveillance systems.
    One slight disappointment is that the time loop in the game is a bit of a cheat – certain events trigger not at particular times each day, but when you approach a specific location – but I can forgive that.
    These days, most video games are created by vast armies of developers operating in teams around the globe, so I was impressed to learn that The Forgotten City was mainly the work of just three people. They have cleverly worked within those limitations – the city you explore is more of a large town, and only hosts a couple of dozen people, while the time loop allows for scenes to be reused without feeling cheap – to create something that really shines.
    Jacob also recommends…
    Games
    The Legend of Zelda: Majora’s Mask
    Nintendo
    The definitive time-loop video game, in which hero Link has just three days to prevent the moon (which has an evil-looking face!) crashing into the planet.
    The Sexy Brutale
    Cavalier Game Studios
    Another time-loop mystery, set in an Agatha Christie-like mansion whose inhabitants are all murdered over a 12-hour period.

    More on these topics: More

  • in

    7200-year-old DNA suggests Denisovans bred with humans on Sulawesi

    By Michael Marshall

    Fragments of a human skull found on the island of Sulawesi in IndonesiaUniversity of Hasanuddin
    For the first time, DNA has been obtained from the bones of a Stone Age person who lived on the Indonesian island of Sulawesi. The genetic information sheds light on the prehistory of the South-East Asian islands – including what happened when our species, Homo sapiens, first reached the area.
    Sulawesi is one of the largest islands in South-East Asia, the region between the Asian mainland and Australia. On the island’s South Peninsula, researchers have excavated a cave called … More

  • in

    The definition of planet is still a sore point – especially among Pluto fans

    For 76 years, Pluto was the beloved ninth planet. No one cared that it was the runt of the solar system, with a moon, Charon, half its size. No one minded that it had a tilted, eccentric orbit. Pluto was a weirdo, but it was our weirdo.

    “Children identify with its smallness,” wrote science writer Dava Sobel in her 2005 book The Planets. “Adults relate to its inadequacy, its marginal existence as a misfit.”

    When Pluto was excluded from the planetary display in 2000 at the American Museum of Natural History in New York City, children sent hate mail to Neil deGrasse Tyson, director of the museum’s planetarium. Likewise, there was a popular uproar when 15 years ago, in August 2006, the International Astronomical Union, or IAU, wrote a new definition of “planet” that left Pluto out. The new definition required that a body 1) orbit the sun, 2) have enough mass to be spherical (or close) and 3) have cleared the neighborhood around its orbit of other bodies. Objects that meet the first two criteria but not the third, like Pluto, were designated “dwarf planets.”

    Science is not sentimental. It doesn’t care what you’re fond of, or what mnemonic you learned in elementary school. Science appeared to have won the day. Scientists learned more about the solar system and revised their views accordingly.

    “I believe that the decision taken was the correct one,” says astronomer Catherine Cesarsky of CEA Saclay in France, who was president of the IAU in 2006. “Pluto is very different from the eight solar system planets, and it would have been very difficult to keep changing the number of solar system planets as more massive [objects beyond Neptune] were being discovered. The intention was not at all to demote Pluto, but on the contrary to promote it as [a] prototype of a new class of solar system objects, of great importance and interest.”

    Sign Up For the Latest from Science News

    Headlines and summaries of the latest Science News articles, delivered to your inbox

    Thank you for signing up!
    There was a problem signing you up.

    For a long time, I shared this view. I’ve been writing about Pluto since my very first newspaper gig at the Cornell Daily Sun, when I was a junior in college in 2006. I interviewed some of my professors about the IAU’s decision. One, planetary scientist Jean-Luc Margot, who is now at UCLA, called it “a triumph of science over emotion. Science is all about recognizing that earlier ideas may have been wrong,” he said at the time. “Pluto is finally where it belongs.”

    But another, planetary scientist Jim Bell, now at Arizona State University in Tempe, thought the decision was a travesty. He still does. The idea that planets have to clear their orbits is particularly irksome, he says. The ability to collect or cast out all that debris doesn’t just depend on the body itself.

    Everything with interesting geology should be a planet, Bell told me recently. “I’m a lumper, not a splitter,” he says. “It doesn’t matter where you are, it matters what you are.”

    Not everyone agrees with him. “Fifteen years ago we finally got it right,” says planetary scientist Mike Brown of Caltech, who uses the Twitter handle @plutokiller because his research helped knock Pluto out of the planetary pantheon. “Pluto had been wrong all along.”

    But since 2006, we’ve learned that Pluto has an atmosphere and maybe even clouds. It has mountains made of water ice, fields of frozen nitrogen, methane snow–capped peaks, and dunes and volcanoes. “It’s a dynamic, complex world unlike any other orbiting the sun,” journalist Christopher Crockett wrote in Science News in 2015 when NASA’s New Horizons spacecraft flew by Pluto.

    Observations from NASA’s New Horizons mission showed that the surface of Pluto’s Sputnik Planitia region is covered in churning nitrogen ice “cells” (white polygonal blocks) that constantly bring fresh material up to the surface from below.JHU-APL, NASA, SWRI

    Closer views highlight the rugged water-ice mountains that border some of these cells.JHU-APL, NASA, SWRI

    The New Horizons mission showed that Pluto has fascinating and active geology to rival that of any rocky world in the inner solar system. And that solidified planetary scientist Philip Metzger’s view that the IAU definition missed the mark.

    “There was an immediate reaction against the dumb definition” when it was proposed, says Metzger, of the University of Central Florida in Orlando. Since then, he and colleagues have been refining their views: “Why do we have this intuition that says that it’s dumb?”

    Retelling the tale

    It turns out that the “we just learned more” narrative isn’t really true, Metzger says. Though the official story is that Pluto was reclassified because new data came in, it’s not that simple. Teaching that narrative is bad for science, and for science education, he says.

    The truth is, there’s no single definition of a planet — and I’m beginning to believe that’s a good thing.

    For centuries, the word “planet” was a much more inclusive term. When Galileo turned his telescope at Jupiter, any largish moving body in the sky was considered a planet — including moons. When astronomers discovered the rocky bodies we now call asteroids in the 1800s, those too were called planets, at least at first.

    Pluto was considered a planet from the very beginning. When Clyde Tombaugh, an amateur astronomer from Kansas newly recruited to the Lowell Observatory in Flagstaff, Ariz., spotted it in photos taken in January 1930, he rushed to the observatory director and declared: “I have found your Planet X.”

    Clyde Tombaugh, shown here with a homemade telescope, discovered Pluto in 1930 when he was 24 years old.GL Archive/Alamy Stock Photo

    The discovery was no accident. In 1903, U.S. astronomer Percival Lowell hypothesized that a hidden planet seven times the mass of Earth orbited 45 times farther from the sun. Lowell had searched for what he called Planet X until he died in 1916. The search continued without him.

    The new planet was thought to be “black as coal, nearly as dense as iron, twice as dense as the heaviest earthly surface rocks,” Science News Letter, the predecessor of Science News, reported in 1930.

    Further research showed Lowell had grossly overestimated Pluto’s mass: It’s more like one five-hundredth the mass of Earth. Things got even weirder when scientists realized Pluto wasn’t alone out there. In 1992, an object about a tenth the diameter of Pluto was found orbiting the sun “in the deep freeze of space well beyond the orbits of Pluto and Neptune,” as Science News described it.

    Since then, more than 2,000 icy bodies have been found hiding in that frigid zone dubbed the Kuiper Belt, and there are many more out there. Awareness of Pluto’s neighbors brought new questions: What characteristics could unite these strange new worlds with the more familiar ones? And what sets them apart? With so many new objects coming into focus, there was a growing desire for a formal definition of “planet.”

    In 2005, Brown spotted the first of the Kuiper Belt bodies that seemed to be larger than Pluto. If Pluto was the ninth planet, then surely the new discovery, nicknamed Xena (in honor of the TV show Xena: Warrior Princess), should be the 10th. But if Xena was an icy leftover from the formation of the solar system undeserving of the “planet” title, so too was Pluto.

    Tensions over how to categorize Pluto and Xena came to a head in 2006 at a meeting in Prague of the IAU. On the final day, August 24, after much acrimonious debate, a new definition of “planet” was put to a vote. Pluto and Xena got the boot. Xena was aptly renamed Eris, the Greek goddess of discord.

    On August 24, 2006, in Prague, members of the International Astronomical Union voted for a new definition of planet that redesignated Pluto and its neighbor Eris as dwarf planets, shrinking the total number of planets in the solar system to eight.Michal Cizek/AFP/Getty Images

    Textbooks were revised, posters were reprinted, but many planetary scientists, especially those who study Pluto, never bothered to change. “Planetary scientists don’t use the IAU’s definition in publishing papers,” Metzger says. “We pretty much just ignore it.”

    In part that might be cheek, or spite. But Metzger and colleagues think there’s good reason to reject the definition. Metzger, Bell and others — including Alan Stern of the Southwest Research Institute, the planetary scientist who led the New Horizons mission and has argued since before the discovery of the Kuiper Belt that the solar system contains hundreds of “planets” — make their case in a pair of recent papers, one published in 2019 in Icarus and one forthcoming.

    After examining hundreds of scientific papers, textbooks and letters dating back centuries, the researchers show that the way scientists and the public have used the word “planet” has changed over time, but not in the way most people think.

    In and out

    Consider Ceres, the first of what are now known as dwarf planets to be discovered. Located in the asteroid belt between Mars and Jupiter, Ceres was considered a planet after its 1801 discovery, too. It’s often said that Ceres was demoted after astronomers found the rest of the bodies in the asteroid belt. By the end of the 1800s, with hundreds of asteroids piling up, Ceres was stripped of its planetary title thanks to its neighbors. In that sense, the story goes, Ceres and Pluto suffered the same fate.

    But that’s not the real story, Metzger and colleagues found. Ceres and other asteroids were considered planets, sometimes dubbed “minor planets,” well into the 20th century. A 1951 article in Science News Letter declared that “thousands of planets are known to circle our sun,” although most are “small fry.” These “baby planets” can be as small as a city block or as wide as Pennsylvania.

    The dwarf planet Ceres orbits in the asteroid belt. It was also once considered a planet. NASA’s Dawn mission visited the dwarf planet in 2015 and found that it is also a geologically interesting world.JPL-Caltech, NASA, UCLA, MPS, DLR, IDA

    It wasn’t until the 1960s, when spacecraft offered better observations of these bodies, that the term “minor planets” fell out of fashion. While the largest asteroids still looked planetlike, most small asteroids turned out to be lumpy and irregular in shape, suggesting a different origin or different geophysics than bigger, rounder planets. The fact that asteroids didn’t “clear their orbits” had nothing to do with the name change, Metzger argues.

    And what about moons? Scientists called them “planets” or “secondary planets” until the 1920s. Surprisingly, it was nonscientific publications, notably astrological almanacs that used the positions of celestial bodies for horoscope readings, that insisted on the simplicity of a limited number of planets moving through the fixed sphere of stars.

    Metzger thinks that older definition of a planet that included moons was forgotten when planetary science went through a “Great Depression” between about 1910 and 1950. So many asteroids had been discovered that searching for new ones or refining their orbits was getting boring. Telescopes weren’t good enough to start exploring asteroids’ geology yet. Other parts of space science were way more exciting, so attention went there.

    But new data that came with space travel brought moons back into the planetary fold. Starting in the 1960s, “planet” reappeared in the scientific literature as a description for satellites, at least the large, round ones.

    Real-world usage

    The planet definition that includes certain moons, asteroids and Kuiper Belt objects has had staying power because it’s useful, Metzger says. Planetary scientists’ work includes comparing a place like Mars (a planet) to Titan (a moon) to Triton (a moon that was probably born in the Kuiper Belt and captured by Neptune long ago) to Pluto (a dwarf planet). It’s scientifically useful to have a word to describe the cosmic bodies where interesting geophysics, including the conditions that enable life, occur, he says. There’s all sorts of extra complexity, from mountains to atmospheres to oceans and rivers, when rocky worlds grow big enough for their own gravity to make them spherical.

    Pluto and hundreds or thousands of other objects that rival Pluto in size and interest orbit in the icy back of the solar system’s fridge, called the Kuiper Belt (white fuzzy ring).NASA

    “We’re not claiming that we have the perfect definition of a planet and that all scientists ought to adopt our definition,” he adds. That’s the same mistake the IAU made. “We’re saying this is something that ought to be debated.”

    A more inclusive definition of “planet” would also give a more accurate concept of what the solar system is. Emphasizing the eight major planets suggests that they dominate the solar system, when in fact the smaller stuff outnumbers those worlds tremendously. The major planets don’t even stay put in their orbits over long time-scales. The gas giants have shuffled around in the past. Teaching the view of the solar system that includes just eight static planets doesn’t do that dynamism justice.

    Caltech’s Brown disagrees. Having the gravitational oomph to nudge other bodies in and out of line is an important feature of a world, he says. Plus, the eight planets clearly dominate our solar system, he says. “If you dropped me in the solar system for the first time, and I looked around and saw what was there, nobody would say anything other than, ‘Wow, there are these eight — choose your word — and a lot of other little things.’ ”

    Pluto rises above the horizon of its largest moon, Charon, in this illustration.Mark Garlick/Science Photo Library/GettyImages Plus

    Thinking of planets that way leads to big-picture questions about how the solar system put itself together.

    One common argument in favor of the IAU’s definition is that it keeps the number of planets manageable. Can you imagine if there were hundreds or thousands of planets? How would the average person keep track of them all? What would we print on lunch boxes? I’m not making fun of this idea; as an astronomy writer who has been obsessed with space since I was 8, I would be reluctant to turn people off to the planets.

    But Metzger thinks teaching just eight planets risks turning people off to all the rest of space. “Back in the early 2000s, there was a lot of excitement when astronomers were discovering new planets in our solar system,” he says. “All that excitement ended in 2006.” But those objects are still out there and are still worthy of interest. By now, there are at least 150 of these dwarf planets, and most people have no clue, he says.

    This is the argument I find most compelling. Why do we need to limit the number of planets? Kids can memorize the names and characteristics of hundreds of dinosaurs, or Pokémon, for that matter. Why not encourage that for planets? Why not inspire students to rediscover and explore the space objects that most appeal to them?

    I’ve come to think that what makes a planet may just be in the eye of the beholders. I may be a lumper, not a splitter, too.

    [embedded content]
    Pluto continues to charm us all, as shown in these 2015 interviews after New Horizons sent its images of the geologic richness of the dwarf planet. More

  • in

    Here’s how cool a star can be and still achieve lasting success

    If you want to be a successful star by making the minimum possible effort, aim for a surface temperature about a quarter of the sun’s. This is the temperature that a new study says separates red dwarf stars, which shine for a long time, from failed stars known as brown dwarfs.

    It’s often hard to distinguish between red and brown dwarfs, because when young they both look the same: red and dim. But only red dwarfs are born with enough mass to sustain the same nuclear reactions that power stars like the sun. In contrast, brown dwarfs glow red primarily from the heat of their birth, but then their nuclear activity sputters out, causing them to cool and fade. Now astrophysicists Dino Hsu and Adam Burgasser at the University of California, San Diego and their colleagues have discerned the dividing line between the two types by exploiting how they move through space.

    When a star is born, it revolves around the Milky Way’s center on a fairly circular orbit. Over time, though, gravitational tugs from giant gas clouds, spiral arms and other stars toss the stars to and fro. These perturbations make the stars’ orbits around the galactic center more and more elliptical. Thus, the orbital paths of stars can reveal their approximate age.

    Most red dwarfs are fairly old; their predicted lifetimes are far longer than the current age of the universe. But because brown dwarfs cool and fade, any that are still warm are young. Thus, on average, red dwarfs should follow more elliptical orbits around the galaxy than young brown dwarfs do.

    Sign Up For the Latest from Science News

    Headlines and summaries of the latest Science News articles, delivered to your inbox

    Thank you for signing up!
    There was a problem signing you up.

    In the new study, Hsu’s team analyzed 172 red and brown dwarfs of different spectral types, classifications based on the objects’ spectra that correlate with their surface temperatures. The researchers found that a sharp break in stellar motions separates warmer objects, which on average have more elliptical orbits and are older, from cooler ones, which on average have more circular orbits and are younger. This break appears at a spectral type between L4 and L6, corresponding to a surface temperature of about 1200° to 1400° Celsius (1,500 to 1,700 kelvins) — a fraction of the sun’s surface temperature of about 5500°C (5,800 K) — the team reports July 5 at arXiv.org.

    Above this critical temperature, the dim suns are a mix of long-lived red dwarfs and young brown dwarfs. Below this temperature, though, “it’s all brown dwarfs,” Hsu says. These are the failed stars that are fated to fizzle out. The study will appear in a future issue of the Astrophysical Journal Supplement Series.

    This new method for detecting the temperature boundary between red and brown dwarfs is intriguing, but the result is tentative, says Trent Dupuy, an astronomer at the University of Edinburgh who was not involved in the work. “It’s right around where you would expect,” he says. Dupuy says additional red and brown dwarfs should be observed to verify the finding.

    Hsu agrees: “We need a more complete sample.” Expanding the sample will be both easy and hard. On the positive side, red dwarfs abound, outnumbering all other stellar types put together, and brown dwarfs are also common. On the negative side, though, red and brown dwarfs are faint. That makes measuring their Doppler shifts, which reveal how fast the objects move toward or away from Earth, a challenge. But knowing this motion is essential for calculating a star’s orbital path around the galaxy. More

  • in

    Modern humans evolved not to swing our hips as much as chimpanzees

    By Michael Marshall

    Based on the average height of humans, we should have longer stridesJohnnyGreig/Getty Images
    Humans have lost their swing. Chimpanzees and other great apes swing their hips when they walk, but modern humans do not. This means our strides are shorter than those of chimpanzees, even though our legs are proportionally longer.
    “We’ve always had this idea that evolution has been acting on fossil humans to make strides longer and longer,” says Nathan Thompson at the New York Institute of Technology in the US. But in fact, he says, “humans right … More