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First Major Discoveries Reported From Project to Read Complete Genetic Sequences of All 70,000 Vertebrate Species

A bold project to read the complete genetic sequences of every known vertebrate species reaches its first milestone by publishing new methods and the first 25 high-quality genomes.

New DNA sequencing technologies and assembly methods let researchers read the entire genomes of 25 species: pale spear-nosed bat, greater horseshoe bat, Egyptian fruit bat, greater mouse-eared bat, Kuhl’s pipistrelle bat, velvety free-tailed bat, Canada lynx, marmoset, vaquita, platypus, echidna, zebra finch, kākāpō, Anna’s hummingbird, domestic duck, emu, Goode’s thornscrub tortoise, two-lined caecilian, zig-zag eel, climbing perch, flier cichlid, eastern happy cichlid, channel bull blenny, blunt-snouted clingfish, and thorny skate. The animals span all major classes of vertebrates. Credit: Irving Geis/HHMI

A bold project to read the complete genetic sequences of every known vertebrate species reaches its first milestone by publishing new methods and the first 25 high-quality genomes.

It’s one of the most audacious projects in biology today – reading the entire genome of every bird, mammal, lizard, fish, and all other creatures with backbones.

And now comes the first major payoff from the Vertebrate Genomes Project (VGP): near complete, high-quality genomes of 25 species, Howard Hughes Medical Institute (HHMI) Investigator Erich Jarvis with scores of coauthors report April 28, 2021, in the journal Nature. These species include the greater horseshoe bat, the Canada lynx, the platypus, and the kākāpō parrot – one of the first high-quality genomes of an endangered vertebrate species.

The paper also lays out the technical advances that let scientists achieve a new level of accuracy and completeness and paves the way for decoding the genomes of the roughly 70,000 vertebrate species living today, says HHMI Investigator and study coauthor David Haussler, a computational geneticist at the University of California, Santa Cruz (UCSC). “We will get a spectacular picture of how nature actually filled out all the ecosystems with this unbelievably diverse array of animals.”

Together with a slew of accompanying papers, the work is beginning to deliver on that promise. The project team has discovered previously unknown chromosomes in the zebra finch genome, for example, and a surprise finding about genetic differences between marmoset and human brains. The new research also offers hope for saving the kākāpō and the endangered vaquita dolphin from extinction.

“These 25 genomes represent a key milestone,” explains Jarvis, VGP chair and a neurogeneticist at The Rockefeller University. “We are learning a lot more than we expected,” he says. “The work is a proof of principle for what’s to come.”

Sagui Marmoset

The marmoset genome reveals that several brain genes have pathogenic differences to those in humans. The finding highlights why it’s important for scientists to consider genomic context when developing animal models.

From 10K to 70K

The VGP milestone has been years in the making. The project’s origins date back to the late-2000s, when Haussler, geneticist Stephen O’Brien, and Oliver Ryder, director of conservation genetics at the San Diego Zoo, figured it was time to think big.

Instead of sequencing just a few species, such as humans and model organisms like fruit flies, why not read the complete genomes of ten thousand animals in a bold “Genome 10K” effort? At the time, though, the price tag was hundreds of millions of dollars, and the plan never really got off the ground. “Everyone knew it was a great idea, but nobody wanted to pay for it,” recalls HHMI Investigator and HHMI Professor Beth Shapiro, an evolutionary biologist at UCSC and a coauthor of the Nature paper.

Plus, scientists’ early efforts at spelling out, or “sequencing,” all the DNA letters in an animal’s genome were riddled with errors. In the original approach used to complete the first rough human genome in 2003, scientists chopped up DNA into short pieces a few hundred letters long and read those letters. Then came the fiendishly difficult job of assembling the fragments in the right order. The methods weren’t up to task, resulting in misassemblies, major gaps, and other mistakes. Often it wasn’t even possible to map genes to individual chromosomes.

Canada Lynx

Canada Lynx (lynx canadensis) in Winter.

The introduction of new sequencing technologies with shorter reads helped make the idea of reading thousands of genomes possible. These rapidly developing technologies slashed costs but also reduced quality in genome assembly structure. Then in 2015, Haussler and colleagues brought in Jarvis, a pioneer in deciphering the intricate neural circuits that let birds trill new tunes after listening to others’ songs. Jarvis had already shown a knack for managing big, complex efforts. In 2014, he and more than a hundred colleagues sequenced the genomes of 48 bird species, which turned up new genes involved in vocal learning. “David and others asked me to take on leadership of the Genome 10K project,” Jarvis recalls. “They felt I had the personality for it.” Or, as Shapiro puts it: “Erich is a very pushy leader, in a nice way. What he wants to happen, he will make happen.”

Jarvis expanded and rebranded the Genome 10K idea to include all vertebrate genomes. He also helped launch a new sequencing center at Rockefeller that, together with one at the Max Planck Institute in Germany led by former HHMI Janelia Research Campus Group Leader Gene Myers, and another at the Sanger Institute in the UK led by Richard Durbin and Mark Blaxter, is currently producing most of the VGP genome data. He asked Adam Phillippy, a leading genome expert at the National Human Genome Research Institute (NHGRI), to chair the VGP assembly team. Then, he found about 60 top scientists willing to use their own grant money to pay for the sequencing costs at the centers to tackle the genomes they were most interested in. The team also negotiated with the Māori in New Zealand and officials in Mexico to get kākāpō and vaquita samples in “a beautiful example of international collaboration,” says Sadye Paez, program director of the VGP at Rockefeller.

Opening doors

The massive team of researchers pulled off a series of technological advances. The new sequencing machines let them read DNA chunks 10,000 or more letters long, instead of just a few hundred. The researchers also devised clever methods for assembling those segments into individual chromosomes. They have been able to tease out which genes were inherited from the mother and the father. This solves a particularly thorny problem known as “false duplication,” where scientists mistakenly label maternal and paternal copies of the same gene as two separate sister genes.

“I think this work opens a set of really important doors, since the technical aspects of assembly have been the bottleneck for sequencing genomes in the past,” says Jenny Tung, a geneticist at Duke University, who was not directly involved with the research. Having high-quality sequencing data “will transform the types of question that people can ask,” she says.

The team’s improved accuracy shows that previous genome sequences are seriously incomplete. In the zebra finch, for example, the team found eight new chromosomes and about 900 genes that had been thought to be missing. Previously unknown chromosomes popped up in the platypus as well, as members of the team reported online in Nature earlier this year. The researchers also plowed through, and correctly assembled, long stretches of repetitive DNA, much of which contain just two of the four genetic letters. Some scientists considered these stretches to be non-functional “junk” or “dark matter.” Wrong. Many of the repeats occur in regions of the genome that code for proteins, says Jarvis, suggesting that the DNA plays a surprisingly crucial role in turning genes on or off.

That’s just the start of what the Nature paper envisions as “a new era of discovery across the life sciences.” With every new genome sequence, Jarvis and his collaborators uncover new – and often unexpected – findings. Jarvis’s lab, for example, has finally nabbed the regulatory region of a key gene parrots and songbirds need to learn tunes; next, his team will try to figure out how it works. The marmoset genome yielded several surprises. While marmoset and human brain genes are largely conserved, the marmoset has several genes for human pathogenic amino acids. That highlights the need to consider genomic context when developing animal models, the team reports in a companion paper in Nature. And in findings published last year in Nature, a group led by Professor Emma Teeling at University College Dublin in Ireland discovered that some bats have lost immunity-related genes, which could help explain their ability to tolerate viruses like SARS-CoV-2, which causes COVID-19.

Kākāpō Parrot

The highly endangered kākāpō parrot lacks genetic diversity but has apparently been able to purge deleterious mutations, a new analysis of its genome suggests.

The new information also may boost efforts to save rare species. “It is a critically important moral duty to help species that are going extinct,” Jarvis says. That’s why the team collected samples from a kākāpō named Jane, part of a captive breeding program that has brought the parrot back from the brink of extinction. In a paper published in the new journal Cell Genomics, of the Cell family of journals, Nicolas Dussex at the University of Otago and colleagues described their studies of Jane’s genes along with other individuals. The work revealed that the last surviving kākāpō population, isolated on an island off New Zealand for the last 10,000 years, has somehow purged deleterious mutations, despite the species’ low genetic diversity. A similar finding was seen for the vaquita, with an estimated 10-20 individuals left on the planet, in a study published in Molecular Ecology Resources, led by Phil Morin at the National Oceanic and Atmospheric Administration Fisheries in La Jolla, California. “That means there is hope for conserving the species,” Jarvis concludes.

Holding Young Platypus

High-quality gene sequences show previously unknown chromosomes in the platypus.

A clear path

The VGP is now focused on sequencing even more species. The project team’s next goal is finishing 260 genomes, representing all vertebrate orders, and then snaring enough funding to tackle thousands more, representing all families. That work won’t be easy, and it will inevitably bring new technical and logistical challenges, Tung says. Once hundreds or even thousands of animals readily found in zoos or labs have been sequenced, scientists may face ethical hurdles obtaining samples from other species, especially when the animals are rare or endangered.

But with the new paper, the path ahead looks clearer than it has in years. The VGP model is even inspiring other large sequencing efforts, including the Earth Biogenome Project, which aims to decode the genomes of all eukaryotic species within 10 years. Perhaps for the first time, it seems possible to realize the dream that Haussler and many others share of reading every letter of every organism’s genome. Darwin saw the enormous diversity of life on Earth as “endless forms most beautiful,” Haussler observes. “Now, we have an incredible opportunity to see how those forms came about.”

Reference: “Towards complete and error-free genome assemblies of all vertebrate species” by Arang Rhie, Shane A. McCarthy,

The visitors from deep space baffling scientists

 

The visitors from deep space baffling scientists
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An artist's impression of the alien object 'Oumuamua (Credit: Alamy)
Astronomers spent decades looking for objects from outside our own solar system. Then two arrived at once. When should we expect the next one? And what can they teach us?

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It emerged from the celestial void in October 2017 – a tiny bright speck on the telescope at Haleakalā ObservatoryHawaii.

Tumbling through space at 57,000mph (90,000 kmph), the object is thought to have come from the direction of Vega, an alien star that resides 147 trillion miles (237 trillion km) away. Possibly shaped like an elongated cigar, possibly formed into an uncannily spaceship-like disc, by the time it was spotted it had already zipped by our own Sun, performed a slick hairpin turn, and begun hurtling off in another direction.

This space anomaly was named 'Oumuamua – pronounced oh-moo-uh-moo-uh – Hawaiian for "a messenger from afar arriving first". Robert Weryk, the astronomer at the University of Hawaii who first detected it, knew immediately from its speed that he was looking at something new to physics. This was no ordinary comet or asteroid, it was an interstellar visitor from a distant, unidentified solar system – the first to have ever been found.

Appropriately for an object with such alien origins, it soon became clear that 'Oumuamua was suitably strange. Two things in particular fixated scientists.

The first was its mysterious acceleration away from the Sun, which was hard to reconcile with many ideas about what it might have been made of. The second was its peculiar shape – by some estimates, it was 10 times as long as it was wide. Before 'Oumuamua, the most elongated known space objects were three times longer than they were wide.

Over the years that followed, scientific journals and global media headlines swarmed with speculation. Was it a block of solid hydrogen? Could it have been a cosmic "dust bunny" – a giant space version of the clumps of hair and debris often found under living room furniture? Or was it, as the esteemed Harvard astronomer Avi Loeb suggested, an artificial construction made by an intelligent extra-terrestrial civilisation?

A surprise guest

Scientists had suspected for decades that our solar system might be regularly visited by these intergalactic voyagers, many of which are thought to have been roaming among the stars for billions of years. But though there are hundreds of specialist instruments scanning the skies each night, from a snow-battered telescope at the South Pole to the sun-baked Atacama Large Millimeter Array (Alma) in the Chilean Andes, none had ever been spotted.  

The brightness of 'Oumuamua was found to fluctuate at regular intervals, suggesting that it's rotating and either highly elongated or disc-shaped (Credit: Alamy)

The brightness of 'Oumuamua was found to fluctuate at regular intervals, suggesting that it's rotating and either highly elongated or disc-shaped (Credit: Alamy)

Then not long after 'Oumuamua appeared, something unexpected happened: they found another one.

On 30 August 2019, the engineer and amateur astronomer Gennady Borisov glimpsed an object moving against the predawn sky from his personal observatory in Nauchnyi, Crimea – using a telescope he had made himself. Even at first sight, he realised it was special – it was travelling in a different direction to the comets that inhabit the main asteroid belt that straddles the Solar System.

2I/Borisov was named in its discoverer's honour, and is suspected to be a rogue comet – one that's not bound to a star. So where did these visitors come from? What can they tell us about alien solar systems? And how often should we expect to see them?

To find out, first it helps to know what they are made of.

A mysterious absence

'Oumuamua has not yet been definitively classified as a comet or an asteroid – it might be something else entirely – but scientists have always thought that most interstellar objects would be the former. Some of the comets that currently inhabit the furthest reaches of our own solar system may have originally been interstellar voyagers before they were captured by the Sun's gravity, so this would make sense.

However, most comets have "tails" – bright smudges that trail behind them – which form when they travel close to the Sun and heat up, releasing the frozen gases and dust inside them. As you might have guessed by now, 'Oumuamua didn't. This was particularly jarring, because its path took it deep into the Solar System, plunging towards the Sun and missing it by a mere 0.26 AU – around a quarter of the distance from the Earth to the Sun.

"As the data came in, more and more peculiarities came about," says Loeb, adding that he attended a conference about 'Oumuamua around this time, and when it ended, he left the room with a colleague who has worked on asteroids for decades. "He said, 'This is so strange, I wish it had never existed' – it took people out of their comfort zone."

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At first, scientists thought that perhaps this meant 'Oumuamua was a rocky asteroid after all. Then more observations came through. "They found that it had this acceleration as it was moving away from the Sun," says Alan Jackson, an astronomer and planetary scientist at Arizona State University.

This was universally baffling. It's perfectly normal for comets to accelerate as they travel back out from a close encounter with the Sun, but only because they are being powered by their tails – the gases being ejected give them a kick, like the engine on a rocket.

'Oumuamua is just 400-800 meters (1,300-2,600 ft) long, and was only visible while it was near the Sun (Credit: ESO/K. Meech et al.)

'Oumuamua is just 400-800 meters (1,300-2,600 ft) long, and was only visible while it was near the Sun (Credit: ESO/K. Meech et al.)

"That is really the straw that broke the camel's back for me, so to speak – in addition to the Sun's force of gravity, there was something pushing it away," says Loeb. "In order to explain this push, you needed about a 10th of the mass of this object to evaporate."

One idea was that perhaps the object was a "hydrogen iceberg" – a giant lump of frozen hydrogen, which could have formed a tail that wouldn't be visible from Earth.

However, not everyone was convinced. For a start, no one has ever seen hydrogen ice in space – Loeb and his colleagues have argued that lumps of it couldn't possibly have remained cold enough for long enough to form a large object like 'Oumuamua. And given that its freezing point (-259C/-434F) is only slightly above the ambient temperature of the Universe, it seems unlikely that it would have survived the several-hundred-million year trek from the nearest region of space thought to make such objects.  As one commentator put it, it would have fallen apart after being "cooked by starlight".

In all the confusion, the idea that 'Oumuamua might have been made by an intelligent alien civilisation began to look a little bit more plausible – for one thing, scientists at the Seti Institute were intrigued enough to point a telescope at it and listen out for any radio signals that it might be emitting.

In the alien technology scenario, the unexplained push 'Oumuamua received from the Sun was caused by the reflection of sunlight off its surface, which would need to be a thin, flat and reflective – like the wind pushing the sail on a boat. The object was indeed extremely shiny for how small it was, "but of course, nature doesn't make sails", says Loeb. "So that's what led me to suggest in a Scientific American article and later in a scientific paper [and now a book] that it may be of artificial origin."

Loeb explains that another object – 2020-SO – received a similarly mysterious acceleration from the Sun in September 2020. It was initially spotted by the same telescope that found 'Oumuamua, and turned out to be a rocket booster from the failed Surveyor II mission launched in 1966, which aimed to land a spacecraft on the Moon. It was successfully launched into space, but quickly lost contact and had been drifting around for decades. Like Loeb's proposed alien "lightsail", it had a flat, reflective surface that could repel light and propel it forwards.

Like the Surveyor III spacecraft, Surveyor II was intended to land on the Moon – but the latter was lost in space shortly after takeoff (Credit: Alamy)

Like the Surveyor III spacecraft, Surveyor II was intended to land on the Moon – but the latter was lost in space shortly after takeoff (Credit: Alamy)

In the end, Seti didn't find anything – though this doesn't rule out the possibility that 'Oumuamua belonged to a long-dead cosmic civilisation.

Then finally, earlier this year Jackson and his colleague Steven Desch came up with an explanation that seems to explain 'Oumuamua's quirky features, without the need for any alien technology. They started by ruling things out. For one thing, they knew that if there were any gases leaving 'Oumuamua, they couldn't include carbon monoxide, water, or carbon dioxide, because astronomers would have seen them.

"It had to be something nobody had considered before," says Desch. It also couldn't have been hydrogen, because the Universe is just too hot. "We just realised that nitrogen ice could supply exactly the amount of push it needs – and it's observed on Pluto," he says. To corroborate the idea, they calculated how shiny the surface of 'Oumuamua was and compared it to the reflectivity of nitrogen ice – and found that the two were more or less exact matches.

The team concluded that the object was likely to be a chunk of nitrogen ice, which was chipped off the surface of a Pluto-like exoplanet around a young star. Based on the evolution of our own solar system, which started out with thousands of similar planets in the icy neighbourhood of the Kuiper belt, they suggested that the fragment may have broken off around half a billion years ago.

"Eventually Neptune moved through that region and ejected a lot of the material – and this happened very early on," says Desch. They suggest that 'Oumuamua has been travelling around the frigid, barren expanse of deep space ever since.

Though the object would have finally reached the very outermost edge of the Solar System many years ago, it would have taken a long time to travel to the balmy, central region where it was first discovered – and been gradually worn down into a pancake as it approached. This explains its unusual shape and its acceleration in one go, because the evaporating nitrogen would have left an invisible tail that propelled it forwards. "Our atmosphere is mostly nitrogen and you can see though it," says Jackson. "Nitrogen gas is difficult to detect."

Again, not everyone is happy with this suggestion.

Pluto's Sputnik Planitia glacier is primarily made from nitrogen ice, and contains thousands of pits suspected to be caused by floating islands of water ice (Credit: Alamy)

Pluto's Sputnik Planitia glacier is primarily made from nitrogen ice, and contains thousands of pits suspected to be caused by floating islands of water ice (Credit: Alamy)

For one thing, Loeb is sceptical that the Pluto-like planet 'Oumuamua came from would have had a large enough surface area for it to be statistically plausible that we have found a fragment of it. His team have calculated that you would need for the stars in the galaxy to have have 100 times the mass they do, to account for us seeing a nitrogen iceberg that's been chipped off. "The surface layer of Pluto is only a few percent of its size," he says, "so that just doesn't make sense".

But if the theory turns out to be correct, 'Oumuamua may have provided a rare glimpse of what lies in alien solar systems.

At the moment, we can only see the planets that orbit other stars indirectly – by how much light they block out as their silhouette passes in front of tthe stars, or though the way their gravity distorts light as they pass by. It's all down to the mind-boggling distances involved. Travelling the 4.2 light years (25 trillion miles) to the nearest star, Proxima Centauri, would take thousands of years with our current technology. If it left the Earth now, a spacecraft like the Voyager – which is currently exploring deep space just outside our solar system – would arrive in the year 75100.  

"Getting to another extrasolar planet is never going to happen in my lifetime, or that of Western civilisation," says Jackson. "But we can have nature deliver pieces of them to us that we can actually see up close.".

The fact that 'Oumuamua was still relatively large when it entered our solar system suggests that was still a pristine fragment of its parent planet, preserved in the icy vacuum of space for half a billion years. In all that time, it is likely to have never encountered another star up close, until it stumbled upon our own. "It probably passed through dozens of solar systems within a fraction of a lightyear, but it wouldn’t have survived another trip near a sun like ours," says Desch.

In particular, 'Oumuamua's possible identity as an icy nitrogen iceberg suggests that other solar systems are reassuringly similar to our own.

Both 'Oumuamua and 2020-SO were spotted by the Pan-STARRS telescope in Hawaii, which has found thousands of space objects (Credit: Alamy)

Both 'Oumuamua and 2020-SO were spotted by the Pan-STARRS telescope in Hawaii, which has found thousands of space objects (Credit: Alamy)

"What it tells us is that in the outer regions of other planetary systems, we have these larger objects like Pluto," says Jackson. Calculations have even suggested that the ice had a reddish tint, similar to the one found layered over Pluto's nitrogen glaciers, which contain methane. "They're large enough that they differentiated – they were hot enough that they separated the different materials they were made out of and produced a layered structure."

Before 'Oumuamua, the outer reaches of other planetary systems were a total mystery, because the objects there are too distant to form much of a silhouette against their neighbourhood star. "We only really know about the ones that are closer in, because they go round more often and block out more of the starlight," says Jackson.

Even the nitrogen itself is news – in the Solar System, it's ubiquitous. But until 'Oumuamua, it was impossible to say whether it was common elsewhere. "That isn't something we have any kind of direct handle on before," says Jackson.

A ‘boring’ comet 

Luckily, 2I/Borisov has turned out to be emphatically less difficult to decipher than its cosmic companion. It's been recognised as the first interstellar comet ever found. Much like those lingering at the outer edges of the Solar System, 2I/Borisov is thought to have been composed of a muddy mixture of water, dust, and carbon monoxide. It had a visible tail and was more or less what scientists were expecting. If anything, 2I/Borisov makes 'Oumuamua seem even weirder.

2I/Borisov is thought to have been ripped from an ancient solar system centred around a red dwarf star, the dimmest and most abundant type in our galaxy. Based on its speed and trajectory, one international team has tentatively calculated that it might have originated around the star Ross 573 – now a white dwarf – which inhabits a region of space around 629 trillion miles (965 trillion km) away from the Sun. They suggest that it was ejected into space after the violent collision of three large objects in this celestial neighbourhood around 900,000 years ago.

However, Jackson is dubious. "We don't know which specific star system 2I/Borisov came from, it's been travelling for too long to track back to an individual system," he says. "But because Borisov looks more like a solar system comet, we would expect that it came from the cloud of comets within its parent system, wherever that is."

2I/Borisov is unusually rich in carbon monoxide, hinting that it came from a cool star – or that other solar systems have different chemistry (Credit: NASA, ESA and D. Jewitt)

2I/Borisov is unusually rich in carbon monoxide, hinting that it came from a cool star – or that other solar systems have different chemistry (Credit: NASA, ESA and D. Jewitt)

An impossible calculation

While some experts are mulling over how 'Oumuamua and 2I/Borisov can be so different, others are working on exactly how many other objects there might be like them.

"We had expected that we would eventually see interstellar objects, because we know that comets in our own solar system are ejected on a reasonably regular basis," says Jackson. It was logical to assume that the same process would happen elsewhere in the galaxy – but totally hypothetical.

Even after the discovery of 'Oumuamua, exactly how rare or statistically improbable its arrival was remained as baffling as the object itself – for all anyone knew its arrival might have been a once-in-a-lifetime event. Equally, our solar system could be swarming with these fragments of the wider galaxy, which are so dark, they only show up when their path happens to take them right past the Sun.

Now that scientists have found two interstellar voyagers, their hunch has been more or less confirmed. But estimating exactly how common these objects are – and how often we can expect to see them – remains extremely tricky.

One early calculation performed by Loeb and colleagues long before any interstellar objects were actually seen, in 2009, looked at how likely we were to find a single one. They based their estimate on the density of stars in the Milky Way and assumptions about the amount of matter each of them is ejecting into the wider universe, then compared this to the sensitivity of the most powerful telescope on Earth. They concluded that the probability it will find one in its entire lifetime of searching is "very small" – between one in a 1,000 and one in 100,000. Objects like 'Oumuamua should be so rare, scientists almost shouldn't have seen it. 

But they did. Based on its successful detection, one team calculated that, in each three-dimensional unit of space with sides the length of the distance from the Earth to the Sun, you would find approximately five similarly-sized cosmic objects there at any given time.

Inspired by a dust cloud found among a supernova in 2014, some scientists have proposed that 'Oumuamua is a giant "dust bunny" (Credit: NASA, ESA, and A. Angelich (NRAO/AUI/NSF))

Inspired by a dust cloud found among a supernova in 2014, some scientists have proposed that 'Oumuamua is a giant "dust bunny" (Credit: NASA, ESA, and A. Angelich (NRAO/AUI/NSF))

This suggests a significantly higher density of interstellar matter in the galaxy than had previously been thought. It also hints that, rather than being solely produced by young solar systems when their planets are forming, these objects are released throughout the entire lives of stars – or they wouldn't be anywhere near as common. 

Meanwhile, more recent research – made after the discovery of 2I/Borisov – suggests that there are around 50 interstellar objects spanning at least 50m accross in our solar system at any given time.

This is significant, because not all interstellar objects are as innocent as our recent visitors. While the impact that killed off the dinosaurs is now thought to have come from an object that originated within our own solar system, interstellar asteroids and comets are likely to be especially destructive, because they travel significantly faster than the ones orbiting our own Sun.

A search for more

Either way, scientists are about to get some answers. Detecting the faint glow of interstellar objects requires powerful equipment – exactly the kind that a new observatory under construction in Chile will have.

The Vera Rubin Observatory sits on top of Cerro Pachón, a 2,682 metre (8,799-ft) high mountain in the north of the country. It's expected to go live in 2022 or 2023 and is home to the largest digital camera ever constructed for the field of astronomy. It will undertake nightly surveys of the night skies, searching for near-earth objects at least 140m (500ft) across – around two-thirds the size of 'Oumuamua and one-seventh the size of 2I/Borisov.

Many astronomers are optimistic that it will find the next interstellar object – as well as our solar system's elusive hypothetical extra planet, Planet Nine. "What we really need is we need to see more objects like 'Oumuamua, then we can look at those statistics and actually get a proper picture of how many of those kind of objects there are," says Jackson. 

The LSST telescope under construction in Chile will be the most powerful on Earth, with glass polished to within a millionth of an inch of the shape needed (Credit: Getty Images)

The LSST telescope under construction in Chile will be the most powerful on Earth, with glass polished to within a millionth of an inch of the shape needed (Credit: Getty Images)

Loeb's hope is that the telescope will identify the next interstellar object when it is on its way into our solar system, with enough warning that we have time to send a spacecraft to intercept it and take a closer look. He cites the Osiris-Rex mission, which launched in September 2016 and has already successfully travelled to the asteroid Bennu, more than 200 million miles (321 million km) from Earth. It's currently on its way back, due to return with photographs and samples in 2023.

"And that will tell us if it's artificial, or, or natural," says Loeb. "And, of course, if it looks artificial, that will be very interesting. And we could land on it, and even read off the labels ‘Made on Planet X’."

Desch is equally enthusiastic about a trip to an interstellar object, though for slightly more conventional reasons. "When we think about any sort of spacecraft going to something in our own solar system, we have a checklist of things we want to get at, and this would be the same," he says, listing off some of the most important items, such as whether it contains amino acids – hinting at possible organic life – and determining if it contains water or carbon monoxide. "To get a rundown of all the chemistry of the object, that's what I'd want," he says.

But whatever happens, Loeb would like to see the scientific community keep an open mind – especially if our third encounter with an interstellar object proves just as baffling as 'Oumuamua. "If we find something that we've never seen before, let's collect more data on it and figure out the nature of it, because then we will learn something new about the nurseries or the factories that make such objects," he says.  

* Zaria Gorvett is a senior journalist for BBC Future and tweets @ZariaGorvett

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This article was updated on 7 May 2021. The original version incorrectly quoted Alan Jackson as describing 'Oumuamua's acceleration as it moved away from the Sun as "rapid".

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The Great Oxygenation Event (GOE) the beginning of oxygen’s permanent presence in the atmosphere.

 occurred 2.33 billion years ago, plus or minus 7 million years.......what we call the Great Oxidation Event—when appreciable levels of oxygen became a permanent feature in our atmosphere,”


discovered a large fractionation of the isotope sulfur-34, indicating a spike in marine sulfate levels around this same time. Such sulfate would have been produced from the reaction between atmospheric oxygen with sulfide minerals in rocks on land, and sulfur dioxide from volcanoes. 

 

This sulfate was then used by ocean-dwelling, sulfate-respiring bacteria to generate a particular pattern of sulfur-34 in subsequent sediment layers that were dated between 1 and 10 million years after the S-MIF transition.The results suggest that

 

 the initial buildup of oxygen in the atmosphere was relatively rapid. Since its first appearance 2.33 billion years ago, oxygen accumulated in high enough concentrations to have a weathering effect on rocks just 10 million years later.


================================

MIT News | Massachusetts Institute of Technology

Study pinpoints timing of oxygen’s first appearance in Earth’s atmosphere
And we need to understand that.”

Beginning 2.33 billion years ago, atmospheric oxygen built up in just 10 million years.
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MIT scientists say that the Great Oxygenation Event (GOE), a period that scientists believe marked the beginning of oxygen’s permanent presence in the atmosphere, started as early as 2.33 billion years ago.
Caption:
MIT scientists say that the Great Oxygenation Event (GOE), a period that scientists believe marked the beginning of oxygen’s permanent presence in the atmosphere, started as early as 2.33 billion years ago.

Today, 21 percent of the air we breathe is made up of molecular oxygen. But this gas was not always in such ample, life-sustaining supply, and in fact was largely absent from the atmosphere for the first 2 billion years of Earth’s history. When, then, did oxygen first accumulate in the atmosphere?

MIT scientists now have an answer. In a paper appearing today in Science Advances, the team reports that the Earth’s atmosphere experienced the first significant, irreversible influx of oxygen as early as 2.33 billion years ago. This period marks the start of the Great Oxygenation Event, which was followed by further increases later in Earth’s history.  

The scientists have also determined that this initial rise in atmospheric oxygen, although small, took place within just 1 to 10 million years and set off a cascade of events that would ultimately lead to the advent of multicellular life.

“It’s the start of a very long interval that culminated in complex life,” says Roger Summons, senior author of the paper and professor in the Department of Earth, Atmospheric, and Planetary Sciences (EAPS) at MIT. “It took another roughly 1.7 billion years for animals similar to those we have today to evolve. But the presence of molecular oxygen in the ocean and the atmosphere means that organisms that respire oxygen could thrive.”

Summons’ MIT co-authors include lead author and postdoc Genming Luo, as well as EAPS Associate Professor Shuhei Ono and graduate student David Wang. Professors Nicolas Beukes from the University of Johannesburg, in South Africa, and Shucheng Xie from the China University of Geosciences are the other co-authors.

Whiffs in the air

For the most part, scientists agree that oxygen, though lacking in the atmosphere, was likely brewing in the oceans as a byproduct of cyanobacterial photosynthesis as early as 3 billion years ago. However, as Summons puts it, oxygen in the ancient ocean “would have instantly been sucked up” by hungry microbes, ferrous iron, and other sinks, keeping it from escaping into the atmosphere.

“There may have been earlier, and temporary, ‘whiffs’ of oxygen in the atmosphere, but their abundances and durations are not currently measurable,” Summons says.

That changed with the Great Oxygenation Event (GOE), a period that scientists believe marked the beginning of oxygen’s permanent presence in the atmosphere. Previous estimates have placed the start of the GOE at around 2.3 billion years ago, though with uncertainties of tens to hundreds of millions of years.

“The dating of this event has been rather imprecise until now,” Summons says.

A transition, pinned

To get a more precise timing for the GOE, Luo first analyzed rocks from around this period, looking for a particular sulfur isotope pattern. When volcanoes erupt, they emit sulfur gases, which, when exposed to the sun’s ultraviolet radiation, can fractionate chemically and isotopically. The pattern of isotopes generated in this process depends on whether or not oxygen was present above a certain threshold.

Luo looked to pinpoint a major transition in a particular sulfur isotope pattern called mass-independent fraction of sulfur isotopes (S-MIF), in order to determine when oxygen first appeared in the Earth’s atmosphere. To do this, he first looked through sediment cores collected by Ono on a previous expedition to South Africa.

“Genming is a very tenacious and thorough guy,” Summons says. “He found rocks from deep in the core had S-MIF, and rocks shallow in the core had no S-MIF, but he didn’t have anything in between. So he went back to South Africa.”

There, he was able to sample from the rest of the sediment core and two others nearby, and determined that the S-MIF transition — marking the permanent passing of the oxygen threshold — occurred 2.33 billion years ago, plus or minus 7 million years, a much smaller uncertainty compared with previous estimates.

Getting a “decent hold”

The team also discovered a large fractionation of the isotope sulfur-34, indicating a spike in marine sulfate levels around this same time. Such sulfate would have been produced from the reaction between atmospheric oxygen with sulfide minerals in rocks on land, and sulfur dioxide from volcanoes. This sulfate was then used by ocean-dwelling, sulfate-respiring bacteria to generate a particular pattern of sulfur-34 in subsequent sediment layers that were dated between 1 and 10 million years after the S-MIF transition.

The results suggest that the initial buildup of oxygen in the atmosphere was relatively rapid. Since its first appearance 2.33 billion years ago, oxygen accumulated in high enough concentrations to have a weathering effect on rocks just 10 million years later. This weathering process, however, would have leached more sulfate and certain metals into waterways and ultimately, the oceans. Summons points out that it would be quite some time before the Earth system would reach another stable state, by the burial of organic carbon, and exceed the higher oxygen thresholds needed to encourage further biological evolution.

“Complex life couldn’t really get a decent hold on the planet until oxygen was prevalent in the deep ocean,” Summons says. “And that took a long, long time. But this is the first step in a cascade of processes.”

Timothy Lyons, professor of biogeochemistry at the University of California, Riverside, says the group’s timeline for oxygen’s rise “is a major contribution toward a refined understanding of the co-evolution of Earth’s early life and environments.”

“There are hints from past research of early transient accumulation of oxygen in the atmosphere and surface oceans before the loss of S-MIF, but the irreversible loss of this signal from the geologic record is now taken as the smoking gun for what we call the Great Oxidation Event—when appreciable levels of oxygen became a permanent feature in our atmosphere,” says Lyons, who did not contribute to the research. “The authors have done the community a great service by refining the timing of this event.”

Now that the team has constrained the timing of the GOE, Summons hopes others will apply the new dates to determine a cause, or mechanism, for the event. One hypothesis that the team hopes to explore is the connection between oxygen’s sudden and rapid appearance, and Snowball Earth, the period in which Earth’s continents and oceans were largely ice-covered. Now, thanks to the improved precision in geochronology, which Summons largely credits to EAPS Professor Samuel Bowring, scientists can start to nail down the mechanisms behind major events in Earth’s history, with more precise dates.

“It’s Sam’s insistence about this whole issue about ‘no dates, no rates’ that I think encourages people to focus on getting better data on the timing and duration of geological events,” Summons says.

“Because the other big question is, why do we have 21 percent oxygen in the Earth’s atmosphere that’s stable? That’s remarkable. And we need to understand that.”

This research was funded by the Simons Foundation with additional support from NASA, the Chinese National Natural Science Foundation, and the National Science Foundation.

And we need to understand that.”



faster-than-light space travel;Warp drives:

 

Warp drives: Physicists give chances of faster-than-light space travel a boost

April 24,
Faster than light travel is the only way humans could ever get to other stars in a reasonable amount of time. Les Bossinas/NASA/Wikimedia Commons

Warp drives: Physicists give chances of faster-than-light space travel a boost

April 24,

April 24,

The closest star to Earth is Proxima Centauri. It is about 4.25 light-years away, or about 25 trillion miles (40 trillion km). The fastest ever spacecraft, the now- in-space Parker Solar Probe will reach a top speed of 450,000 mph. It would take just 20 seconds to go from Los Angeles to New York City at that speed, but it would take the solar probe about 6,633 years to reach Earth’s nearest neighboring solar system.

If humanity ever wants to travel easily between stars, people will need to go faster than light. But so far, faster-than-light travel is possible only in science fiction.

In Issac Asimov’s Foundation series, humanity can travel from planet to planet, star to star or across the universe using jump drives. As a kid, I read as many of those stories as I could get my hands on. I am now a theoretical physicist and study nanotechnology, but I am still fascinated by the ways humanity could one day travel in space.

Some characters – like the astronauts in the movies “Interstellar” and “Thor” – use wormholes to travel between solar systems in seconds. Another approach – familiar to “Star Trek” fans – is warp drive technology. Warp drives are theoretically possible if still far-fetched technology. Two recent papers made headlines in March when researchers claimed to have overcome one of the many challenges that stand between the theory of warp drives and reality.


But how do these theoretical warp drives really work? And will humans be making the jump to warp speed anytime soon?

A circle on a flat blue plane with the surface dipping down in front and rising up behind.
This 2-dimensional representation shows the flat, unwarped bubble of spacetime in the center where a warp drive would sit surrounded by compressed spacetime to the right (downward curve) and expanded spacetime to the left (upward curve). AllenMcC/Wikimedia Commons

Compression and expansion

Physicists’ current understanding of spacetime comes from Albert Einstein’s theory of General Relativity. General Relativity states that space and time are fused and that nothing can travel faster than the speed of light. General relativity also describes how mass and energy warp spacetime – hefty objects like stars and black holes curve spacetime around them. This curvature is what you feel as gravity and why many spacefaring heroes worry about “getting stuck in” or “falling into” a gravity well. Early science fiction writers John Campbell and Asimov saw this warping as a way to skirt the speed limit.

What if a starship could compress space in front of it while expanding spacetime behind it? “Star Trek” took this idea and named it the warp drive.

In 1994, Miguel Alcubierre, a Mexican theoretical physicist, showed that compressing spacetime in front of the spaceship while expanding it behind was mathematically possible within the laws of General Relativity. So, what does that mean? Imagine the distance between two points is 10 meters (33 feet). If you are standing at point A and can travel one meter per second, it would take 10 seconds to get to point B. However, let’s say you could somehow compress the space between you and point B so that the interval is now just one meter. Then, moving through spacetime at your maximum speed of one meter per second, you would be able to reach point B in about one second. In theory, this approach does not contradict the laws of relativity since you are not moving faster than light in the space around you. Alcubierre showed that the warp drive from “Star Trek” was in fact theoretically possible.

Proxima Centauri here we come, right? Unfortunately, Alcubierre’s method of compressing spacetime had one problem: it requires negative energy or negative mass.

A 2–dimensional diagram showing how matter warps spacetime
This 2–dimensional representation shows how positive mass curves spacetime (left side, blue earth) and negative mass curves spacetime in an opposite direction (right side, red earth). Tokamac/Wikimedia Commons, CC BY-SA

A negative energy problem

Alcubierre’s warp drive would work by creating a bubble of flat spacetime around the spaceship and curving spacetime around that bubble to reduce distances. The warp drive would require either negative mass – a theorized type of matter – or a ring of negative energy density to work. Physicists have never observed negative mass, so that leaves negative energy as the only option.

To create negative energy, a warp drive would use a huge amount of mass to create an imbalance between particles and antiparticles. For example, if an electron and an antielectron appear near the warp drive, one of the particles would get trapped by the mass and this results in an imbalance. This imbalance results in negative energy density. Alcubierre’s warp drive would use this negative energy to create the spacetime bubble.

But for a warp drive to generate enough negative energy, you would need a lot of matter. Alcubierre estimated that a warp drive with a 100-meter bubble would require the mass of the entire visible universe.

In 1999, physicist Chris Van Den Broeck showed that expanding the volume inside the bubble but keeping the surface area constant would reduce the energy requirements significantly, to just about the mass of the sun. A significant improvement, but still far beyond all practical possibilities.

A sci-fi future?

Two recent papers – one by Alexey Bobrick and Gianni Martire and another by Erik Lentz – provide solutions that seem to bring warp drives closer to reality.

Bobrick and Martire realized that by modifying spacetime within the bubble in a certain way, they could remove the need to use negative energy. This solution, though, does not produce a warp drive that can go faster than light.


Independently, Lentz also proposed a solution that does not require negative energy. He used a different geometric approach to solve the equations of General Relativity, and by doing so, he found that a warp drive wouldn’t need to use negative energy. Lentz’s solution would allow the bubble to travel faster than the speed of light.

It is essential to point out that these exciting developments are mathematical models. As a physicist, I won’t fully trust models until we have experimental proof. Yet, the science of warp drives is coming into view. As a science fiction fan, I welcome all this innovative thinking. In the words of Captain Picard, things are only impossible until they are not.