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NASA on Wednesday gave the public a first glimpse of what scientists found inside a sealed capsule that was returned to Earth last month carrying a carbon-rich soil sample scooped from an asteroid‘s surface, including water-bearing clay minerals.

A small quantity of the material collected by the OSIRIS-REx spacecraft three years ago from the near-Earth asteroid Bennu was unveiled in an auditorium at NASA’s Johnson Space Center in Houston, a little more than two weeks after it was parachuted into the Utah desert.

The return capsule’s landing capped a seven-year joint mission of the US space agency and the University of Arizona. It was only the third asteroid sample, and by far the biggest, returned to Earth for analysis, following two similar missions by Japan’s space agency ending in 2010 and 2020.

“It’s days like this that continue to amaze me,” NASA chief Bill Nelson said from the stage as he introduced the first picture of material retrieved from Bennu, a celestial artifact about 4.5 billions years old, on a viewing screen.

The image showed a loose cluster of small charcoal-colored rocks, pebbles and dust found to have been left in the outer portion of the sample-collection assembly when the asteroid’s soil was sucked through a filter into the spacecraft’s storage canister.

Technicians are still methodically disassembling hardware surrounding the inner science canister containing the bulk of the specimen, a process expected to take two more weeks.

But the “bonus” sample of overflow material was immediately examined with electron microscopes and X-ray instruments, said Dante Lauretta, principal mission investigator at the University of Arizona.

What they found was material high in carbon, nearly 5% by weight of an element essential to all life on Earth, as well as water molecules locked in the crystallized structure of clay fibers, Lauretta said.

Scientists also discovered iron minerals in the form of iron sulfides and iron oxides, “which themselves are indicative of formation in a water-rich environment,” Lauretta told a later news briefing.

Daniel Glavin, a senior sample scientist at NASA’s Goddard Space Flight Center, said early analysis found the material seems to be “loaded with organics.”

The preliminary findings point to a likelihood of further discoveries that could buttress the hypothesis that early Earth was seeded with the primordial ingredients for life by celestial objects such as comets, asteroids and meteorites that bombarded the young planet.

Ancient rubble pile

Bennu, discovered in 1999, is described by scientists as a relatively loose clump of rocky material, like a rubble pile, held together by gravity. It measures about three-tenths of a mile (500 meters) across, making it slightly wider than the Empire State Building is tall but tiny compared with the Chicxulub asteroid that struck Earth some 66 million years ago, wiping out the dinosaurs.

Like other asteroids, Bennu is a relic of the early solar system. Because its present-day chemistry and mineralogy are virtually unchanged since its formation, it holds clues to the origins and development of rocky planets such as Earth, and could prove central to studies of astrobiology.

The capsule was initially inspected at the Utah Test and Training range near the landing site, then flown to Houston for closer examination in a specially built “clean room” inside a Johnson Space Center astromaterials curation facility.

In the months ahead, the overall asteroid sample is to be parceled out into smaller specimens promised to some 200 scientists in 60 laboratories around the world.

At the time it landed, the Bennu sample was estimated to weigh about 250 grams (8.8 ounces), well above the minimum amount of 60 grams (2 ounces) scientists had hoped to collect. A more precise measurement will come in a few weeks, once the canister has been fully opened and all the contents weighed.

OSIRIS-REx launched in 2016 and reached Bennu in 2018, then spent nearly two years orbiting it before venturing close enough to snatch a sample of the loose surface material with its robotic arm on October 20, 2020.

Lauretta said preliminary analysis of the first bits of the sample showed that orbital observations of the asteroid had “predicted the mineralogy very accurately.” 

NASA is due to launch a separate mission on Thursday to a more distant asteroid called Psyche, a metal-rich body believed to be the remnant core of a protoplanet and the largest known metallic object in the solar system.

© Thomson Reuters 2023


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Astronomers Capture First-Ever Image of a Dead Star That Exploded Twice in Rare Supernova Event

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Astronomers Capture First-Ever Image of a Dead Star That Exploded Twice in Rare Supernova Event

For the first time, a team of astronomers has captured a clear image of a white dwarf star that exploded not just once, but twice, as a Type Ia supernova — a “double-detonation” that scientists hadn’t thought possible until now. The extraordinary observation could revise our long-held notions of how stars die, suggesting that some stars can explode as supernovas without ever crossing the Chandrasekhar limit, the minimum mass normally thought necessary for such an explosion. The astronomers employed the Very Large Telescope’s MUSE instrument to zoom in on the four-century-old supernova remnant SNR 0509-67.5, which sits 60,000 light-years away in the constellation Dorado, revealing evidence of two separate blasting catastrophes in its construction.

First Visual Proof Shows White Dwarfs Can Explode Twice Without Reaching Chandrasekhar Limit

As the researchers report on July 2 in Nature Astronomy, the team found a distinctive “fingerprint” in the debris of SNR 0509-67.5 in the Large Magellanic Cloud that the models predicted. White dwarfs—which are the dead stage of sun-like stars—usually blow up into Type Ia supernovas after they hit the Chandrasekhar limit by stealing matter from a neighbouring star.

However, this finding shows that the detonation can be launched at an earlier time. The explosion is likely to have a two-step origin, the team argues, with the initial blast being generated when an unstable layer of helium that the star had acquired exploded on its surface; the resulting shock wave then drove a second and main detonation.

“This physical proof of a double-detonation not only helps solve a long-standing mystery of what causes these explosions, but it represents the most visually compelling evidence for this origin.” Priyam Das, University of New South Wales, team leader and author.

Something is happening to Type Ia supernovas, the “standard candles” used to measure cosmic distances, because their brightness doesn’t fluctuate. But they have long mystified scientists with how they explode. Until this discovery, an explosion white dwarf that didn’t surpass the Chandrasekhar limit was only considered in theory.

This fresh visual evidence for the double detonation model further informs our knowledge of stellar evolution and also informs how we should interpret light from distant supernovas. More than its scientific implications, its discovery adds a colourful new page to the story of dying stars — stars that, as it now appears, will not go gently into that night but will light up the sky twice over in fantastic fireworks before vanishing from the cosmos.

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Climate Satellite MethaneSAT Fails After Just One Year in Orbit

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Climate Satellite MethaneSAT Fails After Just One Year in Orbit

One of the world’s most advanced satellites for detecting methane and other gases that contribute to the warming of the planet has gone dark and stopped communicating with ground-based controllers just over a year after being launched into orbit. Created by the nonprofit Environmental Defense Fund (EDF), the satellite — estimated to cost as much as $88 million — hitched a ride into space on a SpaceX rocket in March 2024. It was charged with monitoring methane leaks from oil and gas operations, and then making the data available to policymakers and scientists through open access. But on June 20, contact with the satellite was lost, and attempts to recover it have failed. EDF officially reported on July 1 that MethaneSAT has lost power and appears unlikely to recover.

MethaneSAT Failure Marks Setback for Climate Transparency Despite Data Gains and Global Support

As per a statement released by EDF, MethaneSAT’s failure came despite multiple recovery attempts. The satellite was constructed to lift the veil off methane’s invisible, weighty impact on global warming. It is nowhere near as common as carbon dioxide, but over a timescale of, say, a century, it is 20 to 30 times more efficient at trapping heat in the atmosphere than carbon dioxide. That makes its emissions a prime target in the effort to minimize the risks of global warming. MethaneSAT was developed to independently corroborate industrial methane reports, especially those from fossil fuel extraction. The loss of the satellite is a remarkable setback for transparency in climate science and monitoring of emissions worldwide.

Yet mission operators are hopeful that data already collected will have far-reaching effects. EDF emphasized that insights from MethaneSAT’s year in orbit will continue to be processed and made public in the coming months. The mission included backing from 10 partners such as Harvard University, the New Zealand Space Agency, BAE Systems, Google, and the Bezos Earth Fund.

Officials called MethaneSAT a bold and needed move to hold our climate accountable. Although the mission was cut short, it signaled one of the largest joint efforts between science, advocacy, and technology to battle climate change. “To succeed in meeting the climate challenge, we need bold action and fearless innovation,” EDF mentioned, describing the satellite as “at the vanguard of science.”
MethaneSAT’s brief history highlights the difficulty — and importance — of deploying space-based instruments to try and combat climate change. As other missions get ready to blaze the same trail, the data and experience this little spacecraft provided will influence the future of Earth observation.

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Microsoft Says Xbox Chief Phil Spencer Not Retiring ‘Anytime Soon’ After Rumour Surfaces Amid Layoffs

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New Interstellar Comet 3I/ATLAS Speeds Through Solar System

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New Interstellar Comet 3I/ATLAS Speeds Through Solar System

A newly confirmed interstellar comet is making a rare passage through our solar system — and skywatchers can catch it live online tonight. The object, now called 3I/ATLAS, is just the third interstellar visitor ever detected after the well-known ‘Oumuamua (2017) and 2I/Borisov (2019). The comet was so fresh when first detected on July 1 by the ATLAS telescope in Chile that it hadn’t even been given a name yet; the Minor Planet Center has it listed as “3I,” the “I” standing for interstellar. Tonight’s webcast will kick off at 6 p.m. EDT (2200 GMT) from the Virtual Telescope Project’s virtual observing facilities in Italy.

Interstellar Comet 3I/ATLAS Speeds Toward Sun at 68 km/s, Offers Rare Study Opportunity

As per a report by Space.com, 3I/ATLAS was detected as a faint object displaying subtle cometary features, including a marginal coma and a short tail. Currently located 4.5 astronomical units (AU) from the sun — about 670 million kilometers (416 million miles) — the comet is faint at magnitude 18.8, making it invisible to amateur telescopes. The interstellar object is traveling at an astonishing pace of 68 kilometers per second (152,000 mph) relative to the sun, but NASA officials say it poses no danger to Earth.

It was imaged by the Virtual Telescope Project on July 2, showing the comet as a point of light within the trailing background stars — a sure indication that it is indeed moving through space. 3I/ATLAS should brighten a little as it approaches the sun, particularly when it gets closest, or its perihelion, on Oct. 30, when it swings within 1.4 astronomical units of the sun or Mars’ orbit.

The close pass by this interstellar visitor is a rare chance for astronomers to study the materials and dynamics outside our solar system. 3I/ATLAS, which is racing along at a frenetic pace on an elliptical orbit, may also support research into how these objects change as they sit in different stellar environments.

After disappearing behind the sun in late fall, 3I/ATLAS is projected to return to observational reach in early December. Researchers anticipate further analysis then, expanding our understanding of these rare visitors that traverse the galaxy — and occasionally, pass through our celestial neighborhood.

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The Hunt: Rajiv Gandhi Assassination Now Available For Streaming on SonyLIV

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