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NASA's Lucy probe captures 1st close-up images of asteroid Donaldjohanson, revealing 'strikingly complicated geology'

NASA's Lucy probe captures 1st close-up images of asteroid Donaldjohanson, revealing 'strikingly complicated geology'

Yahoo22-04-2025
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NASA's Lucy spacecraft, currently headed toward Jupiter on an asteroid-hopping mission, has captured an impressive close-up of its second target: the space rock 52246 Donaldjohanson.
Lucy launched in 2021, embarking on a 12-year journey toward Jupiter's orbit to study an unexplored swarm of asteroids called Jupiter's Trojans. These asteroids are remnants of our early solar system that share the giant planet's orbit around the sun. Along the way, the spacecraft is also squeezing in time for a few dress rehearsals for its Trojan targets down the road — and on Sunday (April 20), it swooped within 600 miles (1,000 kilometers) of the asteroid 52246 Donaldjohanson, named after American paleoanthropologist Donald Johanson who co-discovered the Lucy hominid fossil in northern Ethiopia in 1974.
Images of the asteroid Lucy took as it approached the three-mile-wide (five-kilometer-wide) asteroid showed wide swings in brightness, suggesting it was either a slowly-rotating rock, appearing brighter when its longer sides faced the spacecraft, or an elongated object. Indeed, close-up images of the asteroid sent home by Lucy on Sunday confirmed both: The asteroid was once two smaller pieces that have conjoined into a larger whole, with a distinct narrow neck between the two lobes.
"Asteroid Donaldjohanson has strikingly complicated geology," Hal Levison, the principal investigator for Lucy at Southwest Research Institute in Colorado, said in a statement. "As we study the complex structures in detail, they will reveal important information about the building blocks and collisional processes that formed the planets in our solar system."
The new images show the asteroid appearing to rotate. However, this apparent motion isn't due to the asteroid itself spinning — which it does at a very slow rate of three years and eight months — but rather the result of the Lucy spacecraft whizzing by during its flyby at a relative velocity of 8.3 miles per second (13.4 kilometers per second), NASA said.
Preliminary analyses of these images suggest the asteroid, which is likely a fragment of a collision about 150 million years ago, is larger than scientists initially estimated — measuring about 5 miles (8 km) long and 2 miles (3.5 km) wide at its widest point.
Related Stories:
— NASA's asteroid-hopping Lucy probe takes 1st images of its next target: Donaldjohanson
— NASA asteroid surveyor snaps stunning views of Earth and moon on way to Jupiter's Trojans
— Asteroid 'Dinky,' visited by NASA's Lucy spacecraft, birthed its own moon
The images do not technically reveal the entire asteroid, to be clear, as it is larger than the Lucy imager's field of view. The mission team anticipates it will take up to a week to download the remaining encounter data from the spacecraft, which will provide a more complete picture of the asteroid's overall shape.
"These early images of Donaldjohanson are again showing the tremendous capabilities of the Lucy spacecraft as an engine of discovery," Tom Statler, the program scientist for the Lucy mission at NASA Headquarters in Washington, said in the statement. "The potential to really open a new window into the history of our solar system when Lucy gets to the Trojan asteroids is immense."
Following this encounter, Lucy will spend the rest of this year cruising through the asteroid belt toward the Jupiter Trojan asteroids. Its first Trojan flyby, of asteroid Eurybates and its satellite Queta, is scheduled for August 2027.
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Late-night SpaceX rocket launch in Florida: When to see liftoff from Daytona to New Smyrna Beach
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Late-night SpaceX rocket launch in Florida: When to see liftoff from Daytona to New Smyrna Beach

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NASA Wasn't Happy When Astronaut John Young Smuggled This Food Into Space
NASA Wasn't Happy When Astronaut John Young Smuggled This Food Into Space

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NASA Wasn't Happy When Astronaut John Young Smuggled This Food Into Space

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Mercury's 'missing' meteorites may have finally been found on Earth
Mercury's 'missing' meteorites may have finally been found on Earth

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Mercury's 'missing' meteorites may have finally been found on Earth

When you buy through links on our articles, Future and its syndication partners may earn a commission. Most meteorites that have reached Earth come from the asteroid belt between Mars and Jupiter. But we have 1,000 or so meteorites that come from the Moon and Mars. This is probably a result of asteroids hitting their surfaces and ejecting material towards our planet. It should also be physically possible for such debris to reach the Earth from Mercury, another nearby rocky body. But so far, none have been confirmed to come from there — presenting a longstanding mystery. A new study my colleagues and I conducted has discovered two meteorites that could have a Mercurian origin. If confirmed, they would offer a rare window into Mercury's formation and evolution, potentially reshaping our understanding of the planet nearest the Sun. Because Mercury is so close to the Sun, any space mission to retrieve a sample from there would be complex and costly. A naturally delivered fragment, therefore, may be the only practical way to study its surface directly — making such a discovery scientifically invaluable. Observations from NASA's Messenger mission have inferred the surface composition of Mercury. This suggests the presence of minerals known as such as sodium-rich plagioclase (such as albite), iron-poor pyroxene (for example enstatite), iron-poor olivine (such as forsterite) and sulfide minerals such as oldhamite. The meteorite Northwest Africa (NWA) 7325 was initially proposed as a possible fragment of Mercury. However, its mineralogy includes chromium-rich pyroxene containing approximately 1% iron. This poorly matches Mercury's estimated surface composition. As a result of this, and other factors, this link has been challenged. Related: Mercury may have a 'potentially habitable' region below its surface, salty glaciers suggest Aubrite meteorites have also been proposed as potential Mercurian fragments. 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Both meteorites contain olivine and pyroxene, minor albitic plagioclase and oldhamite. Such features are consistent with predictions for Mercury's surface composition. Additionally, their oxygen compositions match those of aubrites. These shared characteristics make the samples compelling candidates for being Mercurian material. However, notable differences exist. Both meteorites contain only trace amounts of plagioclase, in contrast to Mercury's surface, which is estimated to contain over 37%. Furthermore, our study suggests that the age of the samples is about 4,528 million years old. This is significantly older than Mercury's oldest recognised surface units, which are predicted (based on crater counting) to be approximately 4,000 million years. If these meteorites do originate from Mercury, they may represent early material that is no longer preserved in the planet's current surface geology. To link any meteorite to a specific asteroid type, moon or planet is extremely challenging. For example, laboratory analysis of Apollo samples allowed meteorites found in desert collection expeditions to be matched with the lunar materials. Martian meteorites have been identified through similarities between the composition of gases trapped in the meteorites with measurements of the martian atmosphere by spacecraft. Until we visit Mercury and bring back material, it will be extremely difficult to assess a meteorite-planet link. The BepiColombo space mission, by the European and Japanese space agencies, is now in orbit around Mercury and is about to send back high-resolution data. This may help us determine the ultimate origin body for Ksar Ghilane 022 and Northwest Africa 15915. If meteorites from Mercury were discovered, they could help resolve a variety of long-standing scientific questions. For example, they could reveal the age and evolution of Mercury's crust, its mineralogical and geochemical composition and the nature of its gases. 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