NASA's Lucy spacecraft flew past asteroid Donaldjohanson on April 20, 2025, revealing a peanut shaped, tumbling body with iron rich clays that only form in the presence of liquid water — the first direct evidence of a... The asteroid is just 155 million years old (a fraction of the age of Bennu or Ryugu), rotates en...
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Create a landscape editorial hero image for this Studio Global article: What did NASA's Lucy mission discover about the asteroid Donaldjohanson during its April 20, 2025 flyby, including evidence of ancient liqui. Article summary: Here is a comprehensive summary of what NASA's Lucy mission discovered about asteroid Donaldjohanson during its April 20, 2025 flyby, synthesized from NASA's official release, the peer-reviewed study in *Science*, and su. Topic tags: general, government, education, general web. Style: premium digital editorial illustration, source-backed research mood, clean composition, high detail, modern web publication hero. Use reference image context only for broad subject, composition, and topical grounding; do not copy the exact image. Avoid: logos, brand marks, copyrighted characters, real person likenesses, fake screenshots, UI text, readable text, watermarks, charts
When NASA's Lucy spacecraft flew past the small main-belt asteroid Donaldjohanson on April 20, 2025, mission scientists expected a useful rehearsal for the Jupiter Trojan encounters ahead. What they got was a compact world with a dramatic story of its own — a peanut-shaped, tumbling body that once held liquid water and is far younger than any other asteroid visited up close.
The findings, published on June 18, 2026, in the journal Science (DOI: 10.1126/science.aec0503), paint a detailed portrait of an asteroid that formed from the debris of a catastrophic collision and has been steadily slowing down and shaking itself apart ever since .
The most striking discovery came not from the visible-light images but from the infrared. Lucy's LEISA spectrometer, part of the L'Ralph instrument, detected iron-rich clay minerals (iron-bearing phyllosilicates) on the asteroid's surface . These clays are chemically similar to those found in carbon-rich meteorites such as QUE 97990 — and crucially, they can only form through the chemical alteration of rock by liquid water
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This is the first direct evidence that Donaldjohanson's parent body once contained liquid water. The alteration appears to have halted at an early stage, likely because the parent body lacked enough water or heat to drive the process further . The asteroid itself is a fragment from that larger, water-rich parent body, shattered in a collision long ago.
Donaldjohanson is a member of the Erigone asteroid family, a group of objects created when a larger, carbon- and water-rich parent body was catastrophically disrupted . That collision happened about 155 million years ago — making Donaldjohanson a teenager compared to well-studied asteroids like Bennu and Ryugu, which are 1–2 billion years old
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Classified as a C-type (carbonaceous) asteroid, it is rich in carbon and water-bearing minerals, consistent with the composition of the Erigone family . Unlike Bennu and Ryugu, both of which migrated into near-Earth orbits, Donaldjohanson has stayed put in the main asteroid belt since it formed
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High-resolution images from Lucy's L'LORRI imager revealed that Donaldjohanson is not a simple, round rock. It has a bilobate, or "peanut," shape — two cratered lobes connected by a relatively smooth neck . This suggests that two fragments from the original parent-body collision gently coalesced under their own gravity to form the asteroid we see today.
But the shape is only half the story. Donaldjohanson does not spin like a typical asteroid. Instead, it undergoes a complex tumbling rotation: it rotates end-over-end once every 10.5 Earth days while simultaneously wobbling around its horizontal axis every 26.5 days . This is a non-principal-axis rotation — think of a wobbly top that has almost lost its spin.
This tumbling was likely induced gradually by the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect, where sunlight exerts tiny torques on an asteroid's irregular shape over millions of years . The asteroid probably rotated at least 10 times faster when it first formed and has since slowed to its current lethargic spin over the last 20–60 million years
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Another surprise: craters smaller than 0.4 km appear to have been preferentially erased from the surface, possibly by seismic shaking from a more recent impact event . The asteroid measures about 0.8 km (half a mile) in diameter
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The Donaldjohanson flyby was never primarily about Donaldjohanson itself. It was explicitly designed as a dress rehearsal for Lucy's primary targets: the never-before-explored Jupiter Trojan asteroids . The encounter allowed the team to:
As SwRI's Dr. Simone Marchi put it: "This encounter gave us an opportunity to test our instruments and our procedures to make sure we are ready when we get to Jupiter's Trojans."
In that sense, Donaldjohanson delivered everything NASA could have asked for — a scientifically rich target that also served as a perfect proving ground for the mission's most ambitious goals.
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NASA's Lucy spacecraft flew past asteroid Donaldjohanson on April 20, 2025, revealing a peanut shaped, tumbling body with iron rich clays that only form in the presence of liquid water — the first direct evidence of a...
NASA's Lucy spacecraft flew past asteroid Donaldjohanson on April 20, 2025, revealing a peanut shaped, tumbling body with iron rich clays that only form in the presence of liquid water — the first direct evidence of a... The asteroid is just 155 million years old (a fraction of the age of Bennu or Ryugu), rotates end over end once every 10.5 days while wobbling every 26.5 days, and the flyby served as a critical dress rehearsal for Lu...