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NASA\u2019s OSIRIS-REx spacecraft descends toward asteroid Bennu during a 2020 rehearsal for sample collection. Credit: NASA\/Goddard\/University of Arizona<\/p>\nNASA\u2019s OSIRIS-REx spacecraft descends toward asteroid Bennu during a 2020 rehearsal for sample collection. Credit: NASA\/Goddard\/University of Arizona<\/p>\n
A few ounces of black asteroid rubble have become something like a forensic archive<\/a> of the early solar system.<\/p>\n Since NASA\u2019s OSIRIS-REx spacecraft delivered 121.6 grams of material from asteroid Bennu to Earth in 2023, scientists have found salts left by ancient water, organic molecules, amino acids and minerals dating to before the planets formed. Now researchers claim they\u2019ve figured out where Bennu\u2019s ancestral material assembled and what Jupiter was doing while the solar system was still under construction.<\/p>\n In a new study, researchers measured subtle variations in iron, titanium, and chromium isotopes in Bennu grains. Their results suggest that the parent body from which Bennu ultimately descended formed near the water-ice line, apparently inside the orbit of the growing Jupiter, from an unusually well-mixed reservoir of fine dust.<\/p>\n Previously, it was thought Bennu was the descendant of a larger planetary body assembled much farther from the Sun.<\/p>\n Chemical Address<\/p>\n Isotopes are versions of the same chemical element with different numbers of neutrons. Tiny differences in their abundances can survive for billions of years, giving planetary scientists something akin to a chemical return address.<\/p>\n Maria Sch\u00f6nb\u00e4chler, an isotope geochemist at ETH Zurich, and her colleagues measured the proportions of different forms of iron, titanium and chromium in several Bennu samples, including individual particle types and larger mixed samples. The iron and titanium isotope patterns were essentially the same across all of them, showing that Bennu\u2019s material was unusually uniform at that scale. The patterns also matched samples returned from asteroid Ryugu and rare CI chondrite meteorites, suggesting all three formed from the same broad reservoir of early solar-system dust.<\/p>\n But the pattern broke with the chromium isotopes. Its isotope ratios varied a little from one Bennu sample to another. The researchers think much of that variation arose after Bennu\u2019s original parent asteroid formed, when liquid water moved through the rock and altered some of its minerals.<\/p>\n \u201cBennu is a hybrid: the material does not clearly match either the inner or the outer solar system,\u201d Sch\u00f6nb\u00e4chler said in an ETH Zurich statement.<\/p>\n \u00d7<\/p>\n Thank you! One more thing…<\/p>\n Please check your inbox and confirm your subscription.<\/p>\n That is a notable shift. In Scientific American\u2019s<\/a> 2025 reporting on the first major Bennu sample results, planetary scientist Timothy McCoy placed its parent body \u201c[at] the current position of Jupiter or beyond,\u201d based partly on its water and volatile-rich chemistry.<\/p>\n And the debate is not settled. A Nature Communications study<\/a> published in July 2026 examined tiny heat-resistant inclusions in Bennu and concluded that its parent body probably accreted beyond proto-Jupiter\u2019s pressure barrier. <\/p>\n The new researchers propose a different reading of much of the same cosmic evidence.<\/p>\n Jupiter, the Giant Sieve<\/p>\n Very early in solar-system history, Jupiter grew enormous. By roughly two million years after the first solids formed, models suggest it may already have exceeded 20 Earth masses.<\/p>\n That growth would have carved a gap through the disk of gas and dust surrounding the young Sun. Crucially, the barrier was not airtight.<\/p>\n Larger particles tended to become trapped in pressure bumps around Jupiter. Tiny grains, however, remained coupled to the gas and could slip through. Collisions continually smashed larger objects into new fragments, supplying still more fine dust.<\/p>\n In this scenario, Jupiter behaved kind of like a giant sieve.<\/p>\n The grains that passed through could mix over vast distances before piling up near the water-ice line, where temperatures became cool enough for water vapor to freeze. Ice coating the particles would have helped them stick, while a local \u201ctraffic jam\u201d of solids could have encouraged them to collapse into larger bodies.<\/p>\n That mechanism could explain two otherwise puzzling features of Bennu: its abundance of water-altered material and its strikingly Sun-like proportions of many chemical elements. Bennu\u2019s parent body may have sampled a particularly thorough mixture of the solar system\u2019s finest dust.<\/p>\n \u201cBennu may offer our best glimpse of the original mix of chemical elements from which the terrestrial planets were ultimately built,\u201d Sch\u00f6nb\u00e4chler said.<\/p>\n This asteroid saw water alteration, collisions, fragmentation, and migration before the rubble pile we see today emerged.<\/p>\n But all of this is precisely what makes the returned sample so valuable. Different grains record different episodes. And three years after OSIRIS-REx dropped its capsule into the Utah desert, scientists are still finding new ways to make a fraction of a gram recount events that unfolded before Earth itself existed.<\/p>\n The study was published in the journal Science Advances<\/a>.<\/p>\n![\"-3\"](\"https:\/\/www.newsbeep.com\/nz\/wp-content\/uploads\/2026\/09\/bennu-asteroid-samples-1024x768.jpg\")
<\/a>Half a gram of this material was sent to ETH: a sample from the asteroid Bennu. Credit: Erika Blumenfeld & Joseph Aebersold \/ NASA<\/p>\n![\"-3\"](\"https:\/\/www.newsbeep.com\/nz\/wp-content\/uploads\/2026\/09\/upJYignb7oEk9xzeUMWbKV-1200-80.jpg-1024x576.webp\")
<\/a>A schematic of where various bodies formed in the solar system, and how Jupiter controlled what dust drifted inwards. Credit: Science Advances<\/p>\n
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