ArticleNature astronomy2025
The variety and origin of materials accreted by Bennu's parent asteroid.
Article in Nature astronomy, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 11 papers.
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Who cites it
11 citing papers in PubMed.
- Nucleosynthetic constraints on the origin of Bennu and CI-like asteroids.Science advances · 2026Article
- Gradual Destruction of Refractory Stardust in Alkali Brines on Asteroid Bennu.Nature communications · 2026Article
- Ryugu and Bennu preserve primordial isotopic heterogeneity absent from the meteorite record.Nature communications · 2026Article
- Refractory inclusions in Bennu samples indicative of outer Solar System accretion.Nature communications · 2026Article
- Nanoscale infrared spectroscopy reveals complex organic-mineral assemblages in asteroid Bennu.Proceedings of the National Academy of Sciences of the United States of America · 2026Article
- Multiple formation pathways for amino acids in the early Solar System based on carbon and nitrogen isotopes in asteroid Bennu samples.Proceedings of the National Academy of Sciences of the United States of America · 2026Article
- Initial Conditions of Planet Formation: Time Constraints from Small Bodies and the Lifetime of Reservoirs in the Solar Protoplanetary Disk.Space science reviews · 2025Review
- Nitrogen- and oxygen-rich organic material indicative of polymerization in pre-aqueous cryochemistry on Bennu's parent body.Nature astronomy · 2025Article
- Abundant supernova dust and heterogeneous aqueous alteration revealed by stardust in two lithologies of asteroid Bennu.Nature astronomy · 2025Article
- Space weathering effects in Bennu asteroid samples.Nature geoscience · 2025Article
- Mineralogical evidence for hydrothermal alteration of Bennu samples.Nature geoscience · 2025Article
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Authors and funding
87 authors.
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No grant is acknowledged in the PubMed record.
Abstract
The first bodies to form in the Solar System acquired their materials from stars, the presolar molecular cloud and the protoplanetary disk. Asteroids that have not undergone planetary differentiation retain evidence of these primary accreted materials. However, geologic processes such as hydrothermal alteration can dramatically change their bulk mineralogy, isotopic compositions and chemistry. Here we analyse the elemental and isotopic compositions of samples from asteroid Bennu to uncover the sources and types of material accreted by its parent body. We show that some primary accreted materials escaped the extensive aqueous alteration that occurred on the parent asteroid, including presolar grains from ancient stars, organic matter from the outer Solar System or molecular cloud, refractory solids that formed close to the Sun, and dust enriched in neutron-rich Ti isotopes. We find Bennu to be richer in isotopically anomalous organic matter, anhydrous silicates, and light isotopes of K and Zn than its closest compositional counterparts, asteroid Ryugu and Ivuna-type (CI) carbonaceous chondrite meteorites. We propose that the parent bodies of Bennu, Ryugu and CI chondrites formed from a common but spatially and/or temporally heterogeneous reservoir of materials in the outer protoplanetary disk.
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