Nanoscale infrared spectroscopy reveals complex organic–mineral assemblages in asteroid Bennu

M Mehmet Yesiltas (Department of Geosciences, Stony Brook University) A Andrew Dopilka (Energy Technologies and Systems Division, Lawrence Berkeley National Laboratory) R Robert Kostecki (Energy Technologies and Systems Division, Lawrence Berkeley National Laboratory) T Timothy D. Glotch (Department of Geosciences, Stony Brook University) P Paul Northrup (Department of Geosciences, Stony Brook University)

Abstract

Asteroid Bennu preserves primitive material from the early solar system, and returned samples allow direct examination of how organics and minerals were assembled and altered. We applied nanoscale infrared spectroscopy together with Raman spectroscopy to the Bennu sample OREX-800066-3 to characterize chemical variability at ~20 nm scales. Analysis of nano-Fourier-transform infrared spectroscopy spectra identifies three recurring compositional domains; aliphatic-rich, carbonate-rich, and nitrogen-bearing organic-rich regions. Statistical evaluation shows that these domains are compositionally and spatially distinct at the nanoscale, with strong negative correlations between aliphatic signatures and both carbonates and N-bearing organics, and negligible correlation between carbonates and N-bearing organics. Organosulfur compounds are spatially restricted to carbonate-rich regions, indicating organic-sulfate interactions during late-stage brine evolution. Raman spectra indicate highly disordered, thermally minimally metamorphosed carbonaceous matter, consistent with preservation of labile functional groups. These results demonstrate that Bennu’s angular lithology (characterized by planar facets and sharp edges) is not chemically uniform and records heterogeneous aqueous alteration rather than pervasive uniform processing. N-bearing organic functional groups are widely preserved despite extensive alteration, and carbonate-rich areas show intimate nanoscale mixing of different carbonate species. The coexistence of distinct organic- and carbonate-rich domains suggests contributions from both primordial compositional diversity and subsequent rock–fluid interaction. Comparison with Ryugu samples highlights shared features but key differences in organic-carbonate associations and carbonate distributions. Overall, Bennu’s nanoscale heterogeneity provides constraints on organic preservation, carbonate formation, organic-sulfate chemistry, and parent-body evolution in volatile-rich early solar system materials.

Article Details

Volume / Issue Vol. 123, Issue 14
Published April 07, 2026
ISSN 0027-8424
Publisher National Academy of Sciences

Authors (5)

M

Mehmet Yesiltas

Department of Geosciences, Stony Brook University

A

Andrew Dopilka

Energy Technologies and Systems Division, Lawrence Berkeley National Laboratory

R

Robert Kostecki

Energy Technologies and Systems Division, Lawrence Berkeley National Laboratory

T

Timothy D. Glotch

Department of Geosciences, Stony Brook University

P

Paul Northrup

Department of Geosciences, Stony Brook University