Composition of organics on asteroid (101955) Bennu

H. H. Kaplan, A. A. Simon, V. E. Hamilton, M. S. Thompson, S. A. Sandford, M. A. Barucci, E. A. Cloutis, J. Brucato, D. C. Reuter, D. P. Glavin, B. E. Clark, J. P. Dworkin, H. Campins, J. P. Emery, S. Fornasier, X. D. Zou, D. S. Lauretta

Research output: Contribution to journalArticlepeer-review

10 Scopus citations


Context. The Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) mission detected an infrared absorption at 3.4 μm on near-Earth asteroid (101955) Bennu. This absorption is indicative of carbon species, including organics, on the surface. Aims. We aim to describe the composition of the organic matter on Bennu by investigating the spectral features in detail. Methods. We use a curated set of spectra acquired by the OSIRIS-REx Visible and InfraRed Spectrometer that have features near 3.4 μm (3.2 to 3.6 μm) attributed to organics. We assess the shapes and strengths of these absorptions in the context of laboratory spectra of extraterrestrial organics and analogs. Results. We find spectral evidence of aromatic and aliphatic CH bonds. The absorptions are broadly consistent in shape and depth with those associated with insoluble organic matter in meteorites. Given the thermal and space weathering environments on Bennu, it is likely that the organics have not been exposed for long enough to substantially decrease the H/C and destroy all aliphatic molecules.

Original languageEnglish (US)
Article numbere2141167
JournalAstronomy and astrophysics
StatePublished - Sep 1 2021


  • Minor planets, asteroids: individual: (101955) Bennu
  • Planets and satellites: composition
  • Techniques: spectroscopic

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


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