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Bright carbonate veins on asteroid (101955) bennu: Implications for aqueous alteration history

  • H. H. Kaplan
  • , D. S. Lauretta
  • , A. A. Simon
  • , V. E. Hamilton
  • , D. N. Dellagiustina
  • , D. R. Golish
  • , D. C. Reuter
  • , C. A. Bennett
  • , K. N. Burke
  • , H. Campins
  • , H. C. Connolly
  • , J. P. Dworkin
  • , J. P. Emery
  • , D. P. Glavin
  • , T. D. Glotch
  • , R. Hanna
  • , K. Ishimaru
  • , E. R. Jawin
  • , T. J. McCoy
  • , N. Porter
  • S. A. Sandford, S. Ferrone, B. E. Clark, J. Y. Li, X. D. Zou, M. G. Daly, O. S. Barnouin, J. A. Seabrook, H. L. Enos
  • NASA Goddard Space Flight Center
  • Southwest Research Institute
  • University of Arizona
  • University of Central Florida
  • Rowan University
  • Northern Arizona University
  • University of Texas at Austin
  • Smithsonian Institution
  • NASA Ames Research Center
  • Ithaca College
  • 12Planetary Science Institute
  • York University Toronto
  • Johns Hopkins University Applied Physics Laboratory

Research output: Contribution to journalArticlepeer-review

118 Scopus citations

Abstract

The composition of asteroids and their connection to meteorites provide insight into geologic processes that occurred in the early Solar System. We present spectra of the Nightingale crater region on near-Earth asteroid Bennu with a distinct infrared absorption around 3.4 micrometers. Corresponding images of boulders show centimeters-thick, roughly meter-long bright veins. We interpret the veins as being composed of carbonates, similar to those found in aqueously altered carbonaceous chondrite meteorites. If the veins on Bennu are carbonates, fluid flow and hydrothermal deposition on Bennu's parent body would have occurred on kilometer scales for thousands to millions of years. This suggests large-scale, open-system hydrothermal alteration of carbonaceous asteroids in the early Solar System.

Original languageEnglish
Article numberabc3557
JournalScience
Volume370
Issue number6517
DOIs
StatePublished - Nov 6 2020

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