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Constraining the Surface Exposure Age of Asteroid Bennu Using Cosmogenic Radionuclides in an OSIRIS-REx Aggregate Sample and Individual ParticlesObservations by NASA’s OSIRIS-REx spacecraft of asteroid Bennu revealed evidence that this small rubble-pile asteroid experiences several active surface processes that likely control its recent surface exposure history. In October 2020, the spacecraft collected a surface sample from a relatively young ~20 m diameter crater (Hokioi) on asteroid Bennu, and the sample was successfully delivered to Earth on September 24, 2023.

Based on the population of craters >50 m diameter, Bennu’s surface is 0.1–1 Ga old, but the old surface is affected by recent processes including smaller meteoroid impacts, mass movement, and particle ejections. The sampling location within Hokioi crater was selected based on its relatively flat surface devoid of large boulders, but the crater floor is also believed to be one of the youngest surfaces on asteroid Bennu, with an age of <100 kyr. As the crater is ~2 m deep, the samples that were collected by OSIRIS-REx may have been relatively shielded from cosmic rays during most of its recent history. This scenario is different from the samples that were collected by Hayabusa2 from asteroid Ryugu, where cosmogenic noble gas and radionuclides indicate cosmic-ray exposure (CRE) ages of ~5 Myr near the surface.

Our goal is to understand the recent exposure history of surface samples of asteroid Bennu utilizing radionuclides (10Be, 26Al, 36Cl, 41Ca) produced by both galactic (GCR) and solar (SCR) cosmic rays. With half- lives ranging from 0.1 to 1.36 million years (Myr), the concentrations of these cosmogenic nuclides provide information on the duration and exposure conditions (irradiation depth) of these samples on a timescale of a few Myr. This work will test one of the OSIRIS-REx mission’s driving hypotheses about asteroid Bennu’s recent evolution: that Hokioi crater is part of a population of small (25 m) spectrally red craters on Bennu that are less than 0.1 Myr old.
Document ID
20240000345
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
K. C. Welten ORCID
(University of California, Berkeley Berkeley, United States)
K. Nishiizumi ORCID
(University of California, Berkeley Berkeley, United States)
M. W. Caffee ORCID
(Purdue University West Lafayette West Lafayette, United States)
J. Masarik ORCID
(Comenius University Bratislava Bratislava, Slovakia)
J. J. Barnes
(University of Arizona Tucson, United States)
A. N. Nguyen
(Johnson Space Center Houston, United States)
H. C. Connolly ORCID
(University of Arizona Tucson, United States)
D. S. Lauretta ORCID
(University of Arizona Tucson, United States)
Date Acquired
January 9, 2024
Publication Date
March 11, 2024
Publication Information
Publisher: Lunar and Planetary Institute
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: 55th Lunar and Planetary Science Conference (LPSC)
Location: The Woodlands, TX
Country: US
Start Date: March 11, 2024
End Date: March 15, 2024
Sponsors: Lunar and Planetary Institute, National Aeronautics and Space Administration
Funding Number(s)
WBS: 828928.04.02.04.05
CONTRACT_GRANT: NNM10AA11C
CONTRACT_GRANT: 80NSSC22K1693
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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