Back to Search Start Over

The unexpected surface of asteroid (101955) Bennu.

Authors :
Lauretta, D. S.
DellaGiustina, D. N.
Bennett, C. A.
Golish, D. R.
Becker, K. J.
Balram-Knutson, S. S.
Barnouin, O. S.
Becker, T. L.
Bottke, W. F.
Boynton, W. V.
Campins, H.
Clark, B. E.
Connolly, H. C.
Drouet d'Aubigny, C. Y.
Dworkin, J. P.
Emery, J. P.
Enos, H. L.
Hamilton, V. E.
Hergenrother, C. W.
Howell, E. S.
Source :
Nature; 4/4/2019, Vol. 568 Issue 7750, p55-60, 6p, 2 Black and White Photographs, 1 Diagram, 5 Charts, 4 Graphs
Publication Year :
2019

Abstract

NASA'S Origins, Spectral Interpretation, Resource Identification and Security-Regolith Explorer (OSIRIS-REx) spacecraft recently arrived at the near-Earth asteroid (101955) Bennu, a primitive body that represents the objects that may have brought prebiotic molecules and volatiles such as water to Earth1. Bennu is a low-albedo B-type asteroid2 that has been linked to organic-rich hydrated carbonaceous chondrites3. Such meteorites are altered by ejection from their parent body and contaminated by atmospheric entry and terrestrial microbes. Therefore, the primary mission objective is to return a sample of Bennu to Earth that is pristine—that is, not affected by these processes4. The OSIRIS-REx spacecraft carries a sophisticated suite of instruments to characterize Bennu's global properties, support the selection of a sampling site and document that site at a sub-centimetre scale5–11. Here we consider early OSIRIS-REx observations of Bennu to understand how the asteroid's properties compare to pre-encounter expectations and to assess the prospects for sample return. The bulk composition of Bennu appears to be hydrated and volatile-rich, as expected. However, in contrast to pre-encounter modelling of Bennu's thermal inertia12 and radar polarization ratios13—which indicated a generally smooth surface covered by centimetre-scale particles—resolved imaging reveals an unexpected surficial diversity. The albedo, texture, particle size and roughness are beyond the spacecraft design specifications. On the basis of our pre-encounter knowledge, we developed a sampling strategy to target 50-metre-diameter patches of loose regolith with grain sizes smaller than two centimetres4. We observe only a small number of apparently hazard-free regions, of the order of 5 to 20 metres in extent, the sampling of which poses a substantial challenge to mission success. Observations of asteroid (101955) Bennu with NASA's OSIRIS-REx spacecraft reveal an unexpected surficial diversity that poses a challenge to the success of the sample-return mission. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00280836
Volume :
568
Issue :
7750
Database :
Complementary Index
Journal :
Nature
Publication Type :
Academic Journal
Accession number :
135797179
Full Text :
https://doi.org/10.1038/s41586-019-1033-6