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Journal article

The operational environment and rotational acceleration of asteroid (101955) Bennu from OSIRIS-REx observations

Abstract:
During its approach to asteroid (101955) Bennu, NASA's Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) spacecraft surveyed Bennu's immediate environment, photometric properties, and rotation state. Discovery of a dusty environment, a natural satellite, or unexpected asteroid characteristics would have had consequences for the mission's safety and observation strategy. Here we show that spacecraft observations during this period were highly sensitive to satellites (sub-meter scale) but reveal none, although later navigational images indicate that further investigation is needed. We constrain average dust production in September 2018 from Bennu's surface to an upper limit of 150 g s-1 averaged over 34 min. Bennu's disk-integrated photometric phase function validates measurements from the pre-encounter astronomical campaign. We demonstrate that Bennu's rotation rate is accelerating continuously at 3.63 ± 0.52 × 10-6 degrees day-2, likely due to the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect, with evolutionary implications.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1038/s41467-019-09213-x

Authors


More by this author
Role:
Author
ORCID:
0000-0001-8316-0680
More by this author
Role:
Author
ORCID:
0000-0003-3841-9977



Publisher:
Springer Nature
Journal:
Nature Communications More from this journal
Volume:
10
Issue:
1
Article number:
1291
Publication date:
2019-03-19
Acceptance date:
2019-02-26
DOI:
EISSN:
2041-1723
Pmid:
30890725


Language:
English
Keywords:
Pubs id:
pubs:986801
UUID:
uuid:a795acd2-4c22-4afc-af12-fd7f128942b9
Local pid:
pubs:986801
Source identifiers:
986801
Deposit date:
2019-05-27

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