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Effects of tidal torques on 1I/2017 U1 (‘Oumuamua)

Abstract:
As observations of ‘Oumuamua were collected well into the outbound component of its hyperbolic orbit, it is not obvious what effects Sol had on its rotational dynamics. Therefore, we simulate ‘Oumuamua as a prolate spheroid and triaxial ellipsoid of uniform mass density and show that the experimentally observed angular velocities remain largely unchanged during ‘Oumuamua’s flyby, supporting previous work suggesting that, in the absence of a collision during its interstellar journey, the asteroid was tumbling in the same manner as when it left its original solar system.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1016/j.icarus.2018.04.005

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Mathematical Institute
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Mathematical Institute
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Mathematical Institute
Role:
Author


Publisher:
Elsevier
Journal:
Icarus More from this journal
Volume:
311
Pages:
170-174
Publication date:
2018-04-04
Acceptance date:
2018-04-03
DOI:
ISSN:
0019-1035


Keywords:
Pubs id:
pubs:843414
UUID:
uuid:c80c9ccd-5cc4-4f2d-a92c-0319f01d7c4a
Local pid:
pubs:843414
Source identifiers:
843414
Deposit date:
2018-04-20

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