Journal article
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
Actions
Access Document
- Files:
-
-
(Preview, Accepted manuscript, pdf, 1.4MB, Terms of use)
-
- Publisher copy:
- 10.1016/j.icarus.2018.04.005
Authors
- 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
Terms of use
- Copyright holder:
- Elsevier Inc
- Copyright date:
- 2018
- Notes:
- Copyright © 2018 Elsevier Inc. This is the accepted manuscript version of the article. The final version is available online from Elsevier at: https://doi.org/10.1016/j.icarus.2018.04.005
If you are the owner of this record, you can report an update to it here: Report update to this record