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dc.contributor.authorScheeres, D. J.
dc.contributor.authorMcMahon, J. W.
dc.contributor.authorBrack, D. N.
dc.contributor.authorFrench, A. S.
dc.contributor.authorChesley, S. R.
dc.contributor.authorFarnocchia, D.
dc.contributor.authorVokrouhlický, D.
dc.contributor.authorBallouz, R.‐L.
dc.contributor.authorEmery, J. P.
dc.contributor.authorRozitis, B.
dc.contributor.authorNolan, M. C.
dc.contributor.authorHergenrother, C. W.
dc.contributor.authorLauretta, D. S.
dc.date.accessioned2021-04-03T02:38:37Z
dc.date.available2021-04-03T02:38:37Z
dc.date.issued2020-03-11
dc.identifier.citationScheeres, D. J., McMahon, J. W., Brack, D. N., French, A. S., Chesley, S. R., Farnocchia, D., ... & Lauretta, D. S. (2020). Particle ejection contributions to the rotational acceleration and orbit evolution of Asteroid (101955) Bennu. Journal of Geophysical Research: Planets, 125(3), e2019JE006284.en_US
dc.identifier.issn2169-9097
dc.identifier.doi10.1029/2019je006284
dc.identifier.urihttp://hdl.handle.net/10150/657617
dc.description.abstractThis paper explores the implications of the observed Bennu particle ejection events for that asteroid's spin rate and orbit evolution, which could complicate interpretation of the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) and Yarkovsky effects on this body's spin rate and orbital evolution. Based on current estimates of particle ejection rates, we find that the overall contribution to Bennu's spin and orbital drift is small or negligible as compared to the Yarkovsky and YORP effects. However, if there is a large unseen component of smaller mass ejections or a strong directionality in the ejection events, it could constitute a significant contribution that could mask the overall YORP effect. This means that the YORP effect may be stronger than currently assumed. The analysis is generalized so that the particle ejection effect can be assessed for other bodies that may be subject to similar mass loss events. Further, our model can be modified to address different potential mechanisms of particle ejection, which are a topic of ongoing study. Plain Language Summary The near-Earth asteroid Bennu has been observed to be ejecting particles of rock from its surface. The possible effect of these particle ejections on the asteroid's spin rate and orbit is studied using numerical modeling. We show that the effect is likely minimal, although for certain ejection geometries, their effect on the spin rate could be more important. The loss of mass caused by the particle ejections would likely limit the asteroid's rotational acceleration, suggesting that the acceleration effect on this body may be larger than assumed. We consider how different mechanisms of ejection could be modeled using our approach.en_US
dc.description.sponsorshipNational Aeronautics and Space Administrationen_US
dc.language.isoenen_US
dc.publisherAMER GEOPHYSICAL UNIONen_US
dc.rights© 2020. The Authors. This is an open access article under the terms of the Creative Commons Attribution License.en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.titleParticle Ejection Contributions to the Rotational Acceleration and Orbit Evolution of Asteroid (101955) Bennuen_US
dc.typeArticleen_US
dc.identifier.eissn2169-9100
dc.contributor.departmentUniv Arizona, Lunar & Planetary Laben_US
dc.identifier.journalJOURNAL OF GEOPHYSICAL RESEARCH-PLANETSen_US
dc.description.noteOpen access articleen_US
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en_US
dc.eprint.versionFinal published versionen_US
dc.source.journaltitleJournal of Geophysical Research: Planets
dc.source.volume125
dc.source.issue3
refterms.dateFOA2021-04-03T02:38:46Z


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© 2020. The Authors. This is an open access article under the terms of the Creative Commons Attribution License.
Except where otherwise noted, this item's license is described as © 2020. The Authors. This is an open access article under the terms of the Creative Commons Attribution License.