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dc.contributor.authorChesley, S. R.
dc.contributor.authorFrench, A. S.
dc.contributor.authorDavis, A. B.
dc.contributor.authorJacobson, R. A.
dc.contributor.authorBrozović, M.
dc.contributor.authorFarnocchia, D.
dc.contributor.authorSelznick, S.
dc.contributor.authorLiounis, A. J.
dc.contributor.authorHergenrother, C. W.
dc.contributor.authorMoreau, M. C.
dc.contributor.authorPelgrift, J.
dc.contributor.authorLessac‐Chenen, E.
dc.contributor.authorMolaro, J. L.
dc.contributor.authorPark, R. S.
dc.contributor.authorRozitis, B.
dc.contributor.authorScheeres, D. J.
dc.contributor.authorTakahashi, Y.
dc.contributor.authorVokrouhlický, D.
dc.contributor.authorWolner, C. W. V.
dc.contributor.authorAdam, C.
dc.contributor.authorBos, B. J.
dc.contributor.authorChristensen, E. J.
dc.contributor.authorEmery, J. P.
dc.contributor.authorLeonard, J. M.
dc.contributor.authorMcMahon, J. W.
dc.contributor.authorNolan, M. C.
dc.contributor.authorShelly, F. C.
dc.contributor.authorLauretta, D. S.
dc.date.accessioned2021-04-17T00:36:38Z
dc.date.available2021-04-17T00:36:38Z
dc.date.issued2020-07-08
dc.identifier.citationChesley, S. R., French, A. S., Davis, A. B., Jacobson, R. A., Brozović, M., Farnocchia, D., ... & Lauretta, D. S. (2020). Trajectory estimation for particles observed in the vicinity of (101955) Bennu. Journal of Geophysical Research: Planets, 125(9), e2019JE006363.en_US
dc.identifier.issn2169-9097
dc.identifier.doi10.1029/2019je006363
dc.identifier.urihttp://hdl.handle.net/10150/657781
dc.description.abstractWe analyze the trajectories of 313 particles seen in the near-Bennu environment between December 2018 and September 2019. Of these, 65% follow suborbital trajectories, 20% undergo more than one orbital revolution around the asteroid, and 15% directly escape on hyperbolic trajectories. The median lifetime of these particles is similar to 6 hr. The trajectories are sensitive to Bennu's gravitational field, which allows us to reliably estimate the spherical harmonic coefficients through degree 8 and to resolve nonuniform mass distribution through degree 3. The particles are perturbed by solar radiation pressure, enabling effective area-to-mass ratios to be estimated. By assuming that particles are oblate ellipsoids of revolution, and incorporating photometric measurements, we find a median axis ratio of 0.27 and diameters for equivalent-volume spheres ranging from 0.22-6.1 cm, with median 0.74 cm. Our size distribution agrees well with that predicted for fragmentation due to diurnal thermal cycling. Detailed models of known accelerations do not produce a match to the observed trajectories, so we also estimate empirical accelerations. These accelerations appear to be related to mismodeling of radiation pressure, but we cannot rule out contributions from mass loss. Most ejections take place at local solar times in the afternoon and evening (12:00-24:00), although they occur at any time of day. We independently identify ten ejection events, some of which have previously been reported. We document a case where a particle ricocheted off the surface, revealing a coefficient of restitution 0.57 +/- 0.01 and demonstrating that some apparent ejections are not related to surface processes. Plain Language Summary The Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer (OSIRIS-REx) mission discovered that near-Earth asteroid (101955) Bennu is periodically ejecting small particles from its surface, placing it in the uncommon class of "active asteroids." We linked together individual detections of ejected particles and used numerical models of the forces acting on them to ascertain their trajectories and fates. We found that most particles have suborbital trajectories, meaning they fall back to Bennu's surface shortly after being ejected, but some orbit Bennu for days at a time, and some escape directly into space. From the particle trajectories, we are able to estimate their sizes (comparable to pebbles, from a few millimeters to a few centimeters in diameter) and shapes (probably flake like). Their trajectories also make it possible to estimate Bennu's gravity field more precisely than spacecraft measurements and help shed light on the possible causes of the ejections.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.titleTrajectory Estimation for Particles Observed in the Vicinity of (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.issue9
refterms.dateFOA2021-04-17T00:36:38Z


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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.