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Jenniskens.Icarus.1-s2.0-S0019 ...
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Author
Jenniskens, PeterLauretta, Dante S.
Koelbel, Lindsey R.
Towner, Martin C.
Bland, Phil
Heathcote, Steve
Abbott, Timothy M.C.
Jehin, Emmanuel
Hanke, Toni
Fahl, Elise
van Wyk, Rynault
Cooper, Tim
Baggaley, Jack W.
Samuels, Dave
Gural, Peter S.
Affiliation
Lunar and Planetary Laboratory, University of ArizonaIssue Date
2023-04
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Elsevier BVCitation
Jenniskens, P., Lauretta, D. S., Koelbel, L. R., Towner, M. C., Bland, P., Heathcote, S., Abbott, T. M. C., Jehin, E., Hanke, T., Fahl, E., van Wyk, R., Cooper, T., Baggaley, J. W., Samuels, D., & Gural, P. S. (2023). An observing campaign to search for meteoroids of Bennu at Earth. Icarus, 394.Journal
IcarusRights
© 2022 The Authors. Published by Elsevier Inc. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).Collection Information
This 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.Abstract
An observing campaign was conducted in the Southern Hemisphere using low-light video camera triangulation to measure the trajectories and orbits of meteoroids with a possible origin at asteroid Bennu. New CAMS (Camera for Allsky Meteor Surveillance) video camera networks were established in Australia, Chile, and Namibia, and networks in New Zealand and South Africa were expanded. During observing periods in September 2019, 2020, and 2021, we measured 7672, 4936, and 5890 orbits, respectively. Based on the non-detection of predicted meteoroid trail encounters, Bennu's meteoroid production rate was <1.5 kg/s during 1500–1800 CE. Indeed, the current production rate is many orders of magnitude lower. Bennu may have an associated annual meteoroid stream of much older ejecta at a particle flux density of ≤1.3 × 10−6 km−2 h−1, based on seven Bennu-like orbits detected during the first three years of observations.Note
Open access articleISSN
0019-1035Version
Final published versionSponsors
National Aeronautics and Space Administrationae974a485f413a2113503eed53cd6c53
10.1016/j.icarus.2022.115403
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Except where otherwise noted, this item's license is described as © 2022 The Authors. Published by Elsevier Inc. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).

