OSSOS. XXIII. 2013 VZ70 and the Temporary Coorbitals of the Giant Planets
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Alexandersen, M.Greenstreet, S.
Gladman, B.J.
Bannister, M.T.
Chen, Y.-T.
Gwyn, S.D.J.
Kavelaars, J.J.
Petit, J.-M.
Volk, K.
Lehner, M.J.
Wang, S.-Y.
Affiliation
Lunar and Planetary Laboratory, University of ArizonaIssue Date
2021
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Alexandersen, M., Greenstreet, S., Gladman, B. J., Bannister, M. T., Chen, Y.-T., Gwyn, S. D. J., Kavelaars, J. J., Petit, J.-M., Volk, K., Lehner, M. J., & Wang, S.-Y. (2021). OSSOS. XXIII. 2013 VZ70 and the Temporary Coorbitals of the Giant Planets. Planetary Science Journal.Journal
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Copyright © 2021 The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.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
We present the discovery of 2013 VZ70, the first known horseshoe coorbital companion of Saturn. Observed by the Outer Solar System Origins Survey for 4.5 yr, the orbit of 2013 VZ70 is determined to high precision, revealing that it currently is in “horseshoe” libration with the planet. This coorbital motion will last at least thousands of years but ends ∼10 kyr from now; 2013 VZ70 is thus another example of the already-known “transient coorbital” populations of the giant planets, with this being the first known prograde example for Saturn (temporary retrograde coorbitals are known for Jupiter and Saturn). We present a theoretical steady-state model of the scattering population of trans-Neptunian origin in the giant planet region (2-34 au), including the temporary coorbital populations of the four giant planets. We expose this model to observational biases using survey simulations in order to compare the model to the real detections made by a set of well-characterized outer solar system surveys. While the observed number of coorbitals relative to the scattering population is higher than predicted, we show that the number of observed transient coorbitals of each giant planet relative to each other is consistent with a trans-Neptunian source. © 2021. The Author(s). Published by the American Astronomical Society.Note
Open access journalISSN
2632-3338Version
Final published versionae974a485f413a2113503eed53cd6c53
10.3847/PSJ/ac1c6b
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Except where otherwise noted, this item's license is described as Copyright © 2021 The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.