The discovery and characterization of (594913) 'Ayló'chaxnim, a kilometre sized asteroid inside the orbit of Venus
Author
Bolin, B.T.Ahumada, T.
Van Dokkum, P.
Fremling, C.
Granvik, M.
Hardegree-Ullman, K.K.
Harikane, Y.
Purdum, J.N.
Serabyn, E.
Southworth, J.
Zhai, C.
Affiliation
Steward Observatory, University of ArizonaIssue Date
2022-08-13
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Oxford University PressCitation
Bryce T Bolin, T Ahumada, P van Dokkum, C Fremling, M Granvik, K K Hardegree-Ullman, Y Harikane, J N Purdum, E Serabyn, J Southworth, C Zhai, The discovery and characterization of (594913) 'Ayló'chaxnim, a kilometre sized asteroid inside the orbit of Venus, Monthly Notices of the Royal Astronomical Society: Letters, Volume 517, Issue 1, November 2022, Pages L49–L54, https://doi.org/10.1093/mnrasl/slac089Rights
Published by Oxford University Press on behalf of Royal Astronomical Society 2022. This work is written by (a) US Government employee(s) and is in the public domain in the US.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
Near-Earth asteroid population models predict the existence of bodies located inside the orbit of Venus. Despite searches up to the end of 2019, none had been found. We report discovery and follow-up observations of (594913) 'Ayló'chaxnim, an asteroid with an orbit entirely interior to Venus. (594913) 'Ayló'chaxnim has an aphelion distance of ∼0.65 au, is ∼2 km in diameter and is red in colour. The detection of such a large asteroid inside the orbit of Venus is surprising given their rarity according to near-Earth asteroid population models. As the first officially numbered and named asteroid located entirely within the orbit of Venus, we propose that the class of interior to Venus asteroids be referred to as 'Ayló'chaxnim asteroids. © 2022 Published by Oxford University Press on behalf of Royal Astronomical Society.Note
Public domain articleISSN
1745-3925Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1093/mnrasl/slac089
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Except where otherwise noted, this item's license is described as Published by Oxford University Press on behalf of Royal Astronomical Society 2022. This work is written by (a) US Government employee(s) and is in the public domain in the US.