Dynamical evolution of asteroid pairs on close orbits

Please use this identifier to cite or link to this item: http://elar.urfu.ru/handle/10995/101555

Title:	Dynamical evolution of asteroid pairs on close orbits
Authors:	Kuznetsov, E. D. Glamazda, D. V. Kaiser, G. T. Krushinsky, V. V. Popov, A. A. Safronova, V. S. Shagabutdinov, A. A. Skripnichenko, P. V. Vibe, Y. S.
Issue Date:	2018
Publisher:	Cambridge University Press
Citation:	Dynamical evolution of asteroid pairs on close orbits / E. D. Kuznetsov, D. V. Glamazda, G. T. Kaiser, et al. — DOI 10.1017/S1743921319003260 // Proceedings of the International Astronomical Union. — 2018. — Vol. 14. — Iss. A30. — P. 16-.
Abstract:	We apply Kholshevnikov metrics defined in the space of Keplerian orbits to search for asteroids in close orbits. We showed that the Yarkovsky effect was required to take into account accurately to carry out precise simulation of dynamical evolution of the asteroid pairs. Determination of physical and rotational parameters of asteroids is needed to solve this problem. © International Astronomical Union 2020.
URI:	http://elar.urfu.ru/handle/10995/101555
Access:	info:eu-repo/semantics/openAccess
SCOPUS ID:	85080905497
PURE ID:	12417872 69a1cfd6-f988-4d36-8b85-8fb538a31752
ISSN:	17439213
DOI:	10.1017/S1743921319003260
Appears in Collections:	Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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