Abstract
The orbit of an active asteroid (457175) 2008 GO98/362P was obtained taking into account non-gravitational acceleration based on the Marsden model. The presence of systematic deviations was revealed in the 2016 observations prior to the cometary activity. The possibility of a collision with a minor body was considered. For this, the momenta of reaching the minimum distances (MOID, Minimum Orbit Intersection Distance) between the orbits of the asteroid (457175) and 585 961 numbered, and 536 561 unnumbered asteroids (according to the status in the Minor Planet Center catalogs of observations as of October 2021) were found. The maximum number of orbital rendezvouses falls on the time when the asteroid was passing in the vicinity of the ascending node, which suggests the possibility of a collision leading to the fragmentation of the main body. Two separation scenarios are considered and orbit variation of the main body and possible fragments are estimated. For the formed fragment, the heliocentric velocity variation amounted to \(dv=0.148\) m s\({}^{-1}\) and non-gravitational acceleration was \(A_{3}=-12.5\times 10^{-8}\) AU day\({}^{-2}\). The main body dynamics did not vary significantly.
Notes
https://iaaras.ru/dept/lsbss/minor_elem/ for February 22, 2022.
V.B. Kuznetsov refined the elements of their orbits according to the MPC observation catalog state as of October 2021.
https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=457175 for March 1, 2022.
REFERENCES
E. Everhart, Bull. Amer. Astron. Soc. 5, 389 (1973).
R. Gil-Hutton and E. García-Migani, Astron. and Astrophys. 590, id. A111 (2016).
D. Jewitt, Astron. J. 143 (3), article id. 66 (2012).
D. Jewitt, H. Hsieh, and J. Agarwal, Asteroids IV, Ed. by P. Michel, F. DeMeo and W. Bottke (University of Arizona Press, Tucson, 2015), pp. 221–241.
G. I. Kokhirova, O. V. Ivanova, F. D. Rakhmatullaeva, et al., Advances in Space Research 67 (1), 639 (2021).
B. G. Marsden, Z. Sekanina, and D. K. Yeomans, Astron. J. 78, 211 (1973).
E. M. Standish, JPL planetary and lunar ephemerides, DE405/LE405, JPL Interoffice Memorandum, Pasadena, 312.F-98-048, 1–18 (1998).
ACKNOWLEDGMENTS
This study used the data and/or the services provided by the Minor Planet Center of the International Astronomical Union. The author thanks the senior researcher of IAA RAS V.B. Kuznetsov for his help with the calculations. The author is also grateful to the anonymous reviewers for comments and recommendations, the account of which allowed to improve the work.
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
The author declares no conflict of interest.
Additional information
Translated by E. Porphiryeva
Rights and permissions
About this article
Cite this article
Chernetenko, Y.A. Causes of Asteroid (457175) 2008 GO98/362P Activity. Astrophys. Bull. 78, 94–99 (2023). https://doi.org/10.1134/S1990341323010030
Received:
Revised:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1990341323010030