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Zhurnal Tekhnicheskoi Fiziki, 2023, Volume 93, Issue 12, Pages 1778–1781
DOI: https://doi.org/10.61011/JTF.2023.12.56820.f251-23 (Mi jtf7161) 		 
International Conference PhysicA.SPb 23-27 October, 2023 St. Petersburg
Astronomy and Astrophysics

Analysis of the dynamic parameters of the Cancrids meteor shower and its drift motion

M. V. Sergienkoa, Yu. A. Nefed'eva, A. O. Andreevab

a Kazan (Volga Region) Federal University, Kazan, Russia
b Kazan State Power Engineering University, 420066 Kazan, Russia
Full-text PDF (458 kB)
DOI: https://doi.org/10.61011/JTF.2023.12.56820.f251-23
Abstract: We consider the Cancrids meteor shower and analyze its dynamical parameters. For each branch of the shower we determined radiants, their displacements, and radiation areas. The dependences of the semi-major axis and eccentricity on magnitude were studied. Resonances from Jupiter were determined for the meteor shower. It is concluded that the branches of the shower have different evolutionary mechanisms of origin.
Keywords: meteor shower, radiants, meteor complex, resonances.
Funding agency Grant number
Russian Science Foundation 22-72-10059
The work was supported by the Russian Science Foundation, grant No. 22-72-10059.
Received: 11.05.2023
Revised: 05.09.2023
Accepted: 30.10.2023
Bibliographic databases:
Document Type: Article
Language: Russian
Citation: M. V. Sergienko, Yu. A. Nefed'ev, A. O. Andreev, “Analysis of the dynamic parameters of the Cancrids meteor shower and its drift motion”, Zhurnal Tekhnicheskoi Fiziki, 93:12 (2023), 1778–1781
Citation in format AMSBIB
\Bibitem{SerNefAnd23}
\by M.~V.~Sergienko, Yu.~A.~Nefed'ev, A.~O.~Andreev
\paper Analysis of the dynamic parameters of the Cancrids meteor shower and its drift motion
\jour Zhurnal Tekhnicheskoi Fiziki
\yr 2023
\vol 93
\issue 12
\pages 1778--1781
\mathnet{http://mi.mathnet.ru/jtf7161}
\crossref{https://doi.org/10.61011/JTF.2023.12.56820.f251-23}
\elib{https://elibrary.ru/item.asp?id=60019354}
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