Zobrazeno 1 - 10
of 14
pro vyhledávání: '"V. M. Chepurova"'
Publikováno v:
Odessa Astronomical Publications, Vol 9, Iss 0, Pp 193-194 (2017)
Solar system comets come from a relict reservoir of cometary bodies (CB). The reservoir consists of two components of common origin, but highly different spatial, dynamical and kinematical characteristics: 1. Dynamically stable on cosmogonic time-sca
Externí odkaz:
https://doaj.org/article/f6370b9ca474445da8aedb65fc59101a
Autor:
N. V. Kulikova, V. M. Chepurova
Publikováno v:
Вісник Астрономічної школи, Vol 6, Iss 1, Pp 98-103 (2009)
So far we investigated the nonperturbation dynamics of meteoroid complexes. The numerical integration of the differential equations of motion in the N-body problem by the Everhart algorithm (N=2–6) and introduction of the intermediate hyperbolic or
Externí odkaz:
https://doaj.org/article/2ad69056ec304072a0d21029fccf90ea
Autor:
N. Kulikova, V. M. Chepurova
Publikováno v:
Астрономия-2018. Том 2.
Autor:
V. M. Chepurova, N. V. Kulikova
Publikováno v:
Вісник Астрономічної школи, Vol 6, Iss 1, Pp 98-103 (2009)
So far we investigated the nonperturbation dynamics of meteoroid complexes. The numerical integration of the differential equations of motion in the N-body problem by the Everhart algorithm (N=2–6) and introduction of the intermediate hyperbolic or
Autor:
V. M. Chepurova, N. V. Kulikova
Publikováno v:
Astronomical & Astrophysical Transactions. 25:291-297
Autor:
V. M. Chepurova, N. V. Kulikova
Publikováno v:
Astronomical & Astrophysical Transactions. 23:469-474
Computer simulation of the formation of meteoroid bodies formed in Tempel–Tuttle comet disintegration in all its known appearances is performed. Simulation results are analysed according to the retrospective review of observational data for this co
Publikováno v:
Astronomical & Astrophysical Transactions. 21:279-291
Publikováno v:
Astronomical & Astrophysical Transactions. 17:351-354
Solar system (SS) comets come from a relict reservoir (RR) of cometary bodies (CB). The reservoir consists of two components of common origin, but highly different spatial, dynamical and kinematical characteristics: (1) a dynamically stable component
Autor:
V. M. Chepurova, F. A. Tsitsin
Publikováno v:
Astronomical & Astrophysical Transactions. 16:49-52
The possible existence and dynamical evolution of a comet relict reservoir among the giant planets is examined. Permanent gravitational encounters with planets and collisions between cometary nuclei tend to throw them out highly eccentric strongly pe
Publikováno v:
Astronomical & Astrophysical Transactions. 15:263-269
The results of computer experiments on modelling stochastic dynamics in a planetary four-body problem are discussed. A scissors effect in this problem was obtained. This result was first observed by the authors as a solution for a stochastic planetar