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pro vyhledávání: '"Emel’yanenko, V. V."'
Autor:
Emel'yanenko, V. V.
Aims. We study the dynamical evolution of a system consisting of the giant planets and a massive planetesimal disk over the age of the Solar System. The main question addressed in this study is whether distant trans-Neptunian objects could have come
Externí odkaz:
http://arxiv.org/abs/2205.12297
Autor:
Emel'yanenko, V. V.
Publikováno v:
Solar System Research 55 (2021) 341-347
Dynamical features of a massive disk of distant trans-Neptunian objects are considered in the model of the formation of small bodies in the Hill region of a giant gas-dust clump that arose as a result of gravitational instability and fragmentation of
Externí odkaz:
http://arxiv.org/abs/2201.01571
Autor:
Emel'yanenko, V. V.
Publikováno v:
A&A 642, L20 (2020)
Context: The discovery of distant trans-Neptunian objects has led to heated discussions about the structure of the outer Solar System. Aims: We study the dynamical evolution of small bodies from the Hill regions of migrating giant gaseous clumps that
Externí odkaz:
http://arxiv.org/abs/2010.07281
Autor:
Emel'yanenko, V. V.
New data on the distribution of distant trans-Neptunian objects and on the properties of comets indicate the importance of dynamical processes in the outer part of the protoplanetary disk in the formation of the observed structure of the Solar system
Externí odkaz:
http://arxiv.org/abs/2001.01205
Autor:
Emel'yanenko, V. V.
Publikováno v:
Solar System Research, 2018, Volume 52, 382-391
The data obtained in the recent Rosetta space mission to comet 67P/Churyumov-Gerasimenko have had a profound impact on the understanding of the nature of comets. In addition to revising the notions on the physical properties and structure of comets,
Externí odkaz:
http://arxiv.org/abs/1912.10747
Akademický článek
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Publikováno v:
Earth, Moon, and Planets, 2013, Volume 110, Issue 1-2, pp. 105-130
A numerical simulation of the Oort cloud is used to explain the observed orbital distributions and numbers of Jupiter-family and Halley-type short-period comets. Comets are given initial orbits with perihelion distances between 5 and 36 AU, and evolv
Externí odkaz:
http://arxiv.org/abs/1402.1339
Autor:
Emel'yanenko, V. V.1 (AUTHOR) vvemel@inasan.ru
Publikováno v:
Solar System Research. Jul2021, Vol. 55 Issue 4, p341-347. 7p.
Akademický článek
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Autor:
Emel’yanenko, V. V.1 vvemel@inasan.ru
Publikováno v:
Solar System Research. Sep2018, Vol. 52 Issue 5, p382-391. 10p.