The dynamical evolution of planetary systems HD12661, υ Andromedae, and some model systems is investigated on time scale of the order 105—107 years. Averaging the canonical equations of the planetary movement is performed by the Hori—Deprit method. The systems of first and second order approximation with respect to masses have been obtained and numerically integrated.
Translated title of the contributionStudy of Stability of a Planetary System on a Cosmogonic Time Scale
Original languageRussian
Title of host publicationФизика Космоса
Subtitle of host publicationТруды 49-й Международной студенческой научной конференции, Екатеринбург, 27-31 января, 2020 г.
Place of PublicationЕкатеринбург
PublisherИздательство Уральского Федерального Университета
Pages180-181
Number of pages2
DOIs
StatePublished - Jan 2020
Event49-я Международная студенческая научная конференция "Физика космоса" - Екатеринбург, Russian Federation
Duration: 27 Jan 202031 Jan 2020

Conference

Conference49-я Международная студенческая научная конференция "Физика космоса"
Country/TerritoryRussian Federation
CityЕкатеринбург
Period27/01/2031/01/20

    Scopus subject areas

  • Astronomy and Astrophysics

ID: 52637394