|
ИСТИНА |
Войти в систему Регистрация |
ИСТИНА ИНХС РАН |
||
Probabilistic analysis of the cosmic masses accumulations in the Solar systemтезисы доклада
- Авторы: Salnikova Tatiana, Samokhin Alexander
- Сборник: The Eleventh Moscow Solar System Symposium (11M-S3). 5–9 October 2020
- Тезисы
- Год издания: 2020
- Место издания: Space Research Institute of the Russian Academy of Sciences (IKI) Moscow, Russia
- Номер статьи: 285-285, 11MS3-SB-12
- Аннотация: Keywords:numerical simulation, cosmic masses, asteroids, dust particles, stable configuration,elliptical orbits, circle orbits, steady statesIntroduction:Cosmic masses: asteroids, small planets, dust particles and dust clouds fill theinterplanetary space. There is still no answer, why instead of one planet, wehave an asteroid belt stable configuration with small planets, such as Ceres.There are many hypotheses for the belt conformation. For example, Sean N.Raymond and Andre Izidoro suggested in [1] that in fact there was no planetaryembryo, and the belt was formed from the debris of the planets duringtheir formation and immediately took its current form. Doi: 0.21046/11MS3-2020
- Добавил в систему: Самохин Александр Сергеевич