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Probabilistic analysis of the cosmic masses accumulations in the Solar systemдоклад на конференции
- Авторы: Salnikova Tatiana, Samokhin Alexander
- Международная Конференция (Симпозиум) : THE ELEVENTH MOSCOW SOLAR SYSTEM SYMPOSIUM 11M-S3.
- Даты проведения конференции: 5-9 октября 2020
- Дата доклада: 8 октября 2020
- Тип доклада: Устный
- Докладчик: Samokhin Alexander
- Место проведения: Москва, Россия
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Аннотация доклада:
KEYWORDS: numerical simulation, cosmic masses, asteroids, dust particles, stable configuration, elliptical orbits, circle orbits, steady states INTRODUCTION: Cosmic masses: asteroids, small planets, dust particles and dust clouds fill the interplanetary space. There is still no answer, why instead of one planet, we have 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 planetary embryo, and the belt was formed from the debris of the planets during their formation and immediately took its current form.
- Добавил в систему: Самохин Александр Сергеевич