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On the possibility of formation of carbonaceous chondrites on small bodiesстатья
- Автор: Busarev V.V.
- Сборник: Reports of International Astronomical Congress "Astrokazan-2011"
- Год издания: 2011
- Место издания: Изд-во Казанского федерального ун-та Казань
- Первая страница: 22
- Последняя страница: 30
- Аннотация: Heliocentric distribution of spectral (taxonomic) types of asteroids characterizes the structure of the Main asteroid belt on the content of matter. The structure, in turn, bears the "imprint" of the primary dynamical, physical and chemical processes in the solar system. "The end product" of these same processes may be carbonaceous chondrites – the most primitive meteorites. This assumption is confirmed by the structure of the asteroid belt, reflectance spectra of asteroids and characteristics of the carbonaceous chondrites.
- Добавил в систему: Бусарев Владимир Васильевич