Spectrophotometric Studies of Near-Earth and Main-Belt Asteroids

Shcherbina, M.P.; Busarev, V.V.; Barabanov, S.I.

Информация о цитировании статьи получена из Web of Science, Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 13 мая 2020 г.

Авторы: Shcherbina M.P., Busarev V.V., Barabanov S.I.
Журнал: Moscow University Physics Bulletin
Том: 74
Номер: 6
Год издания: 2019
Издательство: Allerton Press
Местоположение издательства: New York, N.Y., United States
Первая страница: 675
Последняя страница: 678
DOI: 10.3103/S0027134919060237
Аннотация: The reflectance spectra of five near-Earth asteroids, one Mars crosser, and four classical asteroids of the main belt in the range 0.35–0.95 µm have been observed, calculated, and analyzed. Asteroids with a magnitude up to 17 were observed in 2013–2017 with a 2-m telescope with a CCD spectrograph with extremely low spectral resolution (R ∼ 100) of the Terskol Observatory of the Institute of Astronomy of the Russian Academy of Sciences in order to determine their taxonomic types and composition. These results show that the composition of some of the studied near-Earth asteroids is heterogeneous judging by the variations in their reflectance spectra within adjacent taxonomic classes. It is notable that some of these asteroids are binary. The physical and chemical-mineralogical interpretation of reflectance spectra is presented.
Добавил в систему: Щербина Марина Петровна

	ИСТИНА	Войти в систему Регистрация
	ИСТИНА ИНХС РАН
	Главная Поиск Статистика О проекте Помощь

ИСТИНА

ИСТИНА ИНХС РАН

Spectrophotometric Studies of Near-Earth and Main-Belt Asteroidsстатья

Прикрепленные файлы