Английская Википедия:Carme (moon)
Шаблон:Short description Шаблон:Use dmy dates Шаблон:Infobox planet
Carme Шаблон:IPAc-en is a retrograde irregular satellite of Jupiter. It was discovered by Seth Barnes Nicholson at Mount Wilson Observatory in California in July 1938.[1] It is named after the mythological Carme, mother by Zeus of Britomartis, a Cretan goddess.
History
Carme did not receive its present name until 1975;[2] before then, it was simply known as Шаблон:Nowrap. It was sometimes called "Pan"[3] between 1955 and 1975 (Pan is now the name of a satellite of Saturn).
It gives its name to the Carme group, made up of irregular retrograde moons orbiting Jupiter at a distance ranging between 23 and 24 Gm and at an inclination of about 165°. Its orbital elements are as of January 2000.[4] They are continuously changing due to solar and planetary perturbations.
Properties
With a diameter of Шаблон:Val, it is the largest member of the Carme group and the fourth largest irregular moon of Jupiter.[5] It is light red in color (B−V=0.76, V−R=0.47), similar to D-type asteroids and consistent with Taygete, but not Kalyke.[6]
See also
References
External links
- Carme Profile by NASA's Solar System Exploration
- David Jewitt pages
- Jupiter's Known Satellites (by Scott S. Sheppard)
- ↑ Ошибка цитирования Неверный тег
<ref>; для сносокNicholson1938не указан текст - ↑ IAUC 2846: Satellites of Jupiter 1974 October 7 (naming the moon)
- ↑ Шаблон:Cite book
- ↑ Ошибка цитирования Неверный тег
<ref>; для сносокJacobson2000не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>; для сносокGrav2015не указан текст - ↑ Шаблон:Cite journal
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