Home Page - YouTube Channel



Metis (moon) - Simple English Wikipedia, the free encyclopedia

Metis (moon)

From the Simple English Wikipedia, the free encyclopedia that anyone can change

Metis
Image:metis2.gif
Image of Metis was taken by Galileo's solid state imaging system between November 1996 and June 1997.
Discovery
Discovered by: S. Synnott
Discovery date: March 4, 1979
Orbital characteristics
Periapsis: 127,974 km
Apoapsis 128,026 km
Mean radius of orbit: 128,000 km (1.792 RJ)
Eccentricity: 0.0002
Orbital period: 0.294780 d (7 h 4.5 min)
Avg. orbital speed: 31.501 km/s
Inclination: 0.06° (to Jupiter's equator)
Satellite of: Jupiter
Physical characteristics
Mean radius: 21.5 ± 2.0 km
Volume: ~42,700 km³
Mass: 3.6 ×1016 kg
Mean density: 0.86 g/cm³ (assumed)
Equatorial surface gravity: 0.005 m/s² (0.0005 g)
Escape velocity: 0.012 km/s
Rotation period: synchronous
Axial tilt: zero
Albedo: 0.061 ± 0.003
Temperature: ~123 K

Metis or Jupiter XVI, is Jupiter's closest moon.

Metis was found in 1979 by Stephen P. Synnott in images taken by the Voyager 1 probe. Its designation was S/1979 J 3. In 1983 it was named after the mythological Metis, a Titaness who was the first wife of Zeus (the Greek equivalent of Jupiter).

Metis not a sphere and measures 60×40×34 km across. The composition and mass of Metis are not known, but assuming that its mean density is like that of Amalthea (~0.86 g/cm³), its mass can be estimated as ~7×1016 kg. Amalthea's density implies that that moon is composed of water ice with a porosity of 10-15%, and Adrastea may be similar.

The surface of Metis is very cratered. It is dark and appears to be reddish in color.

[change] Orbit

Metis is the closest moon to Jupiter. It orbits Jupiter at a distance of ~128,000 km. Its orbit has very small eccentricity (~0.0002) and inclination (~ 0.06°) relative to the equator of Jupiter.

[change] Exploration

The images taken by Voyager 1 showed Metis only as a dot, and very little was know about Metis until the arrival of the Galileo spacecraft. Galileo took pictures of almost all of the surface of Metis and put constraints on its composition.


[change] Other websites


Wikipedia HTML 2008 in other languages

100 000 +

Česká (Czech)  •  English  •  Deutsch (German)  •  日本語 (Japanese)  •  Français (French)  •  Polski (Polish)  •  Suomi (Finnish)  •  Svenska (Swedish)  •  Nederlands (Dutch)  •  Español (Spanish)  •  Italiano (Italian)  •  Norsk (Norwegian Bokmål)  •  Português (Portuguese)  •  Română (Romanian)  •  Русский (Russian)  •  Türkçe (Turkish)  •  Українська (Ukrainian)  •  中文 (Chinese)

10 000 +

العربية (Arabic)  •  Български (Bulgarian)  •  Bosanski (Bosnian)  •  Català (Catalan)  •  Cymraeg (Welsh)  •  Dansk (Danish)  •  Ελληνικά (Greek)  •  Esperanto  •  Eesti (Estonian)  •  Euskara (Basque)  •  Galego (Galician)  •  עברית (Hebrew)  •  हिन्दी (Hindi)  •  Hrvatski (Croatian)  •  Magyar (Hungarian)  •  Ido  •  Bahasa Indonesia (Indonesian)  •  Íslenska (Icelandic)  •  Basa Jawa (Javanese)  •  한국어 (Korean)  •  Latina (Latin)  •  Lëtzebuergesch (Luxembourgish)  •  Lietuvių (Lithuanian)  •  Latviešu (Latvian)  •  Bahasa Melayu (Malay)  •  Plattdüütsch (Low Saxon)  •  Norsk (Norwegian Nynorsk)  •  فارسی (Persian)  •  Sicilianu (Sicilian)  •  Slovenčina (Slovak)  •  Slovenščina (Slovenian)  •  Српски (Serbian)  •  Basa Sunda (Sundanese)  •  தமிழ் (Tamil)  •  ไทย (Thai)  •  Tiếng Việt (Vietnamese)

1 000 +

Afrikaans  •  Asturianu (Asturian)  •  Беларуская (Belarusian)  •  Kaszëbsczi (Kashubian)  •  Frysk (Western Frisian)  •  Gaeilge (Irish)  •  Interlingua  •  Kurdî (Kurdish)  •  Kernewek (Cornish)  •  Māori  •  Bân-lâm-gú (Southern Min)  •  Occitan  •  संस्कृत (Sanskrit)  •  Scots  •  Tatarça (Tatar)  •  اردو (Urdu) Walon (Walloon)  •  יידיש (Yiddish)  •  古文/文言文 (Classical Chinese)

100 +

Nehiyaw (Cree)  •  словѣньскъ (Old Church Slavonic)  •  gutisk (Gothic)  •  ລາວ (Laos)