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Io (moon)
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1ER8VNIMRGH
Geliefert zwischen Mi., 26.11.2025 und Do., 27.11.2025
Details
Io is the innermost of the four Galilean moons of the planet Jupiter and, with a diameter of 3,642 kilometres, the fourth-largest moon in the Solar System. It was named after Io, a priestess of Hera who became one of the lovers of Zeus. With over 400 active volcanoes, Io is the most geologically active object in the Solar System. This extreme geologic activity is the result of tidal heating from friction generated within Io's interior by Jupiter's varying pull. Several volcanoes produce plumes of sulfur and sulfur dioxide that climb as high as 500 km (310 mi). Io's surface is also dotted with more than 100 mountains that have been uplifted by extensive compression at the base of the moon's silicate crust. Some of these peaks are taller than Earth's Mount Everest. Unlike most satellites in the outer Solar System (which have a thick coating of ice), Io is primarily composed of silicate rock surrounding a molten iron or iron sulfide core. Most of Io's surface is characterized by extensive plains coated with sulfur and sulfur dioxide frost. Io's volcanism is responsible for many of that satellite's unique features.
Weitere Informationen
- Allgemeine Informationen
- GTIN 09786130271589
- Editor Frederic P. Miller, Agnes F. Vandome, John McBrewster
- Sprache Englisch
- Genre Physik & Astronomie
- Größe H220mm x B150mm x T17mm
- Jahr 2009
- EAN 9786130271589
- Format Fachbuch
- ISBN 978-613-0-27158-9
- Titel Io (moon)
- Untertitel Galilean moons, Moons of Jupiter, Diameter, Kilometre, List of natural satellites, Zeus, Solar System, Volcano, Jupiter, Sulfur, Mount Everest, Magnetosphere of Jupiter, Galileo Galilei
- Gewicht 439g
- Herausgeber Alphascript Publishing
- Anzahl Seiten 284
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