Haumea (Dwarf Planet)
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High Quality Content by WIKIPEDIA articles! Haumea, formal designation (136108) Haumea, is a dwarf planet in the Kuiper belt. Its mass is one-third the mass of Pluto. It was discovered in 2004 by a team headed by Mike Brown of Caltech at the Palomar Observatory in the United States and, in 2005, by a team headed by J. L. Ortiz at the Sierra Nevada Observatory in Spain, though the latter claim has been contested. On September 17, 2008, it was designated a dwarf planet by the International Astronomical Union (IAU) and named after Haumea, the Hawaiian goddess of childbirth. Haumea's extreme elongation makes it unique among known trans-Neptunian objects (TNOs). Although its shape has not been directly observed, calculations from its light curve suggest it is an ellipsoid, with its greatest axis twice as long as its shortest. Nonetheless, its gravity is believed sufficient for it to have relaxed into hydrostatic equilibrium, thereby meeting the definition of a dwarf planet.
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GarantieWeitere Informationen
- Allgemeine Informationen
- GTIN 09786130252083
- Editor Frederic P. Miller, Agnes F. Vandome, John McBrewster
- Sprache Englisch
- Genre Physik & Astronomie
- Größe H220mm x B150mm x T7mm
- Jahr 2009
- EAN 9786130252083
- Format Fachbuch
- ISBN 978-613-0-25208-3
- Titel Haumea (Dwarf Planet)
- Untertitel Controversy over the discovery of Haumea, Moons of Haumea, Haumea family, Minor planet designation, Dwarf planet, Kuiper belt, Michael E. Brown, Palomar Observatory, International Astronomical Union
- Gewicht 195g
- Herausgeber Alphascript Publishing
- Anzahl Seiten 120
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