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Although the asteroid belt is often portrayed in science fiction as a place of violent collisions, packed full of large rocks too dangerous for even the most skilled of space pilots to navigate, it is actually very sparse. In total, the asteroid belt contains just 4% of the mass of the Moon, with
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168:. Named after the Greek goddess Pallas Athena, 2 Pallas is about 510 kilometres wide. This makes it the third largest asteroid in the main belt and one of the biggest asteroids in the entire Solar System. It contains about 7% of the mass of the entire
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found it in 1892. Today, it is understood that C-type asteroids may actually be bodies from the outer Solar System following the migration of the giant planets. As such, they may contain ice in their interior.
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If the file has been modified from its original state, some details may not fully reflect the modified file.
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about half of this mass contained in the four largest residents:
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Lista obiektów w Układzie Słonecznym ze względu na masę
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Clockwise from top left, the asteroids shown here are
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782:Список об'єктів Сонячної системи за розміром
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324:– to copy, distribute and transmit the work
223:http://www.eso.org/public/images/potw1749a/
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589:List of exceptional asteroids
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787:Список найбільших астероїдів
772:İstisnai asteroitler listesi
717:Lista de asteroides notáveis
395:Items portrayed in this file
383:ESO image of (324) Bamberga
232:Credit: ESO/Vernazza et al.
116:Potw1749a Bamberga crop.png
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672:バンベルガ (小惑星)
594:User:Fotaun
554:Kwamikagami
452:copyrighted
339:attribution
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546:198 × 185
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351:CC BY 4.0
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819:28.35 dpc
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240:Licensing
198:10 Hygiea
123:English:
58:image/png
795:Metadata
376:Captions
328:to remix
322:to share
313:license.
166:89 Julia
162:2 Pallas
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