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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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149:, Chile. These strikingly-detailed views reveal four of the millions of rocky bodies in the main asteroid belt, a ring of asteroids between Mars and Jupiter that separates the rocky inner planets of the Solar System from the gaseous and icy outer planets.
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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270:"Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts and captions, are licensed under a
341:– You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
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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.
172:— so hefty that it was once classified as a planet. A third of the size of 2 Pallas, 89 Julia is thought to be named after St Julia of Corsica. Its stony composition led to its classification as an
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176:. Another S-type asteroid is 29 Amphitrite, which was only discovered in 1854. 324 Bamberga, one of the largest
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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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Creative
Commons Attribution 4.0 International License
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Clockwise from top left, the asteroids shown here are
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Spectro-Polarimetric High-Contrast
Exoplanet Research
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Commons is a freely licensed media file repository.
697:Список об'єктів Сонячної системи за розміром
180:in the asteroid belt, was discovered even later:
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56:(152 × 149 pixels, file size: 9 KB, MIME type:
657:Список на тела во Сончевиот Систем по големина
488:Creative Commons Attribution 4.0 International
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348:https://creativecommons.org/licenses/by/4.0
324:– to copy, distribute and transmit the work
223:http://www.eso.org/public/images/potw1749a/
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617:Anexo:Objetos del sistema solar por tamaño
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137:These images were taken by ESO's SPHERE (
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257:This media was created by the
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395:Items portrayed in this file
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232:Credit: ESO/Vernazza et al.
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92:You can help
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22:File history
554:Kwamikagami
452:copyrighted
339:attribution
114:Description
607:(89) Julia
565:File usage
546:152 × 149
522:Dimensions
351:CC BY 4.0
27:File usage
739:28.35 dpc
731:28.35 dpc
677:(89) Юлия
519:Thumbnail
516:Date/Time
240:Licensing
198:10 Hygiea
123:English:
58:image/png
715:Metadata
707:89 Julia
687:89 Julia
647:89 Julia
627:89 Julia
574:89 Julia
416:89 Julia
376:Captions
328:to remix
322:to share
313:license.
166:89 Julia
162:2 Pallas
37:Metadata
533:current
528:Comment
400:depicts
380:English
194:4 Vesta
145:at the
106:Summary
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548:(9 KB)
229:Author
214:Source
164:, and
190:Ceres
525:User
360:true
357:true
206:Date
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268::
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Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
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