File:Formación de Meteoroides.png
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DescriptionFormación de Meteoroides.png |
Español: FORMACIÓN DE METEOROIDES:
1) El cuerpo primordial pudo haber sido un gran asteroide, por ejemplo de 650 kms de diámetro. No solamente los meteoroides se forman por el impacto entre asteroides o entre sus fragmentos, sino también son partículas o fragmentos cometarios siendo su origen las colas de los cometas formadas por gases y polvo (silicatos), a su vez creadas por sublimación al acercarse el astro al Sol. |
Date | |
Source | Own work based on "The New Solar System". Beatty, Petersen & Chaikin. Cambridge University Press. 4th. Edition. |
Author | Fernando de Gorocica |
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File history
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 12:39, 6 June 2018 | 1,524 × 1,048 (85 KB) | Fernando de Gorocica (talk | contribs) | Nueva imagen que he diseñado para el estudio de la formación de meteoroides. | |
19:40, 30 September 2017 | 1,424 × 1,056 (2.23 MB) | Fernando de Gorocica (talk | contribs) | Infografía más actualizada. | ||
13:16, 30 September 2017 | 427 × 624 (393 KB) | Fernando de Gorocica (talk | contribs) | User created page with UploadWizard |
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