File:Huecos de Kirkwood.svg
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Size of this PNG preview of this SVG file: 776 × 600 pixels. Other resolutions: 311 × 240 pixels | 621 × 480 pixels | 994 × 768 pixels | 1,280 × 989 pixels | 2,560 × 1,978 pixels | 792 × 612 pixels.
Original file (SVG file, nominally 792 × 612 pixels, file size: 122 KB)
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DescriptionHuecos de Kirkwood.svg |
English: This histogram clearly shows the primary Kirkwood gaps in the asteroid main-belt. These gaps (labeled "3:1", "5:2", "7:3", "2:1") are caused by mean-motion resonances between an asteroid and Jupiter. For example, the 3:1 Kirkwood gap is located where the ratio of an asteroid's orbital period to that of Jupiter is 3/1 (the asteroid completes 3 orbits for every 1 orbit of Jupiter). The effect of these mean-motion resonances is a change in the asteroid's orbital elements (particularly semimajor axis) sufficient to create these gaps in semimajor axis space. |
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This is a retouched picture, which means that it has been digitally altered from its original version. Modifications: Traducida al castellano. The original can be viewed here: Kirkwood Gaps.svg: . Modifications made by Karshan.
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Public domainPublic domainfalsefalse |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ||
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Original upload log[edit]
This image is a derivative work of the following images:
- File:Kirkwood_Gaps.svg licensed with PD-USGov-NASA
- 2009-08-04T20:57:44Z Quibik 792x612 (114442 Bytes) Further optimized.
- 2009-08-04T19:34:47Z Quibik 792x612 (173601 Bytes) Combined vertical bars into single path, thus reducing file size. Made SVG-standard compliant.
- 2009-01-25T01:14:06Z Jtratcliff 792x612 (556736 Bytes) {{Information |Description={{en|1=This histogram clearly shows the primary Kirkwood gaps in the asteroid main-belt. These gaps (labeled "3:1", "5:2", "7:3", "2:1") are caused by mean-motion resonances between an asteroid and
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 14:15, 12 December 2009 | 792 × 612 (122 KB) | Karshan (talk | contribs) | Mejorado. | |
12:27, 12 December 2009 | 792 × 612 (119 KB) | Karshan (talk | contribs) | {{Information |Description={{en|1=This histogram clearly shows the primary Kirkwood gaps in the asteroid main-belt. These gaps (labeled "3:1", "5:2", "7:3", "2:1") are caused by mean-motion resonances between an asteroid and Jupiter. For example, the 3:1 |
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