Datoteka:Kirkwood Gaps.svg
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W3C-validity not checked.| OpisKirkwood Gaps.svg | English: This histogram clearly shows the primaryKirkwood gaps in the asteroid main-belt. These gaps (labeled "3:1", "5:2", "7:3", "2:1") are caused bymean-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. |
| Datum | |
| Izvor | http://ssd.jpl.nasa.gov/images/ast_histo.ps |
| Autor | based on plot by Alan Chamberlain, JPL/Caltech |
| Ostale verzije |
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| Public domainPublic domainfalsefalse |
 | This file is in thepublic domain in the United States because it was solely created byNASA. NASA copyright policy states that "NASA material is not protected by copyrightunless noted". (SeeTemplate:PD-USGov,NASA copyright policy page orJPL Image Use Policy.) |  |
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| Datum/vrijeme | Minijatura | Dimenzije | Korisnik | Komentar | |
|---|---|---|---|---|---|
| aktualna | 6. marta 2023. u 18:58 | | 792 × 612(79 kB) | Aspere | File uploaded using svgtranslate tool (https://svgtranslate.toolforge.org/). Added translation for ko. |
| 13. decembra 2016. u 02:48 |  | 792 × 612(58 kB) | Rfassbind | colorized MBA division (inner, middle, outer) at 2.5 and 2.82 AU | |
| 11. maja 2012. u 17:24 |  | 792 × 612(60 kB) | Autiwa | Suppression of one of the two paths (one was used for the line, and the other for the surface). Improving a bit the size of the image. | |
| 4. augusta 2009. u 21:57 |  | 792 × 612(112 kB) | Quibik | Further optimized. | |
| 4. augusta 2009. u 20:34 |  | 792 × 612(170 kB) | Quibik | Combined vertical bars into single path, thus reducing file size. Made SVG-standard compliant. | |
| 25. januara 2009. u 02:14 |  | 792 × 612(544 kB) | Jtratcliff | {{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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