File:Kirkwood Gaps.svg

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Summary

Description
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.
 
inner main-belt (a < 2.5 AU)
 
middle main-belt (2.5 AU < a > 2.82 AU)
 
outer main-belt (a > 2.82 AU
Date
Source http://ssd.jpl.nasa.gov/images/ast_histo.ps
Author based on plot by Alan Chamberlain, JPL/Caltech
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Licensing

Public domain 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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June 2007

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current19:58, 6 March 2023Thumbnail for version as of 19:58, 6 March 2023792 × 612 (79 KB)wikimediacommons>AspereFile uploaded using svgtranslate tool (https://svgtranslate.toolforge.org/). Added translation for ko.

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