File:Kirkwood Gaps.svg

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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[edit]

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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Date/TimeThumbnailDimensionsUserComment
current17:58, 6 March 2023Thumbnail for version as of 17:58, 6 March 2023792 × 612 (79 KB)Aspere (talk | contribs)File uploaded using svgtranslate tool (https://svgtranslate.toolforge.org/). Added translation for ko.
01:48, 13 December 2016Thumbnail for version as of 01:48, 13 December 2016792 × 612 (58 KB)Rfassbind (talk | contribs)colorized MBA division (inner, middle, outer) at 2.5 and 2.82 AU
16:24, 11 May 2012Thumbnail for version as of 16:24, 11 May 2012792 × 612 (60 KB)Autiwa (talk | contribs)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.
20:57, 4 August 2009Thumbnail for version as of 20:57, 4 August 2009792 × 612 (112 KB)Quibik (talk | contribs)Further optimized.
19:34, 4 August 2009Thumbnail for version as of 19:34, 4 August 2009792 × 612 (170 KB)Quibik (talk | contribs)Combined vertical bars into single path, thus reducing file size. Made SVG-standard compliant.
01:14, 25 January 2009Thumbnail for version as of 01:14, 25 January 2009792 × 612 (544 KB)Jtratcliff (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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