Fil:Kirkwood Gaps.svg

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SkildringKirkwood Gaps.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. inner main-belt (a < 2.5 AU) middle main-belt (2.5 AU < a > 2.82 AU) outer main-belt (a > 2.82 AU
Dato	juni 2007
Kjelde	http://ssd.jpl.nasa.gov/images/ast_histo.ps
Opphavsperson	based on plot by Alan Chamberlain, JPL/Caltech
Andre versjonar	español македонски polski

	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.)
	Warnings: Use of NASA logos, insignia and emblems is restricted per U.S. law 14 CFR 1221. The NASA website hosts a large number of images from the Soviet/Russian space agency, and other non-American space agencies. These are not necessarily in the public domain. Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI.[1] See also {{PD-Hubble}} and {{Cc-Hubble}}. The SOHO (ESA & NASA) joint project implies that all materials created by its probe are copyrighted and require permission for commercial non-educational use. [2] Images featured on the Astronomy Picture of the Day (APOD) web site may be copyrighted. [3] The National Space Science Data Center (NSSDC) site has been known to host copyrighted content. Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain "Unless otherwise noted."

Klikk på dato/klokkeslett for å sjå fila slik ho var på det tidspunktet.

	Dato/klokkeslett	Oppløysing	Brukar	Kommentar
gjeldande	6. mars 2023 kl. 19:58	792 × 612 (79 KB)	Aspere	File uploaded using svgtranslate tool (https://svgtranslate.toolforge.org/). Added translation for ko.
	13. desember 2016 kl. 03:48	792 × 612 (58 KB)	Rfassbind	colorized MBA division (inner, middle, outer) at 2.5 and 2.82 AU
	11. mai 2012 kl. 18:24	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. august 2009 kl. 22:57	792 × 612 (112 KB)	Quibik	Further optimized.
	4. august 2009 kl. 21:34	792 × 612 (170 KB)	Quibik	Combined vertical bars into single path, thus reducing file size. Made SVG-standard compliant.
	25. januar 2009 kl. 03:14	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