Datoteka:Kirkwood Gaps.svg

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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
Datum
Izvor http://ssd.jpl.nasa.gov/images/ast_histo.ps
Autor based on plot by Alan Chamberlain, JPL/Caltech
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Licenciranje

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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prikazuje

juna 2007

vrsta medija na Internetu Serbian (Latin script)

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Historija datoteke

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Datum/vrijemeMinijaturaDimenzijeKorisnikKomentar
aktualna6. marta 2023. u 18:58Minijatura verzije (6. marta 2023. u 18:58)792 × 612 (79 kB)AspereFile uploaded using svgtranslate tool (https://svgtranslate.toolforge.org/). Added translation for ko.
13. decembra 2016. u 02:48Minijatura verzije (13. decembra 2016. u 02:48)792 × 612 (58 kB)Rfassbindcolorized MBA division (inner, middle, outer) at 2.5 and 2.82 AU
11. maja 2012. u 17:24Minijatura verzije (11. maja 2012. u 17:24)792 × 612 (60 kB)AutiwaSuppression 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 21:57Minijatura verzije (4. augusta 2009. u 21:57)792 × 612 (112 kB)QuibikFurther optimized.
4. augusta 2009. u 20:34Minijatura verzije (4. augusta 2009. u 20:34)792 × 612 (170 kB)QuibikCombined vertical bars into single path, thus reducing file size. Made SVG-standard compliant.
25. januara 2009. u 02:14Minijatura verzije (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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