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[[Fasciculus:InnerSolarSystem-la.png|thumb|200px|Systema solare interius]]
'''Cingulus asteroidum''' sive '''zona asteroidum''' est [[regio]] [[torus|toriformis]] in [[Systema Solare|systemate Solari]], plerumque inter [[planeta]]s [[Mars (planeta)|Martem]] et [[Iuppiter (planeta)|Iovem]] sita, quae permulta [[corpus caeleste|corpora]] solida et deformia multarum [[magnitudo|magnitudinum]], sed planetis minores, [[asteroides]] vel [[planeta minor|planetas minores]] appellatas, continet. Hic asteroidum cingulus etiam '''principalis asteroidum cingulus''' et '''praecipuus cingulus''' appellatur ad eum ab aliis asteroidibus in Systemate Solari, sicut [[asteroides prope Tellurem|asteroidibus prope Tellurem]] et [[asteroides troianis]] distinguendum.<ref name = Williams>{{cite news |url=http://www.universetoday.com/32856/asteroid-belt/ |title=What is the Asteroid Belt? |author=Matt Williams |work=Universe Today |date=23 Augusti [[2015]] |access-date=30 Ianuarii 2016}}.</ref>
== Origo ==
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Circiter 10% asteroidum non inter [[Mars (planeta)|Martem]] et [[Iuppiter (planeta)|Iovem]] siti sunt.
==Bibliographia==
* Elkins-Tanton, Linda T. [[2006]]. ''Asteroids, Meteorites, and Comets.'' Novi Eboraci: Chelsea House. ISBN 978-0-8160-5195-3.
{{astro-stipula}}
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