Cingulus asteroidum -

Cingulus asteroidum

(Redirectum de Asteroides_Cinguli_Principalis)

Cingulus asteroidum sive zona asteroidum est regio systematis Solaris, quae maximam partem asteroidum continet. Situs est inter Martem et Iovem.


De ortu cinguli, creditissimus cum systema Solare formabatur est. Per processum hoc loco materiam, quam ad planetam sit, numquam adfiebant, quia trahebatur inter Solis Iovisque vires tractionis. Etiam si asteroides simul ponis, non satis magnopere erit ad planetam videri. Alia res credita est, asteroides omnes olim planetam fuisse, sed perditam fuisse certa causa, exempli gratia aliquo formae vehementis belli ut bellum bombae atomicae.

Diffusio asteroidum

Diffusio horum corporum caelestium variat: Maximus numerus est in regione inter 2.06 ua (resonantia orbitalis 4:1 Iove) et 3.27 ua (resonantia 2:1 Iove), quae cingulus asteroidum principalis vel breviter cingulus principalis vocatur.


Circiter 10% asteroidum non inter Martem et Iovem siti sunt.

Haec stipula ad astronomiam spectat. Amplifica , si potes!

Categoriae: Astronomia

Origo: Wikipedia - asteroidum (Auctores [Historia])    Licentia: CC-by-sa-3.0

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