Impact simulation explaining the origin of Hygiea’s round shape

Computational simulation of the fragmentation and reassembly that led to the formation of Hygiea and its family of asteroids, following an impact with a large object. While changes in the shape of Hygiea occur after the impact, the dwarf-planet candidate eventually acquires a round shape.

Autorska prava:

P. Ševeček/Charles University

O video klipu

Datum objavljivanja:28. oktobar 2019. 17:00
Povezana saopštenja:eso1918
Trajanje:34 s
Frame rate:25 fps

O objektu

Tip:Solar System : Interplanetary Body : Dwarf planet
Kategorija:Solar System

Ultra HD (info)



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