Comet 67P/Churyumov-Gerasimenko is a curious comet. Not just because of its peculiar name, but also because of its odd, rubber-ducky shape. The comet — hereafter referred to as Chury — seems to be made up of two cometary nuclei that gently collided and stuck together at some point in the past.
Astronomers believed that for two comets to merge in such a way, they must possess three traits: They must be extremely low in density, rich in volatiles (elements and compounds with low boiling points), and most importantly, moving very slowly so that they don’t completely pulverize each other upon contact. The problem is that astronomers also know that such sluggish collisions primarily occurred in the infant solar system, some four billion years ago.
So, if a fragile rock the size of Chury (with a radius of roughly a mile) has been roaming a collision-heavy region of the solar system for the past four billion years, how has it survived?
Yesterday, a team of researchers published a
study in
Nature Astronomy showing they finally have an answer to that question: It didn’t.
Instead, the international team used numerical simulations, run at the Mésocentre Sigamm at the Observatoire de la Côte d'Azur, to show that when two comets catastrophically collide (at speeds of up to 2,200 miles per hour), only a small amount of material is actually pulverized and lost into space.