Where are all of Ceres ’ with child impingement craters ? That was a question that stump scientist when the Dawn spacecraft arrived in orbit in March 2015 . Now , we may be stuffy to an result thanks to a squad of Dawn scientists .
Ceres is far-famed for get no tumid craters make by impacts on its surface . Its largest , the Kerwan Basin , is a “ measly ” 285 kilometers ( 177 miles ) in diameter . In fact , model suggest it should have 40 Crater larger than 100 kilometers ( 60 statute mile ) wide , and 10 to 15 larger than 400 kilometers ( 250 miles ) . But it has just 16 of the former , and none of the latter .
On other standardized humankind , like protoplanet Vesta , also in the asteroid belt , we see plenty of grounds for large impact . Ceres , being locate in the asteroid belt and having formed 4.55 billion geezerhood ago , should sure enough have them too .

But the reason why it does n’t may be due to one of the key differences between Vesta and Ceres . Whereas the former is mostly rocky , Ceres seems to control large amounts of methamphetamine . And it is this shabu that may be fundamental to its less pummeled appearing .
Publishing their finding inNature Communications , the team suggest that if the encrustation of Ceres contains a pregnant amount of ice and salts , it could be weak enough that large Crater may smooth out over meter , or even disappear . This could be aggravate by inner heat from Ceres , driven by the radioactive disintegration of elements – similar to what we remember is happening on Pluto .
The Vendimia Planitia depression may be the remnant of an ancient large impact . Southwest Research Institute / Simone Marchi
“ If Ceres were highly rocky , we ’d expect wallop volcanic crater of all sizes to be preserved , ” sound out David Williams from Arizona State University , a member of the Dawn team behind this study , in astatement . “ Remote detection from Earth , however , told us even before Dawn arrive that the crust of Ceres obtain a important fraction of methamphetamine hydrochloride in some word form . ”
Evidence for this activity is defend by the comportment of the famous burnished spots on the surface , which are thought to be salts left on the control surface , but may be linked to cryovolcanism .
It would seem probable , then , that Ceres did have big impact in the past tense – but the dwarf planet has enshroud them from our view . Indeed , we can sort of see the remnants of such impacts , declamatory low up to 800 kilometers ( 500 mi ) wide .