After reading this comment from yesterday's journal:
Luis says:
March 6, 2015 at 5:43 pm
Marc,
Interesting that many of the impact craters on the surface of Ceres show what look like to be central peaks uplift, even in some of the smaller size ones. How important will this type of complex craters be to understand the subsurface characteristics of the dwarf planet, namely its upper crustal composition?
I went back and re-examined each of the frames of
the moving* gif of Ceres rotating. I too see many craters with central peaks.
So, of course, I will now give my opinion of how they were created:
Upon impact, some asteroids will melt the subsurface ice layer, and through some low gravity, extremely cold mechanism, the water freezes before it can flow back.
This also implies that the ice layer is very, very near the surface.
Or something like that.