See other posts from July 2011
A different face of Vesta (oh, *there's* the craters!)
Posted By Emily Lakdawalla
2011/07/29 12:30 CDT
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Here's the latest image release from Dawn at Vesta, taken from an altitude about twice as high as that of their first mapping orbit. This is the first view that they've shown us that hasn't contained the enormous central-peaked crater that dominates the south pole of the asteroid belt's second largest resident. I'm not exactly sure where on Vesta we are, but it's different; there are a lot more small craters here than you can see near the south polar basin.

NASA / JPL-Caltech / UCLA / MPS / DLR / IDA
Vesta on July 23, 2011
Dawn took this photo on July 23, 2011 from a distance of 5,200 kilometers.But most places in this image I see lots and lots of small craters, at a density I don't think I saw in the earlier photos (though you have to be careful when making that comparison, because the earlier photos have inherently lower resolution so you wouldn't see as many smaller craters as are visible in this latest photo). Why do I care about how many little craters there are? Because the density of craters is used as a proxy for the age of surfaces in the solar system. An older surface, exposed to space for longer, will have more craters. Different crater densities across Vesta would mean that different bits of it have different ages, so Vesta has been a place that has changed geologically with time.
There's a press briefing Monday. Since it's been scheduled for a relatively early 9:00 a.m. I won't be able to get to JPL to cover it in time, but I'll be watching from home and hopefully will get to call in with some questions! As usual for JPL press briefings, you can watch live and chat on Ustream.
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