Help Shape the Future of Space Exploration

Join The Planetary Society Now Join Now!

Join our eNewsletter for updates & action alerts

   Please leave this field empty
Blogs

Headshot of Emily Lakdawalla

A different face of Vesta (oh, *there's* the craters!)

Posted by Emily Lakdawalla

29-07-2011 12:30 CDT

Topics: asteroid 4 Vesta, pretty pictures, asteroids, Dawn

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.

Vesta on July 23, 2011

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.

I like the "snowman" series of craters on the left side. They're so crisp, and if I'm seeing things correctly, they're surrounded by a splat of ejecta that seems to lack the peppering of small craters that you can see elsewhere in this photo -- are the two biggest craters in the "snowman" a relatively fresh, double impact crater? That would be very cool. I also like the huge scarp that lies close to the terminator (the day-night boundary) -- is that part of the south polar basin? I'm not sure. And there's a nice dark splat near the bottom of the image, maybe another fresh crater.

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.

 
See other posts from July 2011

 

Or read more blog entries about: asteroid 4 Vesta, pretty pictures, asteroids, Dawn

Facebook Twitter Email RSS AddThis

Blog Search

JOIN THE
PLANETARY SOCIETY

Our Curiosity Knows No Bounds!

Become a member of The Planetary Society and together we will create the future of space exploration.

Join Us

Featured Images

Hubble's view of Mars during the Comet Siding Spring flyby

Mars from Hubble STIS, April 26, 2012
Hubble's view of Mars on October 19, 2014 (color)
Mars as viewed by Hubble ACS/SBC, May 30, 2014
More Images

Featured Video

View Larger »

Space in Images

Pretty pictures and
awe-inspiring science.

See More

Join the New Millennium Committee

Let’s invent the future together!

Become a Member

Connect With Us

Facebook! Twitter! Google+ and more…
Continue the conversation with our online community!