MSL Landing Sites |
MSL Landing Sites |
Sep 22 2006, 06:33 AM
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#1
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Newbie Group: Members Posts: 17 Joined: 11-March 04 Member No.: 55 |
I thought you guys might be interested in seeing some results from a campaign we've been running to get mosaics of all the proposed MSL landing sites. We've currently got 22 of the potential landing sites made in day/night and vis, and many with thermal inertia. Here's 4 examples with links to the full pages. You can see the rest of them at http://themis.asu.edu/landingsites
Nili Fossae Trough Holden Crater Fan Terby Crater Marwth Vallis |
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Sep 22 2006, 03:37 PM
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#2
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Junior Member Group: Members Posts: 50 Joined: 7-July 06 From: Selden, NY Member No.: 960 |
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Guest_AlexBlackwell_* |
Sep 22 2006, 06:33 PM
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#3
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Guests |
I thought you guys might be interested in seeing some results from a campaign we've been running to get mosaics of all the proposed MSL landing sites. We've currently got 22 of the potential landing sites made in day/night and vis, and many with thermal inertia. Here's 4 examples with links to the full pages. You can see the rest of them at http://themis.asu.edu/landingsites Thanks for the reminder, Noel. Tim had also tipped us to this a short while back. |
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Dec 1 2006, 04:16 PM
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#4
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Member Group: Members Posts: 548 Joined: 19-March 05 From: Princeton, NJ, USA Member No.: 212 |
Excellent.
perhaps you can update with MRO images as they become available ken |
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Guest_Sunspot_* |
Dec 10 2006, 11:49 AM
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#5
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Guests |
Holden Crater might turn out like Gusev Crater.
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Dec 10 2006, 11:59 AM
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#6
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Founder Group: Chairman Posts: 14434 Joined: 8-February 04 Member No.: 1 |
Holden Crater might turn out like Gusev Crater. I don't think so http://hiroc.lpl.arizona.edu/images/TRA/TRA_000861_1530/ Doug |
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Feb 15 2007, 05:33 PM
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#7
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Junior Member Group: Members Posts: 50 Joined: 7-July 06 From: Selden, NY Member No.: 960 |
Some new data are available on the THEMIS MSL landing site selection website: http://themis.asu.edu/landingsites
The new data consist of THEMIS IR decorrelation stretch mosaics of the landing sites, which are intended to show the some of the compositional variability detectable by THEMIS. |
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