LRO development |
LRO development |
May 2 2005, 01:31 AM
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#1
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Senior Member Group: Moderator Posts: 2262 Joined: 9-February 04 From: Melbourne - Oz Member No.: 16 |
Just read this interesting article about LRO
http://science.nasa.gov/headlines/y2005/28apr_lro.htm QUOTE "This is the first in a string of missions," says Gordon Chin, project scientist for LRO at NASA's Goddard Space Flight Center. "More robots will follow, about one per year, leading up to manned flight" no later than 2020." One per Year? Is this just wishful thinking or have any tentitve plans been mentioned for follow up missions after LRO? If the next one is going to be 2009/10 then I guess some desisions about it will have to be made fairly soon. James -------------------- |
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Feb 9 2006, 01:23 PM
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#2
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Solar System Cartographer Group: Members Posts: 10256 Joined: 5-April 05 From: Canada Member No.: 227 |
It might *just* be possible, Bob, but the tracks will not really have much if any albedo difference - Apollo disturbed soil was only darker near the LM, where the descent engine exhaust brightened the surface and any disturbance exposed darker material again (probably a texture difference rather than true albedo). LRV tracks far from the LM were not darker.
Much more useful for the Lunokhods will be the pattern of larger craters along the route. We don't know exactly where Lk1 is, but Soviet maps of the route show the pattern of craters nearby. That will be visible in LRO images if they happen to fall in the right area. Lk2 should be easier to find as we know its location relative to nearby craters fairly well. It will still be barely resolved, though. Phil -------------------- ... because the Solar System ain't gonna map itself.
Also to be found posting similar content on https://mastodon.social/@PhilStooke Maps for download (free PDF: https://upload.wikimedia.org/wikipedia/comm...Cartography.pdf NOTE: everything created by me which I post on UMSF is considered to be in the public domain (NOT CC, public domain) |
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Feb 9 2006, 01:49 PM
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#3
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Senior Member Group: Members Posts: 2454 Joined: 8-July 05 From: NGC 5907 Member No.: 430 |
QUOTE (Phil Stooke @ Feb 9 2006, 08:23 AM) It might *just* be possible, Bob, but the tracks will not really have much if any albedo difference - Apollo disturbed soil was only darker near the LM, where the descent engine exhaust brightened the surface and any disturbance exposed darker material again (probably a texture difference rather than true albedo). LRV tracks far from the LM were not darker. Much more useful for the Lunokhods will be the pattern of larger craters along the route. We don't know exactly where Lk1 is, but Soviet maps of the route show the pattern of craters nearby. That will be visible in LRO images if they happen to fall in the right area. Lk2 should be easier to find as we know its location relative to nearby craters fairly well. It will still be barely resolved, though. Phil Don't they still use the laser reflector on Lunakhod 1, or at least they did. I recall they could not do this with Lunakhod 2 as they were not able to position it properly at the premature end of its mission. Couldn't they just check the records and have literal pinpoint accuracy as to L1's location? http://www.astrosurf.com/lunascan/luna_17.htm -------------------- "After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance. I see that such intercourse long continued would make one thoroughly prosaic, hard, and coarse. But the longest intercourse with Nature, though in her rudest moods, does not thus harden and make coarse. A hard, sensible man whom we liken to a rock is indeed much harder than a rock. From hard, coarse, insensible men with whom I have no sympathy, I go to commune with the rocks, whose hearts are comparatively soft." - Henry David Thoreau, November 15, 1853 |
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