MESSENGER science results |
MESSENGER science results |
Sep 28 2011, 05:14 AM
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#1
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Senior Member Group: Members Posts: 1729 Joined: 3-August 06 From: 43° 35' 53" N 1° 26' 35" E Member No.: 1004 |
to be announced Thursday and to be published in Science Friday.
MESSENGER Reveals New Details of Planet Mercury this looks like a geeky cool Thursday (Thursday evening here in Europe): we have a WISE NEO update at 17 UTC and this MESSENGER teleconf at 18 UTC! |
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Sep 29 2011, 06:32 PM
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#2
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Senior Member Group: Members Posts: 1598 Joined: 14-October 05 From: Vermont Member No.: 530 |
http://messenger.jhuapl.edu/news_room/telecon7_multi.html
http://messenger.jhuapl.edu/news_room/details.php?id=184 The Blewitt images are mind-blewing. |
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Sep 29 2011, 06:52 PM
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#3
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Senior Member Group: Members Posts: 2113 Joined: 13-February 10 From: Ontario Member No.: 5221 |
The view from the surface must be like that as well; if there's ever a landing site candidate someday, that's the place! (Along with the poles).
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Sep 29 2011, 07:46 PM
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#4
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Solar System Cartographer Group: Members Posts: 10256 Joined: 5-April 05 From: Canada Member No.: 227 |
I told you about those pits! - and check out the LRO thread where I highlight similar pits on the Moon. But on the Moon there are VERY few and they are quite old. But they still exist. On Mercury, zillions of them and could still be forming today.
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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Sep 29 2011, 07:52 PM
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#5
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Senior Member Group: Members Posts: 1729 Joined: 3-August 06 From: 43° 35' 53" N 1° 26' 35" E Member No.: 1004 |
for lucky subscribers, Science papers are here
http://www.sciencemag.org/site/feature/dat...pics/messenger/ |
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Sep 29 2011, 09:32 PM
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#6
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Solar System Cartographer Group: Members Posts: 10256 Joined: 5-April 05 From: Canada Member No.: 227 |
A few further thoughts on the pits for clarification. There are two distinct types, the large deep pits such as those I illustrated near a crater in Caloris, with 'false color orange' surroundings (and as shown by Jim Head in the new release), and much smaller shallow 'hollows' making up the bright patches on some crater floors, illustrated by Blewitt in the new release. Both kinds are seen in Tyagaraja crater. The smaller ones are more like the small lunar pits I've been showing in LROC images. The larger ones might be more like the big pyroclastic center south of Orientale on the Moon, surrounded by a dark halo. In both cases, they are found on the Moon, but few and old, and on Mercury where they are plentifull and probably a lot younger.
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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Sep 29 2011, 10:16 PM
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#7
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Member Group: Members Posts: 318 Joined: 1-October 06 Member No.: 1206 |
Wow!
Not only great presentations but a reminder that Messenger truly is a quiet achiever. Many of those depressions have an 'Ina caldera' look about them. Vulcanism on Mercury certainly is more interesting than we might have expected... P |
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Sep 30 2011, 12:21 AM
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#8
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Merciless Robot Group: Admin Posts: 8789 Joined: 8-December 05 From: Los Angeles Member No.: 602 |
Nothing useful to say, but I must add: !!!!!!!!!!!!!!
Absolutely remarkable. -------------------- A few will take this knowledge and use this power of a dream realized as a force for change, an impetus for further discovery to make less ancient dreams real.
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Sep 30 2011, 11:20 AM
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#9
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Newbie Group: Members Posts: 16 Joined: 30-March 08 Member No.: 4078 |
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Sep 30 2011, 12:12 PM
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#10
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Member Group: Members Posts: 813 Joined: 29-December 05 From: NE Oh, USA Member No.: 627 |
A volatile rich Mercury..... just WOW!
Craig |
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Sep 30 2011, 03:54 PM
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#11
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Member Group: Members Posts: 259 Joined: 23-January 05 From: Seattle, WA Member No.: 156 |
Of course, at Mercury's surface temps, what counts as volatile is a bit different than what most of us usually think of as volatile...
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Oct 2 2011, 11:46 PM
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#12
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Junior Member Group: Members Posts: 73 Joined: 14-June 05 From: Cambridge, MA Member No.: 411 |
How does finding all these volatiles on the surface of Mercury square with the "Late Heavy Bombardment" hypothesis? It would seem that, if there was such an event and it included Mercury, these volatiles on its surface would have been destroyed. Is LHB in trouble?
- John Sheff Cambridge, MA |
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Oct 3 2011, 12:22 AM
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#13
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Merciless Robot Group: Admin Posts: 8789 Joined: 8-December 05 From: Los Angeles Member No.: 602 |
Gsnorgathon had an insightful comment about that; check above.
I don't think the LHB is in trouble. One thing to remember about Mercury is that as the innermost planet it probably gets mo' betta impacts than everything else but Jupiter & the Sun over time, and therefore a greater influx rate of elements/minerals. Just my opinion, of course. However, Messenger is definitely proving to be a fascinating mission! -------------------- A few will take this knowledge and use this power of a dream realized as a force for change, an impetus for further discovery to make less ancient dreams real.
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Oct 4 2011, 12:07 AM
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#14
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Member Group: Members Posts: 813 Joined: 29-December 05 From: NE Oh, USA Member No.: 627 |
Thanks Gsnorgathon... Volatiles are relative. My remark earlier should have been qualified. I was not thinking what we Earthlings commonly think of as volatites - H2O, CO2, NH3, etc. I grew up with text books that offered a silicate, iron model of Mercury that left little room for higher temperature volaties such as K and S. The sulfur content is 10 x the Earth. That is significant. Again I say WOW. There will be a joint ESO-DPS MESSENGER breifing Wednesday at 12:15 CSET. Going to try and catch it .... not sure if anything new since last week but what the heck. Wednesday 05 October – Mercury and MESSENGER Mission Briefing Mercury after 6 months of MESSENGER orbital observations (Sean Solomon), Geometry of Mercury's magnetic field and implications for Mercury's dynamo and magnetosphere–surface interactions (Brian Anderson), The dynamics of Mercury's exosphere (Bill McClintock), Mercury's geological and surface compositional evolution (Brett Denevi), Variations in surface reflectance spectra (Noam Izenberg), BepiColombo Current Status (Johannes Benkhoff). Webcast link: http://meetings.copernicus.org/epsc-dps201.../wednesday.html Craig |
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Oct 5 2011, 05:33 PM
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#15
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Senior Member Group: Members Posts: 1598 Joined: 14-October 05 From: Vermont Member No.: 530 |
Presentations and release available here:
http://messenger.jhuapl.edu/news_room/presscon10.html Emily's summary from the conference here: http://planetary.org/blog/article/00003211/ |
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