Post Block Island Meteor Studies (The Western Route), The 6th Leg in our Zig Zag Journey to Endeavour Crater |
Post Block Island Meteor Studies (The Western Route), The 6th Leg in our Zig Zag Journey to Endeavour Crater |
Nov 15 2009, 05:41 PM
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#706
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Member Group: Members Posts: 233 Joined: 21-April 05 Member No.: 328 |
Tesheiner and Centsworth_II, thanks for the enhancements of the latest MI work -- and my God, what an incredible sight it is! It brings to mind so many things I don't even now where to start, so I will just throw out a couple of breathless thoughts.
First -- and I am not sure if it is even permissible to allude to this...... ADMIN ..... so why post it? Please don't intentionally and knowingly add to the administrative workload. |
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Nov 15 2009, 05:50 PM
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#707
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Senior Member Group: Members Posts: 2173 Joined: 28-December 04 From: Florida, USA Member No.: 132 |
...Centsworth_II, thanks... Just to be clear, I posted the work of talented image worker Hortonheardawho.
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Nov 15 2009, 05:58 PM
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#708
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Senior Member Group: Members Posts: 2173 Joined: 28-December 04 From: Florida, USA Member No.: 132 |
First -- and I am not sure if it is even permissible to allude to this...... You should have just said, "it's like being there..." ADMIN ..... so why post it? Please don't intentionally and knowingly add to the administrative workload. I think you actually said its better than being there, but I don't think you'd get a lot of agreement on that. |
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Nov 16 2009, 03:58 AM
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#709
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Senior Member Group: Members Posts: 2228 Joined: 1-December 04 From: Marble Falls, Texas, USA Member No.: 116 |
Yesterday, a full set of right-filter images of Marquette came down. I made a right-filter, false color composite to see if this rock mineralogically resembled typical Meridiani sediments. This is the same false color image from right filter ratios that we've seen used in the past to emphasize the hematite concretions in these rocks. These RGB composites use R=R1/R2, G=R1, and B=R5/R7. An example from early in the mission is available here.
I won't speculate as to the mineralogy of Marquette, but it has a very different color and appearance in this image compared to typical Meridiani sediments. Remember, this is made from raw imagery which can only be used qualitatively. You can compare its yellow color to the blue color of the bedrock beneath it. The purplish hues are artifacts of the shadows. This image also shows that most of the cobbles lying around here display the same colors as Marquette, and therefore are probably fragments of the same original body. -------------------- ...Tom
I'm not a Space Fan, I'm a Space Exploration Enthusiast. |
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Nov 16 2009, 11:00 AM
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#710
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Senior Member Group: Moderator Posts: 4279 Joined: 19-April 05 From: .br at .es Member No.: 253 |
From today's batch of pancams: http://nasa.exploratorium.edu/mars/opportu...cam/2009-11-16/
Wilderness, Voight, and Hessel Bays. |
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Nov 16 2009, 11:05 AM
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#711
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Member Group: Members Posts: 155 Joined: 8-February 04 From: Phoenix, AZ USA Member No.: 9 |
The texture and fabric of Marquette in the MI's looks like a micro-vesicular extrusive igneous rock, with some vesicles filled with lighter-colored minerals. That may include a pre-impact origin as a lava flow (basalt), dome (intermediate/andesite), or pre-existing impact melt. Like me in Texas, it ain't from around here...
-------------------- Tim Demko
BioLink site |
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Nov 16 2009, 03:22 PM
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#712
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Member Group: Members Posts: 237 Joined: 22-December 07 From: Alice Springs, N.T. Australia Member No.: 3989 |
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Nov 16 2009, 05:54 PM
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#713
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Senior Member Group: Members Posts: 3008 Joined: 30-October 04 Member No.: 105 |
QUOTE (tim) The texture and fabric of Marquette in the MI's looks like... My first impression, too. Looks like a piece of basaltic "basement" ejecta. Easy to spot with the R721 images. From the looks, this rock has had an interesting history. There should be some more MI handlens images today.--Bill -------------------- |
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Nov 16 2009, 08:18 PM
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#714
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Senior Member Group: Moderator Posts: 2262 Joined: 9-February 04 From: Melbourne - Oz Member No.: 16 |
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Nov 17 2009, 08:30 AM
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#715
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Senior Member Group: Moderator Posts: 4279 Joined: 19-April 05 From: .br at .es Member No.: 253 |
With all the activity and expectations (knock on wood!) on Spirit today, the information about her sister at the other side of the planet was left a little bit behind. Just checked the tracking web to know about the imaging plan and found that the RAT will be used tomorrow, sol 2068.
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Guest_PhilCo126_* |
Nov 17 2009, 05:04 PM
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#716
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Guests |
Did NASA-JPL give an estimate of the size of "Mackinac" meteorite ?
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Nov 18 2009, 03:13 PM
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#717
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Senior Member Group: Moderator Posts: 4279 Joined: 19-April 05 From: .br at .es Member No.: 253 |
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Nov 18 2009, 03:35 PM
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#718
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Founder Group: Chairman Posts: 14434 Joined: 8-February 04 Member No.: 1 |
That's a good pre-grind position. Time for some rock-chomping, not done any for a while
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Nov 18 2009, 04:40 PM
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#719
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Senior Member Group: Members Posts: 2922 Joined: 14-February 06 From: Very close to the Pyrénées Mountains (France) Member No.: 682 |
Interesting! We kind of debated the value of grinding and gave a No Go. Is JPL still reading us?
OK, they'll may be "only" brush; but I wonder whether they choose to "attack" Marquette because of very big interest or because they consider "interesting enough" to use the tools since it's supposed to work (I know, we had a fault last time) instead of saving it for Endeavour with no garenty to get to there. This is the same debate as whether or not trying to move Marquette considered a few days ago by Deimos with very interesting rationales. -------------------- |
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Nov 18 2009, 05:43 PM
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#720
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Founder Group: Chairman Posts: 14434 Joined: 8-February 04 Member No.: 1 |
I'd have gone for it because we need down time for the FR wheel - it's presenting itself very well for IDD work given the limitations of the IDD since its trouble - and it's fairly unique, perhaps deep ejecta from a nearby crater.
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