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You could use QuickTime or QuickTime Alternative.
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http://www.spaceref.com/news/viewpr.html?pid=18095 This article is what Jerry was referring to, the heat inertia is low, meaning the heat from the Sun is gone when the comet surface turns into shadow. If this comet's heat inertia is anywhere near comet Wild 2's heat inertia it totally invalidates any model of jet production based on solar heating. On Wild 2 specifically, jets were emitting from the dark side and if we get any news on the jets from Tempel 1 I suspect it will confirm this impossibility. To show what I mean: this website shows results from all the telescopes that imaged the impact. http://deepimpact.umd.edu/collab_pub/imagep.shtml Click on "Images" and look at the result from the NOT telescope in Spain: Image caption: Quote:
Cheers. |
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Just a Deep Impact update:
NASA - Mission Update - November 2005 Quote:
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Thanks for the link,
I'll try to find what I'm looking for (what causes cometary jets, and what are the bright spots/patches seen in close-ups of comets), but I'm not very hopeful. Cheers. Last edited by VanderL; 04-December-2005 at 02:38 PM. |
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I asked the DI team directly about the origin of the jets and bright spots, several times, but didn't even get an acknowledgement that the question was received. Cheers. |
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There is no question they are downplaying the surprises. These include:
1) virtually all of the ejecta was dust with very little water vapor. 2) The dust is fairly high in iron content. (Remember, comets are thought to consist of only primal material found at the edges of the solar system when it formed. Most of the iron should be in the inner solar system.) 3) The minerals found take significant temperatures ~400+K to form. Again, this was not expected. While it is true many in the field had been leaning towards an "Icy dirt ball" rather than a "dirty ice ball". the results contraindicate long-standing solar models. If you couple this with the amount of iron showing up on Pheobe, and possibly other saturn moons, the trend is undeniably at odds with the consensus model of solar evolution.
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jwj It's ok not to know. We should try harder to find out. |
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Btw where are the Genesis data? Cheers. |
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Cheers. |
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Hello everyone. I'm new, just tooling around and found my way here.
In case you're interested, Dr. Schultz is here at the Ames Vertical Gun Range this week conducting some experiments related to Deep Impact. I cannot go into too many specifics (he keeps these things tightly to himself until numbers are crunched and such), but I can answer general questions. As for me, I am an engineering tech here at NASA Ames, and have been one of the three operators of this and other light gas guns for the past 5+ years. Just thought I'd say hello and see if I could provide some insight into the research related to this event. |
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Hi Superheat, Welcome to the forum, I hope you can give some extra dimension to this Deep Impact thread, there's many questions and I hope you stick around to answer a few. Here's some for starters: the Deep Impact flyby camera showed an early flash (as Dr Schulz mentioned these were also seen at the Ames facility experiments) showing up in only one frame, meaning it lasted less that 50 mseconds, followed by several frames where "nothing happens" and then the plume starts erupting. How can this time be several frames (at least 100 msec) long? Do you know the specific numbers? At the speed of the impactor such a delay would mean it could have travelled almost a kilometer deep? That seems hardly possible, do you know what could have caused such a delay, maybe the early flash was not produced on impact, but before impact for whatever reason? Cheers. Last edited by VanderL; 08-December-2005 at 06:26 PM. |
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[My education is m.e.] My general question is...that's a vertically downward gun, right? [I won't ask about pumpkin ballistics.]Wouldn't penetration, even in talc-like material, require a narrow body? It was Newton who reasoned the displacement material would be accelerated to the speed of the object, roughly; so the cross section to mass ratio must remain small for serious penetration.
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Lighten up! This is a stellar board! Author: duh. "The Sun, with all the planets revolving around it, and depending on it, can still ripen a bunch of grapes as though it had nothing else in the universe to do..." Author: Galileo supposedly. |
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Thanks for the warm welcome!
I'll answer George's question first, and follow up with VanderL when I can get some answers from Pete :-) Quote:
I hope this is helpful, and I will find out more when I speak to Pete. Regards. |
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Lighten up! This is a stellar board! Author: duh. "The Sun, with all the planets revolving around it, and depending on it, can still ripen a bunch of grapes as though it had nothing else in the universe to do..." Author: Galileo supposedly. |
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Hoping to make up for my lack of cratering physics knowledge, how about a nice picture of Pete profiling a crater in the impact chamber? This was shot by me on 8/20/02 during some early DI research. Image Last edited by Wolverine; 09-December-2005 at 11:50 AM. Reason: Converted large image to URL. |
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Thanks, Superheat. We like to encourage the use of smaller images. I use Image Shack to host large images. You can then insert their thumbnail/link image. This reduces the board's load.
It is nice to see how you profile the crater. This image seems to show a broad crater for the size projectiles you mentioned. Interesting.
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Lighten up! This is a stellar board! Author: duh. "The Sun, with all the planets revolving around it, and depending on it, can still ripen a bunch of grapes as though it had nothing else in the universe to do..." Author: Galileo supposedly. |