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#31
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![]() "Thomas Lee Elifritz" wrote in message ... February 15, 2004 George wrote: As long as you make clear that you are speculating or making asumptions, you are probably going to be fine. It is when you make lots of assumptions and then make definite conclusions based on them that you and I get in trouble. Am I wrong? Yes. But only you are in trouble. Conclusions are called falsifiable hypotheses, crackpot. You test them, with experiments, and further evidence, to produce more conclusion and hypotheses. It's called the scientific method. However, being the crackpot that you are, you ridicule, then dismiss, and and remain skeptical, without offering any evidence, except that you still remain a crackpot. Thomas Lee Elifritz http://elifritz.members.atlantic.net Gee, I haven't felt the need to do this in a long, long time. So it gives me great pleasure to say to you PLONK! |
#32
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Hell why look for just primitives.......
How about a fossil Pisces feces facies ... :-) like in the Phosphoria. ;-) Bob "Rich Webb" wrote in message ... On Sat, 14 Feb 2004 14:59:26 GMT, "Sir Charles W. Shults III" wrote: [snip...snip...] If c) is true, then we have found what we are after. I notice that many of the spheres have odd characteristics, such as "tapered" ends, or small depressions. Could these be traces of some structure that an original organism had? Sponge-like critters would seem to be a possibility. They evolved very early here and have fossilized remains that are similar to some of the fragments. http://www.colossal-fossil-site.com/...07porifera.htm http://www.colossal-fossil-site.com/...06porifera.htm http://www.oum.ox.ac.uk/children/fossils/sponges.htm Of course, there's always the "Face on Mars" problem: Look at enough chunks of rock and eventually you'll see something recognizable. Would be cool, though... -- Rich Webb Norfolk, VA |
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February 15, 2004
George wrote: Am I wrong? Yes. But only you are in trouble. Conclusions are called falsifiable hypotheses, crackpot. You test them, with experiments, and further evidence, to produce more conclusion and hypotheses. It's called the scientific method. However, being the crackpot that you are, you ridicule, then dismiss, and and remain skeptical, without offering any evidence, except that you still remain a crackpot. Gee, I haven't felt the need to do this in a long, long time. So it gives me great pleasure to say to you PLONK! Crackpot keyword : 'plonk'. Another crackpot down, 6 billion more crackpots to go. Too bad they are breeding like ... rabbits. Thomas Lee Elifritz http://elifritz.members.atlantic.net |
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In article ,
says... snip The spherules found at the Apollo14 site, and at Opportunity are close to the same size (no larger than a few milimeters). The spherules at the Opportunity site are smaller than you must think they are. Note that rocks at the Apollo 14 site were similar to the bulk composition that appears to be seen at the Opportunity site: That is there is lots of olivine, which indicates that there is a basaltic source rock somewhere in the vicinity. The plagioclase at the Apollo 14 site no doubt originated from the basaltic rocks in which the craters in the region were formed. Well, there you are dead wrong. The plagioclase on the Moon was formed when the early Moon, just after accretion, developed a "magma ocean" in which plagioclase flotation resulted in an anorthositic crust. (Anorthosite is a rock made up mostly of a single mineral, plagioclase.) The plag at the Apollo 14 site was excavated from the highland materials (i.e., the brecciated remnants of the original lunar crust) in the target area of the Imbrium impact. The Fra Mauro formation on which Apollo 14 landed is a huge splash sheet of ejecta from the Imbrium impact -- very little (if any) rock from the original local surface remains on the surface at the landing site. According to the experts who have studied the Apollo 14 rock samples, not even Cone Crater was deep enough to punch through the Imbrium ejecta. So everything at Fra Mauro was originally located somewhere in what is now Mare Imbrium. The interesting thing is that there seems to have been a fair amount of mare basalt in the Imbrium target rock, since many of the clasts and some of the matrices in the breccias collected by Shepard and Mitchell are indeed basaltic, and analyze out at anywhere from 3.9 to 4.1 billion years old, considerably older than the age of the Imbrium impact itself (which is somewhere between 3.83 and 3.86 billion years). But the impact melt itself, as collected at Fra Mauro, is predominately noritic (anorthosite with some admixture of olivine). I'd like to see a cite for these "spherules" from the Apollo 14 collection -- I've seen a lot of discussion of the breccias from the site, and seen it noted that ALL of the Apollo 14 samples are indeed breccias. Perhaps you're thinking of spherical clasts within the breccias? I'd love to know which sample numbers you're speaking of... Doug |
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Doug... wrote:
OK, George, I'll buy that. Now, explain to me how you get a landslide on what appears to be topography that is extraordinarily flat for miles and miles in all directions? But just how flat is it? Have you seen the Opportunity landing bounce reconstruction? The initial bounce was to the north, yet with each successive bounce the path curved dramatically toward the west. I suppose this could have been caused by a strong easterly wind, although I'm a bit skeptical that such a thin atmosphere could cause something so massive to alter course that much. East is also not the typical wind diection given the plumes on the craters. Perhaps the terrain isn't as flat as it appears to be? Perhaps there is a slope to the whole plain, or perhaps there is a more localized slope, maybe from the ejecta from the large crater to the east. I suppose the answer is in the MOLA data, or perhaps in a 3-D ME image of the area (although I'm not aware of one of these yet). -- Greg Crinklaw Astronomical Software Developer Cloudcroft, New Mexico, USA (33N, 106W, 2700m) SkyTools Software for the Observer: http://www.skyhound.com/cs.html Skyhound Observing Pages: http://www.skyhound.com/sh/skyhound.html To reply remove spleen |
#37
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![]() " George" wrote I think it is safe to say that the analysis it made is representative of the area as a whole. FWIW, here is a great montage Doug Ellison made of part of the outcrop, with the blueberries resplendent & some idea of the variation. http://mer.rlproject.com/index.php?a...pe=post&id=111 (warning: big file) Joe |
#38
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![]() "Greg Crinklaw" wrote in message ... Doug... wrote: OK, George, I'll buy that. Now, explain to me how you get a landslide on what appears to be topography that is extraordinarily flat for miles and miles in all directions? But just how flat is it? Have you seen the Opportunity landing bounce reconstruction? The initial bounce was to the north, yet with each successive bounce the path curved dramatically toward the west. I suppose this could have been caused by a strong easterly wind, although I'm a bit skeptical that such a thin atmosphere could cause something so massive to alter course that much. East is also not the typical wind diection given the plumes on the craters. Perhaps the terrain isn't as flat as it appears to be? Perhaps there is a slope to the whole plain, or perhaps there is a more localized slope, maybe from the ejecta from the large crater to the east. I suppose the answer is in the MOLA data, or perhaps in a 3-D ME image of the area (although I'm not aware of one of these yet). -- Greg Crinklaw Astronomical Software Developer Cloudcroft, New Mexico, USA (33N, 106W, 2700m) SkyTools Software for the Observer: http://www.skyhound.com/cs.html Skyhound Observing Pages: http://www.skyhound.com/sh/skyhound.html To reply remove spleen If you look at the topographic map at the following link, you will note the the site does slope from northeast to southwest. http://marsoweb.nas.nasa.gov/dataViz.../HematiteWest/ Also note that the region is a large filled crater. Now, there may be landslides buried under the sediments. Given that it was formerly a large crater, I do not think there is a doubt that you could find landslide deposits within the crater. However, since the northeastern quadrant of the crater has been completely filled, and appears to be filled nearly to the center of the crater, I find it highly unlikely that the Opportunity site and vicinity would contains surface exposures of landslide material, unless you looked deep into some of the larger craters. It will be interesting to see what Opportunity finds when it makes its journey to the larger crater in the coming weeks. |
#39
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![]() "Doug..." wrote in message ... In article , says... snip But we see the same phenomenon in landslides in desert regions on the earth. There is evidence that some large landslides will behave as a fluid due to the creation of a layer of compressed air between the landslide material and the ground upon which it is sliding. Such a layer acts like a lubricant that reduces friction, and will allow the slide to behave as a fluid. In the case of Mars, the air would consist of the CO2 atmosphere. Now, I am not saying that water doesn't exist on Mars. Obviously it does, at least at the poles. And of course, we have all seen some evidence that there may be ground water, and/or frozen water in the subsurface. What I am saying is that there are other explanations for the fluid appearance of these landslides on Mars. OK, George, I'll buy that. Now, explain to me how you get a landslide on what appears to be topography that is extraordinarily flat for miles and miles in all directions? The simple answer is that you don't. The more complex answer is that the region is a large filled crater, that indeed may have older deposts composed of landslide fill buried deep within the crater fill deposits. Noting in the following link that the fill material comes from the northeast, and has nearly completely filled the crater to the center, and sloping to the southwest towards the crater wall, I find it highly unlikely that there are landslide desposits exposed at the surface in the vicinity of Opportunity. The only likely place where you could view such landslide deposits would be possibly within the walls and floor of a large crater that has breeched the surface deposits of the plain. Such a potential crater, in fact is within traveling distance of Opportunity, and I think they plan to drive there in the coming weeks. As I mentioned before, there are no large craters that would create these "splash" landforms as ejecta, at least not in the right place to have caused the effects visible in the DIMES images. They don't have to be close by. There are so many craters, both large and small on Mars that any one of them, or at least most of the larger ones could have ejected material that could travel completely around the Martian globe, and even sent material into orbit. This material has to come down somewhere, and just as often as not, it will land somewhere other than in proximity to where it originated. I would not be at all surprised to find that material from craters that do exist in the vicinity to have left material at the Opportunity site. In fact, I would be very surprised if they didn't. I'm not saying that water has flowed over or under this surface recently. It may have been more than a billion years since water flowed over this surface. But I believe it's very possible that water HAS had a hand in the sculpting of the surface we're observing, even at very high resolution. Doug What features are present that leads you to believe that flowing water has had a hand in sculpturing the landscape at the Opportunity landing site and/or vicinity? And please try to restrict you answer to features that could only have come from the flow of water, and nothing else. |
#40
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![]() "Joe Knapp" wrote in message .com... " George" wrote I think it is safe to say that the analysis it made is representative of the area as a whole. FWIW, here is a great montage Doug Ellison made of part of the outcrop, with the blueberries resplendent & some idea of the variation. http://mer.rlproject.com/index.php?a...pe=post&id=111 (warning: big file) Joe Thank you for that link. That is quite a good montage. I must say that it is quite annoying that JPL doesn't post these images in final form on their web site. I guess my problem all along has been to rely on the spottiness of their color image posts. And the fact that never having had to do the colorizing myself also makes matters worse. It was only recently that I even figured out how to do this, so thanks to whoever posted that information. Having said that, I find the color of the outcrop to be very intriquing, as it looks just like some rhyolites I've seen in the field in the Western U.S. That doesn't mean that I think the rock IS rhyolite, hoever, as I've never heard of rhyolites with concentration of sulfure that this rock has. What software are they using to generate the color images? I have several that could possibly be used (Corel PhotoPaint, Adobe Photoshop, Corel Painter 8, Picture Window Pro, and Astrovideo,which is great for processing black and white CCD astro photos into color using color filters). Unfortunately, the art of colorizing is fairly new to me. By the way, don't be stingy about posting links to great pics such as this one. Since JPL isn't posting many color-processed images directly into their web site, People like me are scarmbling to find them. another annoyance is that they don't post higher resolution images. The Mars Express site is posting images at 300 and 400 dpi, while we have to rely on 72 and 96 dpi images. Screw the file size: I have adsl! I want HIGH resolution! The larger, the better. Again, thanks. As an aside commentary, I find the purplish "reaction"? discoloration on the rocks where there are "berries embedded in them very interesting, indeed. Any comments on them? |
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