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#51
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asteroid close approach, 2011 Nov 08
On Nov 8, 9:37*am, Chris L Peterson wrote:
On Tue, 8 Nov 2011 03:23:11 -0800 (PST), wrote: The "policy skills" to which you seemed to have alluded are inherently unethical and would always be unwise. Precisely the immature viewpoint that demonstrates our societal weaknesses! Your statement demonstrates your ignorance and naivete. Any "policy" that advocates the control or guidance of future human evolution is merely eugenics in disguise. Inevitably, the rights of some people would be violated. At least BT included a mild disclaimer when he mentioned the idea. You weren't even smart enough to do that. |
#52
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asteroid close approach, 2011 Nov 08
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#53
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asteroid close approach, 2011 Nov 08
On Nov 1, 12:35*pm, wrote:
The article at the link below indicates a forthcoming asteroid approach by 2005 YU55 to within 325,000 km of Earth and states that the object is about 400m across. I would imagine that such an object would be quite bright! How bright will it get, and which hemisphere is favored observation-wise? http://www.scientificamerican.com/po...d=asteroid-pla.... That imaging opportunity of YU55 was certainly a big disappointment. Good thing that much like our physically dark moon, whereas each giving off a great deal of IR is what made the little fuzzy dot via KECK materialize. They must have been utilizing their very least possible magnification, as almost a wide-angle FOV compared to what KECK has previously demonstrated. However, it does demonstrate just how physically dark items like YU55 and our moon really are. Perhaps those radar images of 2 meter resolution will eventually surface and get resampled for their best interpretation of YU55. Instead they give us crappy movies of it that cuts the resolution potential down by a good 10:1, instead of frame stacking and PhotoShop resampling, and there's still nothing of gamma spectrometry to speak of, as well as no better determination of its mass. Of course this means that those Muslim ETs could just as easily hit us with a full blown WMD km sized black rock of 8+ g/cm3 density, and at best our crack team KECK would only detect a little fuzzy IR imaged dot as of the same day as the impact would take place. http://translate.google.com/# Brad Guth, Brad_Guth, Brad.Guth, BradGuth, BG / “Guth Usenet” |
#54
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asteroid close approach, 2011 Nov 08
On Nov 2, 4:46*pm, StarDust wrote:
That's about the Moon's orbit, so not very close. It passed near 16% closer than the moon. That most recent imaging opportunity of YU55 was certainly a big disappointment. Good thing that much like our physically dark moon, whereas each of these items giving off a great deal of IR is what made the little fuzzy dot via KECK materialize. They must have been utilizing their very least possible magnification, as almost a wide-angle FOV compared to what KECK has previously demonstrated. However, it does a good job of demonstrate just how physically dark items like YU55 and our moon really are. Perhaps those radar images of 2 meter resolution will eventually surface and get sufficiently stacked and resampled for their best interpretation of YU55. Instead they give us crappy movies of it that cuts their resolution potential down by a good 10:1, instead of proper frame stacking and PhotoShop resampling, and there's still nothing of gamma spectrometry to speak of, as well as no better determination of its mass, so it must be a heavy sucker that we outsiders are not supposed to know anything about. Of course this means that those Muslim ETs could just as easily hit us with a full blown WMD of a km sized black rock of 8+ g/cm3 density, and at best our crack team KECK would only detect a little fuzzy IR imaged dot as of the same day as the impact would take place. http://translate.google.com/# Brad Guth, Brad_Guth, Brad.Guth, BradGuth, BG / “Guth Usenet” |
#55
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asteroid close approach, 2011 Nov 08
On 11/9/11 12:21 PM, Brad Guth wrote:
That imaging opportunity of YU55 was certainly a big disappointment. http://apod.nasa.gov/apod/ap111109.html |
#56
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asteroid close approach, 2011 Nov 08
On Wed, 9 Nov 2011 10:32:55 -0800 (PST), Brad Guth
wrote: Good thing that much like our physically dark moon, whereas each of these items giving off a great deal of IR is what made the little fuzzy dot via KECK materialize. They must have been utilizing their very least possible magnification, as almost a wide-angle FOV compared to what KECK has previously demonstrated. The term "magnification" means nothing in this context. The telescope was used at its highest possible resolution. The IR in this case was near IR, not long wavelength (thermal) IR. The asteroid is not IR bright at this wavelength; near IR is used by Keck for adaptive optics because of the physics behind the process. |
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asteroid close approach, 2011 Nov 08
On 11/9/2011 1:48 PM, Chris L Peterson wrote:
On Wed, 9 Nov 2011 10:32:55 -0800 (PST), Brad Guth wrote: Good thing that much like our physically dark moon, whereas each of these items giving off a great deal of IR is what made the little fuzzy dot via KECK materialize. They must have been utilizing their very least possible magnification, as almost a wide-angle FOV compared to what KECK has previously demonstrated. The term "magnification" means nothing in this context. The telescope was used at its highest possible resolution. The IR in this case was near IR, not long wavelength (thermal) IR. The asteroid is not IR bright at this wavelength; near IR is used by Keck for adaptive optics because of the physics behind the process. Just curious did you get any images of this asteroid ? I check your web page every meteor shower and for new images. Have not seen any new images from you in a while except for meteors. -- AM http://sctuser.home.comcast.net http://www.novac.com |
#58
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asteroid close approach, 2011 Nov 08
On Wed, 09 Nov 2011 16:27:57 -0500, AM wrote:
Just curious did you get any images of this asteroid ? No, I was out of town last night. Had I been home, I might have tried- just for kicks, mainly. I check your web page every meteor shower and for new images. Have not seen any new images from you in a while except for meteors. I got bored with aesthetic imaging, so I don't do much of it lately. Besides the meteor work, most of what I do now is photometry, and I haven't been posting that work. |
#59
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asteroid close approach, 2011 Nov 08
On Nov 9, 10:21*am, Brad Guth wrote:
That imaging opportunity of YU55 was certainly a big disappointment. From some of the local amateurs... http://www.youtube.com/watch?v=u25iC...ature=youtu.be |
#60
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asteroid close approach, 2011 Nov 08
On Nov 9, 10:48*am, Chris L Peterson wrote:
On Wed, 9 Nov 2011 10:32:55 -0800 (PST), Brad Guth wrote: Good thing that much like our physically dark moon, whereas each of these items giving off a great deal of IR is what made the little fuzzy dot via KECK materialize. *They must have been utilizing their very least possible magnification, as almost a wide-angle FOV compared to what KECK has previously demonstrated. The term "magnification" means nothing in this context. The telescope was used at its highest possible resolution. The IR in this case was near IR, not long wavelength (thermal) IR. The asteroid is not IR bright at this wavelength; near IR is used by Keck for adaptive optics because of the physics behind the process. It was a good one of proving just how physically dark our moon actually is. KECK could have accomplished at least ten fold better resolution, but that would have been problematic for NASA. http://translate.google.com/# Brad Guth, Brad_Guth, Brad.Guth, BradGuth, BG / “Guth Usenet” |
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