Difference between revisions of "October 22, 2012"
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=Crazy Quilt Imbrium= | =Crazy Quilt Imbrium= | ||
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<em>image processed by Jeff Gillis and Paul Lucey, University of Hawaii</em><br /> | <em>image processed by Jeff Gillis and Paul Lucey, University of Hawaii</em><br /> | ||
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| − | Are you lost looking at this image? Its our Moon, but as seen through very odd spectral glasses. To help get your bearings I've labeled some craters: A = Aristarchus, C = Copernicus, H = Harpalus, P = Plato; you can figure out the rest! Where did this image come from? The Clementine spacecraft imaged the Moon in 11 wavelengths, including 6 in the near infrared. As an aside: The NIR images have finally been calibrated so they can be used to identify various elements and minerals. Jeff Gillis and Paul Lucey used this data to search for evidence of water-bearing minerals. Alas, they found none (including at Reiner Gamma which is sometimes interpreted as a comet impact). They did, however, find that a resultant image made by ratioing images acquired in the visible and red regions of the spectrum dramatically distinguishes many different lava flows, presumably with different compositions. Some of these flows - such as the one in the middle of Imbrium - are well known, but others have never before been delineated so carefully. It is remarkable that [http://www.lpod.org/archive/archive/2004/01/LPOD-2004-01-28.htm amateur images] with commercial digital cameras can pick up some of these flows. I bet that digital imaging through color filters could approach this Clementine derived image in detecting lava flows with only subtle color differences. Who will be first to try it?<br /> | + | Are you lost looking at this image? Its our Moon, but as seen through very odd spectral glasses. To help get your bearings I've labeled some craters: A = Aristarchus, C = Copernicus, H = Harpalus, P = Plato; you can figure out the rest! Where did this image come from? The Clementine spacecraft imaged the Moon in 11 wavelengths, including 6 in the near infrared. As an aside: The NIR images have finally been calibrated so they can be used to identify various elements and minerals. Jeff Gillis and Paul Lucey used this data to search for evidence of water-bearing minerals. Alas, they found none (including at Reiner Gamma which is sometimes interpreted as a comet impact). They did, however, find that a resultant image made by ratioing images acquired in the visible and red regions of the spectrum dramatically distinguishes many different lava flows, presumably with different compositions. Some of these flows - such as the one in the middle of Imbrium - are well known, but others have never before been delineated so carefully. It is remarkable that [http://www.lpod.org/archive/archive/2004/01/LPOD-2004-01-28.htm" rel="nofollow amateur images] with commercial digital cameras can pick up some of these flows. I bet that digital imaging through color filters could approach this Clementine derived image in detecting lava flows with only subtle color differences. Who will be first to try it?<br /> |
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| − | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | + | <em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><br /> |
| − | Note - I am still traveling so here is another classic LPOD from [http://www.lpod.org/archive/archive/2004/02/LPOD-2004-02-08.htm Feb 8, 2004]<br /> | + | Note - I am still traveling so here is another classic LPOD from [http://www.lpod.org/archive/archive/2004/02/LPOD-2004-02-08.htm" rel="nofollow Feb 8, 2004]<br /> |
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<strong>Technical Details</strong><br /> | <strong>Technical Details</strong><br /> | ||
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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
| − | [http://www.lpi.usra.edu/meetings/lpsc2004/pdf/2158.pdf Clementine 2.7 Micrometer Data: Mapping the mare and searching for water.] JJ Gillis & PG Lucey, Lunar & Planetary Science XXXV (2004)<br /> | + | [http://www.lpi.usra.edu/meetings/lpsc2004/pdf/2158.pdf" rel="nofollow Clementine 2.7 Micrometer Data: Mapping the mare and searching for water.] JJ Gillis & PG Lucey, Lunar & Planetary Science XXXV (2004)<br /> |
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Revision as of 22:37, 4 January 2015
Crazy Quilt Imbrium
image processed by Jeff Gillis and Paul Lucey, University of Hawaii
Are you lost looking at this image? Its our Moon, but as seen through very odd spectral glasses. To help get your bearings I've labeled some craters: A = Aristarchus, C = Copernicus, H = Harpalus, P = Plato; you can figure out the rest! Where did this image come from? The Clementine spacecraft imaged the Moon in 11 wavelengths, including 6 in the near infrared. As an aside: The NIR images have finally been calibrated so they can be used to identify various elements and minerals. Jeff Gillis and Paul Lucey used this data to search for evidence of water-bearing minerals. Alas, they found none (including at Reiner Gamma which is sometimes interpreted as a comet impact). They did, however, find that a resultant image made by ratioing images acquired in the visible and red regions of the spectrum dramatically distinguishes many different lava flows, presumably with different compositions. Some of these flows - such as the one in the middle of Imbrium - are well known, but others have never before been delineated so carefully. It is remarkable that " rel="nofollow amateur images with commercial digital cameras can pick up some of these flows. I bet that digital imaging through color filters could approach this Clementine derived image in detecting lava flows with only subtle color differences. Who will be first to try it?
" rel="nofollow Chuck Wood
Note - I am still traveling so here is another classic LPOD from " rel="nofollow Feb 8, 2004
Technical Details
Image formed from the 415/750 ratio of calibrated Clementine image mosaics taken with 0.415 and 0.75 micrometer wavelength filters. 0° to 70°N, 70°W to 30°E. The vertical white and black bars are areas lacking data. The bottom image (or the right one if you have a big monitor) shows this exact area in a more familiar perspective (through a visible filter - 0.415 micrometer).
Related Links
" rel="nofollow Clementine 2.7 Micrometer Data: Mapping the mare and searching for water. JJ Gillis & PG Lucey, Lunar & Planetary Science XXXV (2004)
