Difference between revisions of "February 8, 2004"
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=Crazy Quilt Imbrium= | =Crazy Quilt Imbrium= | ||
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| − | + | [LPOD-2004-02-08b.htm [[File:LPOD-2004-02-08.jpeg|LPOD-2004-02-08.jpeg]]]</div> | |
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| − | + | <td><div align="center" span class="main_sm">Image Credit: [mailto:gillis@higp.hawaii.edu Jeff Gillis] and Paul Lucey, University of Hawaii</div></td> | |
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<table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td> | <table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td> | ||
| − | + | <p class="story" align="center"><b>Crazy Quilt Imbrium </b></p> | |
| − | + | <p class="story" align="left">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! 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 | |
| − | + | bright one in the middle of Imbrium - are well known, but others have never before been delineated so carefully. | |
| − | + | It is remarkable that [../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?</p> | |
| − | + | <p><b>Technical Details:</b><br> | |
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Image formed from the 415/750 ratio of calibrated Clementine image mosaics taken with 0.415 and 0.75 | 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 | micrometer wavelength filters. 0° to 70°N, 70°W to 30°E. The vertical white and black bars are areas | ||
lacking data. To see this exact area in a more familiar perspective (through a visible filter - | lacking data. To see this exact area in a more familiar perspective (through a visible filter - | ||
0.415 micrometer) click the image. </p> | 0.415 micrometer) click the image. </p> | ||
| − | + | <p class="story"><b>Related Links:</b><br> | |
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[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)</p> | [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)</p> | ||
| − | + | <p class="story"> <b>Tomorrow's LPOD:</b> Seeing Double: Pythagoras</p> | |
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| − | + | <p align="center" class="main_titles"><b>Author & Editor:</b><br> | |
| − | + | [mailto:tychocrater@yahoo.com Charles A. Wood]</p> | |
| − | + | <p align="center" class="main_titles"><b>Technical Consultant:</b><br> | |
| − | + | [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p> | |
| − | + | <p align="center" class="main_titles"><b>A service of:</b><br> | |
| − | + | [http://www.observingthesky.org/ ObservingTheSky.Org]</p> | |
| − | + | <p align="center" class="main_titles"><b>Visit these other PODs:</b> <br> | |
| − | + | [http://antwrp.gsfc.nasa.gov/apod/astropix.html Astronomy] | [http://www.msss.com/ Mars] | [http://epod.usra.edu/ Earth]</p></td> | |
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===COMMENTS?=== | ===COMMENTS?=== | ||
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment. | Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment. | ||
Revision as of 18:15, 4 January 2015
Crazy Quilt Imbrium
[LPOD-2004-02-08b.htm
 ] |
Image Credit: Jeff Gillis and Paul Lucey, University of Hawaii |
|
Crazy Quilt Imbrium 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! 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 bright one in the middle of Imbrium - are well known, but others have never before been delineated so carefully. It is remarkable that [../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? Technical Details: Related Links: Tomorrow's LPOD: Seeing Double: Pythagoras |
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Author & Editor: Technical Consultant: A service of: |
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.
