Difference between revisions of "May 13, 2005"
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| − | + | <td width="50%"><h2><nobr>Hotspots Identified!</nobr></h2></td> | |
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| − | + | <tr><td><div align="center" class="main_sm">Image Credit: [mailto:bill@bblevins.com Bill & Julie Blevins]</p> | |
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| − | + | <p align="center"><b>Hotspots Identified!</b></p> | |
| − | + | <p align="left">LPOD for [http://www.lpod.org/LPOD-2005-04-28.htm April 28] featured a red Moon created by the MSX satellite that imaged infrared radiation as the Moon cooled during an eclipse. My strong enhancement of the image revealed many hot spots that were probably due to bare rock surfaces inside the youngest craters on the Moon. I ended the LPOD by hoping that somewhat would merge the enhanced infrared image with a normal full Moon view to enable the identification of the young craters. And that is exactly what Bill Blevins did - a mouseover will show one of Bills full Moon images and moving your mouse on and off the image will allow you to quickly move between the two images. Julie Blevins undertook the task of identifying some of the brightest craters. But many more less bright ones exist. It would be a fascinating project for someone to identify as many of these craters as possible and see if they are very fresh and have rays. The Blevins good work has revealed that there is a good study hiding in these images!</p> | |
| − | + | <blockquote><p align="right">— [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote> | |
<p align="left"><p><b>Technical Details:</b><br> | <p align="left"><p><b>Technical Details:</b><br> | ||
Here is how Bill did it. He used one of his full Moon images from 9/27/04 and transformed it in Photoshop to correct for rotation/libration differences. He then put the two in a flash animation for comparison. Click [http://www.bblevins.com/temp/infrared_moon_compare.html here] to see the animation.</p> | Here is how Bill did it. He used one of his full Moon images from 9/27/04 and transformed it in Photoshop to correct for rotation/libration differences. He then put the two in a flash animation for comparison. Click [http://www.bblevins.com/temp/infrared_moon_compare.html here] to see the animation.</p> | ||
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[http://www.ipac.caltech.edu/ipac/msx/msx.html MSX Team] | [http://www.ipac.caltech.edu/ipac/msx/msx.html MSX Team] | ||
<p align="left"><b>Tomorrow's LPOD: </b> Ancient Island</p> | <p align="left"><b>Tomorrow's LPOD: </b> Ancient Island</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>Contact Translator:</b><br> | |
| − | + | [mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey] (Es)<br> | |
| − | + | [mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p> | |
| − | + | <p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p> | |
| − | + | <p align="center" class="main_titles"><b>A service of:</b><br> | |
| − | + | [http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p> | |
| − | + | <p align="center" class="main_titles"><b>Visit these other PODs:</b> <br> | |
| − | + | [http://antwrp.gsfc.nasa.gov/apod/astropix.html" class="one Astronomy] | [http://www.msss.com/" class="one Mars] | [http://epod.usra.edu/" class="one Earth]</p> | |
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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 18:32, 4 January 2015
Hotspots Identified!
<nobr>Hotspots Identified!</nobr> |
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Image Credit: Bill & Julie Blevins
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Hotspots Identified! LPOD for April 28 featured a red Moon created by the MSX satellite that imaged infrared radiation as the Moon cooled during an eclipse. My strong enhancement of the image revealed many hot spots that were probably due to bare rock surfaces inside the youngest craters on the Moon. I ended the LPOD by hoping that somewhat would merge the enhanced infrared image with a normal full Moon view to enable the identification of the young craters. And that is exactly what Bill Blevins did - a mouseover will show one of Bills full Moon images and moving your mouse on and off the image will allow you to quickly move between the two images. Julie Blevins undertook the task of identifying some of the brightest craters. But many more less bright ones exist. It would be a fascinating project for someone to identify as many of these craters as possible and see if they are very fresh and have rays. The Blevins good work has revealed that there is a good study hiding in these images! Technical Details: Related Links: Tomorrow's LPOD: Ancient Island |
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Author & Editor: Technical Consultant: Contact Translator: A service of: Visit these other PODs: |
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.
