Difference between revisions of "October 14, 2004"
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| − | + | <td width="50%"><h2><nobr>A Rille, No Rim and a Rain of Ejecta</nobr></h2></td> | |
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| − | + | <tr><td colspan="2" valign="top"><div align="center"> | |
| − | + | <img src="archive/2004/10/images/LPOD-2004-10-14.jpeg" border="0"> | |
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<table width="80%" border="0" align="center" cellpadding="8"> | <table width="80%" border="0" align="center" cellpadding="8"> | ||
| − | + | <tr><td><div align="center" class="main_sm">Image Credit: [mailto:alessandro.bertoglio@fastwebnet.it Alessandro Bertoglio]</p> | |
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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 align="center"><b>A Rille, No Rim and a Rain of Ejecta</b></p> | |
| − | + | <p align="left">North of Mare Imbrium, towards the lunar north pole, is a region considerably different than the southern pole. Instead of towering mountains and deep craters, the topography of the region poleward of 60 degrees N latitude is battered and muted with only an occasional younger [http://www.lpod.org/archive/2004/05/LPOD-2004-05-14.htm crater] to attract attention. What happened? This image of the half crater known as Gartner provides a clue. At 102 km wide, Gartner probably looked like Copernicus about 4 billion years ago. But then at 3.85 billion years ago a gigantic impact excavated the Imbrium basin, spewing ejecta in all directions. Much of the north polar region was splattered with mountains and boulders and flour size ejecta. The hilly rubble in Gartner is probably part of the ejecta and the smoother material surrounding the hills may also be from Imbrium. Apparently the area of Mare Frigoris subsided, carrying down the southern rim of Gartner, which was covered by later Frigoris lavas. The rille in Gartner is hard to explain. It is not radial or concentric to a basin (perhaps it could be considered radial to Serenitatis), and if it formed in ejecta rather than lava, it can not be a lava tube. Perhaps the smooth plains material is older, non-mare composition lava. In fact, with full Moon [http://www.lpi.usra.edu/research/cla/info/ai/ lighting] the areas around the small craters near the rille's north end appear dark, like a pyroclastic deposit. This area is not covered by good Lunar Orbiter imagery and has not been investigated fully.</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> | ||
Sept 3, 2004, 2:31 UT. Takahashi Mewlon 300 + 3x barlow + anti-IR filter + SBIG ST7 XME CCD. Median of 10 1/10 s exposures of 181 obtained. Processed with Astroart 3.0 and Photoshop. | Sept 3, 2004, 2:31 UT. Takahashi Mewlon 300 + 3x barlow + anti-IR filter + SBIG ST7 XME CCD. Median of 10 1/10 s exposures of 181 obtained. Processed with Astroart 3.0 and Photoshop. | ||
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<br>Bussey & Spudis <i>Clementine Atlas of the Moon</i> Sheet 13 | <br>Bussey & Spudis <i>Clementine Atlas of the Moon</i> Sheet 13 | ||
<p align="left"><b>Tomorrow's LPOD: </b> A Lumpy Mare</p> | <p align="left"><b>Tomorrow's LPOD: </b> A Lumpy Mare</p> | ||
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</table> | </table> | ||
<br> | <br> | ||
<table width="100%" border="0" cellspacing="2" cellpadding="4"> | <table width="100%" border="0" cellspacing="2" cellpadding="4"> | ||
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| − | + | <td><hr></td> | |
| − | + | </tr> | |
| − | + | <tr><td> | |
| − | + | <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> | |
| − | + | </td></tr> | |
</table> | </table> | ||
<p> </p> | <p> </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 18:26, 4 January 2015
A Rille, No Rim and a Rain of Ejecta
<nobr>A Rille, No Rim and a Rain of Ejecta</nobr> |
<img src="archive/2004/10/images/LPOD-2004-10-14.jpeg" border="0"> |
Image Credit: Alessandro Bertoglio
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|
A Rille, No Rim and a Rain of Ejecta North of Mare Imbrium, towards the lunar north pole, is a region considerably different than the southern pole. Instead of towering mountains and deep craters, the topography of the region poleward of 60 degrees N latitude is battered and muted with only an occasional younger crater to attract attention. What happened? This image of the half crater known as Gartner provides a clue. At 102 km wide, Gartner probably looked like Copernicus about 4 billion years ago. But then at 3.85 billion years ago a gigantic impact excavated the Imbrium basin, spewing ejecta in all directions. Much of the north polar region was splattered with mountains and boulders and flour size ejecta. The hilly rubble in Gartner is probably part of the ejecta and the smoother material surrounding the hills may also be from Imbrium. Apparently the area of Mare Frigoris subsided, carrying down the southern rim of Gartner, which was covered by later Frigoris lavas. The rille in Gartner is hard to explain. It is not radial or concentric to a basin (perhaps it could be considered radial to Serenitatis), and if it formed in ejecta rather than lava, it can not be a lava tube. Perhaps the smooth plains material is older, non-mare composition lava. In fact, with full Moon lighting the areas around the small craters near the rille's north end appear dark, like a pyroclastic deposit. This area is not covered by good Lunar Orbiter imagery and has not been investigated fully. Technical Details: Related Links: Tomorrow's LPOD: A Lumpy Mare |
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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.
