Difference between revisions of "May 4, 2004"
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=Inside Nectaris= | =Inside Nectaris= | ||
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| − | <td><div align="center | + | <td><div align="center">Image Credit: [mailto:berryfam850@earthlink.net Peter Berry]</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>Inside Nectaris</b></p> | <p class="Story" align="center"><b>Inside Nectaris</b></p> | ||
| − | <p class="story" align="left">Mare Nectaris is one of the smallest mare on the floor of an impact basin. This low sun mosaic by Peter Berry provides a close-up view of relations between the mare lavas and adjacent impact craters. The center of the mare is mostly unscarred and is the top of a relatively thin (~ 1 km thick) frozen lava lake; most of the action is nearer the mare's edges. At top left (NW) is [ | + | <p class="story" align="left">Mare Nectaris is one of the smallest mare on the floor of an impact basin. This low sun mosaic by Peter Berry provides a close-up view of relations between the mare lavas and adjacent impact craters. The center of the mare is mostly unscarred and is the top of a relatively thin (~ 1 km thick) frozen lava lake; most of the action is nearer the mare's edges. At top left (NW) is [[February_1,_2004|Theophilus]], whose ejecta cut into and overlays the nearby mare - Theophilus is obviously younger than the mare. At the bottom of the image is [[April_6,_2004|Fracastorius]] which was tilted toward the center of the basin and then flooded with mare lava - Fracastorius formed during the period of lava flooding. At the north end of Nectaris is the ruined crater Daguerre. Its called a ruin on the assumption that it was originally a normal impact crater that has been nearly completely overwhelmed by mare lavas. It could be a smaller, and more deeply covered version of Fracastorius, and it probably is. But there are some peculiar aspects that suggest local volcanism too. Daguerre has an associated 300 km2 pyroclastic deposit, and has peculiar double rims near its northern end. And in case any one is interested in odd analogues, Peter points out the resemble of Fracastorius, with its ovoid shape, pockmarked surface, and the rounded-off edges to a prickly pear cactus pad!</p> |
<p class="story"><b>Related Links:</b><br>[http://www.lpi.usra.edu/research/lunar_orbiter/bin/info.shtml?164 Lunar Orbiter IV View]</p> | <p class="story"><b>Related Links:</b><br>[http://www.lpi.usra.edu/research/lunar_orbiter/bin/info.shtml?164 Lunar Orbiter IV View]</p> | ||
<p class="story"><b>Technical Details:</b><br> | <p class="story"><b>Technical Details:</b><br> | ||
Composite of two images from 11/23/02, taken with the I-M Alter-603 MCT afocally using the Sony TRV-900 camcorder, composited in the Photoshop Elements photomerge utility. Click for larger view.</p> | Composite of two images from 11/23/02, taken with the I-M Alter-603 MCT afocally using the Sony TRV-900 camcorder, composited in the Photoshop Elements photomerge utility. Click for larger view.</p> | ||
| − | <p | + | <p><b>Yesterday's LPOD:</b> [[May 3, 2004|Bully for Bullialdus!]] </p> |
| − | </p> | + | <p><b>Tomorrow's LPOD:</b> [[May 5, 2004|Magnificent Greek Eclipse!]] </p> |
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<td><p align="center" class="main_titles"><b>Author & Editor:</b><br> | <td><p align="center" class="main_titles"><b>Author & Editor:</b><br> | ||
[mailto:tychocrater@yahoo.com Charles A. Wood]</p> | [mailto:tychocrater@yahoo.com Charles A. Wood]</p> | ||
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Latest revision as of 18:16, 7 February 2015
Inside Nectaris
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Image Credit: Peter Berry |
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Inside Nectaris Mare Nectaris is one of the smallest mare on the floor of an impact basin. This low sun mosaic by Peter Berry provides a close-up view of relations between the mare lavas and adjacent impact craters. The center of the mare is mostly unscarred and is the top of a relatively thin (~ 1 km thick) frozen lava lake; most of the action is nearer the mare's edges. At top left (NW) is Theophilus, whose ejecta cut into and overlays the nearby mare - Theophilus is obviously younger than the mare. At the bottom of the image is Fracastorius which was tilted toward the center of the basin and then flooded with mare lava - Fracastorius formed during the period of lava flooding. At the north end of Nectaris is the ruined crater Daguerre. Its called a ruin on the assumption that it was originally a normal impact crater that has been nearly completely overwhelmed by mare lavas. It could be a smaller, and more deeply covered version of Fracastorius, and it probably is. But there are some peculiar aspects that suggest local volcanism too. Daguerre has an associated 300 km2 pyroclastic deposit, and has peculiar double rims near its northern end. And in case any one is interested in odd analogues, Peter points out the resemble of Fracastorius, with its ovoid shape, pockmarked surface, and the rounded-off edges to a prickly pear cactus pad! Related Links: Technical Details: Yesterday's LPOD: Bully for Bullialdus! Tomorrow's LPOD: Magnificent Greek Eclipse! |
Author & Editor:
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