Difference between revisions of "October 23, 2004"
| (6 intermediate revisions by the same user not shown) | |||
| Line 1: | Line 1: | ||
__NOTOC__ | __NOTOC__ | ||
=Imaging the First Lunar Photographer= | =Imaging the First Lunar Photographer= | ||
| + | <!-- Start of content --> | ||
<table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | <table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | ||
<tr> | <tr> | ||
| Line 12: | Line 13: | ||
</table> | </table> | ||
<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:starman2@flash.net Wes Higgins]</p> | + | <tr><td><div align="center" class="main_sm"><p>Image Credit: [mailto:starman2@flash.net Wes Higgins]</p> |
</div></td> | </div></td> | ||
</tr> | </tr> | ||
| Line 25: | Line 26: | ||
Sept 3, 2004. Starmaster 14.5 + DMK-21F04 camera at 30FPS; stack of 864 frames from 3000.</p> | Sept 3, 2004. Starmaster 14.5 + DMK-21F04 camera at 30FPS; stack of 864 frames from 3000.</p> | ||
<p><b>Related Links:</b><br> | <p><b>Related Links:</b><br> | ||
| − | [ | + | [http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_072_h2.jpg Lunar Orbiter IV View] |
<br>Rukl <i>Atlas of the Moon,</i> Sheet 47 | <br>Rukl <i>Atlas of the Moon,</i> Sheet 47 | ||
</p> | </p> | ||
| − | <p | + | <p><b>Yesterday's LPOD:</b> [[October 22, 2004|H-Alpha Moon]] </p> |
| + | <p><b>Tomorrow's LPOD:</b> [[October 24, 2004|A Long, Cold Mare]] </p> | ||
</tr> | </tr> | ||
</table> | </table> | ||
| Line 39: | Line 41: | ||
<p align="center" class="main_titles"><b>Author & Editor:</b><br> | <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> | ||
| − | < | + | <!-- Cleanup of credits --> |
| − | + | <!-- Cleanup of credits --> | |
| − | < | + | <!-- Cleanup of credits --> |
| − | + | <!-- Cleanup of credits --> | |
| − | + | <!-- Cleanup of credits --> | |
| − | < | + | <!-- Cleanup of credits --> |
| − | < | + | <!-- Cleanup of credits --> |
| − | + | <!-- Cleanup of credits --> | |
| − | < | + | <!-- Cleanup of credits --> |
| − | + | <!-- Cleanup of credits --> | |
</td></tr> | </td></tr> | ||
</table> | </table> | ||
<p> </p> | <p> </p> | ||
| − | ---- | + | <!-- End of content --> |
| − | + | {{wiki/ArticleFooter}} | |
| − | |||
Latest revision as of 14:01, 15 March 2015
Imaging the First Lunar Photographer
|
Image Credit: Wes Higgins |
|
Imaging the First Lunar Photographer In 1839. Louis Daguerre took the first photograph of the Moon. It was a lousy shot, showing no features, but inaugurating imaging studies that have culminated (so far) with exquisite images such as this one of Daguerre's namesake crater. (Perhaps if his photo were better he would have gotten a better crater.) Daguerre (diameter 46 km) is a mirror of Fracastoris on the opposite side of Mare Nectaris. Both were formed on the floor of the impact basin and were flooded when later mare lavas engulfed them. Some volcanists, who searched for evidence that lunar craters were volcanoes rather than the result of impact, believed that Daguerre's rim was double in some places - clearly a sign of eruption along parallel curving faults. Also, the darkness visible here along the northern portion of the rim is from pyroclastic (volcanic ash) deposits. So the volcanists' interpretation was that the double rim and the pyroclastics meant that the entire crater had to be volcanic. Wes' high resolution image dispels the notion of a double rim. The extra rim on the left side is actually the rim of a Daguerre-like crater immediately to the west. And the few ridges inside the main rim are probably just normal terraces of an impact crater inner wall. But the pyroclastics are evidence of a real volcanic eruption, probably from small vents at the NNE portion of Daguerre's rim. But volcanic eruptions on the rim of a crater do not mean the crater is volcanic! Three more things of note here. First, the area to the right of Daguerre may be another old, lava-covered crater, but its southern side has peculiar triangular and lozenge-shaped surfaces divided by a though. This seems more like Mars topography than lunar. Second, the area is peppered with small pits that are secondary craters from Theophilus. Third, a peculiar ray, apparently from Madler, crosses the western rim of Deguerre. This has been a busy neighborhood! Technical Details: Related Links: Yesterday's LPOD: H-Alpha Moon Tomorrow's LPOD: A Long, Cold Mare |
|
Author & Editor: |
COMMENTS?
Register, Log in, and join in the comments.
