Difference between revisions of "May 19, 2008"
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| − | (1) In answer to the first question: it lacks the clarity of Jérôme's photo, but the shadow cast by the scarp in Hayn A at a lower sun angle is visible in [http://www.lpi.usra.edu/resources/cla/info/a1/ Plate A1] of the <em>[ | + | (1) In answer to the first question: it lacks the clarity of Jérôme's photo, but the shadow cast by the scarp in Hayn A at a lower sun angle is visible in [http://www.lpi.usra.edu/resources/cla/info/a1/ Plate A1] of the <em>[https://the-moon.us/wiki/Consolidated_Lunar_Atlas Consolidated Lunar Atlas]</em>. <!-- ws:start:WikiTextUserlinkRule:00:[[user:JimMosher]] --><span class="membersnap">- [http://www.wikispaces.com/user/view/JimMosher http://www.wikispaces.com/user/pic/JimMosher-lg.jpg] [http://www.wikispaces.com/user/view/JimMosher JimMosher]</span><!-- ws:end:WikiTextUserlinkRule:00 --><br /> |
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Latest revision as of 18:53, 13 October 2018
Edge World
image by Jérôme Grenier
The central peaks of 198 km wide Belkovich are right on the 90°E meridian, and here we can see a little beyond to the far rim of the giant crater. Belkovich A is a broad, smooth-floored crater with the simple crater B inside it. Hayn is a fresh crater with central peaks. Here you can see a characteristic of peaks - they are much lower (almost always) than the walls of their craters. The crater Hayn A is unusual for having a curved Humboldtianum Basin?
Chuck Wood
Technical Details
11 May 2008. Orion Optics (UK) OMC 12" + barlow 2x + red filter + Dmk31AF03 camera; mosaic of six views.
Related Links
Rükl plates 6 & 7
Jérôme's website
Yesterday's LPOD: Unified Lunar Data Tool
Tomorrow's LPOD: Farside 50 - Almost
COMMENTS
(1) In answer to the first question: it lacks the clarity of Jérôme's photo, but the shadow cast by the scarp in Hayn A at a lower sun angle is visible in Plate A1 of the Consolidated Lunar Atlas. - 
JimMosher
COMMENTS?
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