Difference between revisions of "May 11, 2011"
| Line 3: | Line 3: | ||
<!-- ws:start:WikiTextHeadingRule:0:<h1> --> | <!-- ws:start:WikiTextHeadingRule:0:<h1> --> | ||
<!-- ws:start:WikiTextLocalImageRule:6:<img src="/file/view/LPOD-Aug29-08.jpg/36352959/LPOD-Aug29-08.jpg" alt="" title="" /> -->[[File:LPOD-Aug29-08.jpg|LPOD-Aug29-08.jpg]]<!-- ws:end:WikiTextLocalImageRule:6 --><br /> | <!-- ws:start:WikiTextLocalImageRule:6:<img src="/file/view/LPOD-Aug29-08.jpg/36352959/LPOD-Aug29-08.jpg" alt="" title="" /> -->[[File:LPOD-Aug29-08.jpg|LPOD-Aug29-08.jpg]]<!-- ws:end:WikiTextLocalImageRule:6 --><br /> | ||
| − | <em>image by [mailto:starman2@allegiance.tv | + | <em>image by [mailto:starman2@allegiance.tv Wes Higgins]</em><br /> |
<br /> | <br /> | ||
| − | Just below Tycho's eastern rim crest (at 2 o'clock and 4 o'clock positions) are smooth ponds of impact melt. Wes' remarkable image also shows that secondaries are concentrated on the east side of the crater, and a high Sun [http://www.lpod.org/?m=20060417 | + | Just below Tycho's eastern rim crest (at 2 o'clock and 4 o'clock positions) are smooth ponds of impact melt. Wes' remarkable image also shows that secondaries are concentrated on the east side of the crater, and a high Sun [http://www.lpod.org/?m=20060417 view] demonstrates that there are fewer rays to the west. Tycho was formed by an oblique impact, with the projectile coming from the west. The forward momentum carried ejecta debris to the east, raking the surface with small impacts. It wouldn't have been a good place to be 109 my ago. <br /> |
<br /> | <br /> | ||
| − | <em>[mailto:tychocrater@yahoo.com | + | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> |
<em>This is a repeat of a glorious LPOD from [http://lpod.wikispaces.com/August+29%2C+2008 Aug 29, 2008.]</em><br /> | <em>This is a repeat of a glorious LPOD from [http://lpod.wikispaces.com/August+29%2C+2008 Aug 29, 2008.]</em><br /> | ||
<br /> | <br /> | ||
| Line 15: | Line 15: | ||
<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
Rükl plate 64<br /> | Rükl plate 64<br /> | ||
| − | Entire [http://higginsandsons.com/astro/images/Tycho-08-23-08.jpg | + | Entire [http://higginsandsons.com/astro/images/Tycho-08-23-08.jpg frame]<br /> |
<br /> | <br /> | ||
<hr /> | <hr /> | ||
Revision as of 17:34, 11 January 2015
Ballistic Rake
image by Wes Higgins
Just below Tycho's eastern rim crest (at 2 o'clock and 4 o'clock positions) are smooth ponds of impact melt. Wes' remarkable image also shows that secondaries are concentrated on the east side of the crater, and a high Sun view demonstrates that there are fewer rays to the west. Tycho was formed by an oblique impact, with the projectile coming from the west. The forward momentum carried ejecta debris to the east, raking the surface with small impacts. It wouldn't have been a good place to be 109 my ago.
Chuck Wood
This is a repeat of a glorious LPOD from Aug 29, 2008.
Technical Details
08/23/08, 11:41:27 UT. 18" Reflector, Infinity 2-1m camera, MAP 150X64, stack of 498 frames .
Related Links
Rükl plate 64
Entire frame
