Difference between revisions of "May 21, 2011"
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=Ignoring the Heroes= | =Ignoring the Heroes= | ||
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<em>image by [mailto:dpeach_78@yahoo.co.uk Damian Peach]</em><br /> | <em>image by [mailto:dpeach_78@yahoo.co.uk Damian Peach]</em><br /> | ||
<br /> | <br /> | ||
| − | Did you know Hercules G - the crater on the lava-covered floor of Hercules - was a banded crater? | + | Did you know Hercules G - the crater on the lava-covered floor of Hercules - was a banded crater? |
| − | I didn't either until I saw Damian's great image. Being banded is not exceptional, and looking at | + | I didn't either until I saw Damian's great image. Being banded is not exceptional, and looking at |
| − | earlier images I found that it was captured previously in a wonderful high Sun [http://lpod.org/coppermine/displayimage.php?pos=-3902 view], but I never | + | earlier images I found that it was captured previously in a wonderful high Sun [http://lpod.org/coppermine/displayimage.php?pos=-3902 view], but I never |
| − | noticed it before. The rim of G seems low just where the dark band reaches it, and if you look | + | noticed it before. The rim of G seems low just where the dark band reaches it, and if you look carefully (or take the image into Photoshop and jack up the brightness) you will see that the bright band |
| − | + | of ejecta surrounding the crater is widest towards the north. Enlarge the high-Sun LRO [http://target.lroc.asu.edu/da/qmap.html mosaic] and | |
| − | of ejecta surrounding the crater is widest towards the north. Enlarge the high-Sun LRO [http://target.lroc.asu.edu/da/qmap.html mosaic] and | + | you will see that the bright area corresponds exactly to the distribution of G's secondary craters. |
| − | you will see that the bright area corresponds exactly to the distribution of G's secondary craters. | + | I suppose that G formed as an oblique impact. The two craters on the walls of Hercules were probably |
| − | I suppose that G formed as an oblique impact. The two craters on the walls of Hercules were probably | + | standard near-vertical impacts, but because they occurred on inward-sloping walls the craters were |
| − | standard near-vertical impacts, but because they occurred on inward-sloping walls the craters were | + | elongated in the downhill direction. Finally, notice Hercules D, the fresh, small-floored crater to the |
| − | elongated in the downhill direction. Finally, notice Hercules D, the fresh, small-floored crater to the | + | right of Hercules. It has a bright, round protuberance high on its north wall. The Clementine [http://www.mapaplanet.org/explorer-bin/explorer.cgi?map=Moon&layers=moon_clementine_base_v2&west=39.06&south=44.44&east=40.47&north=45.15&center_lat=&center=39.765&defaultcenter=on&grid=none&stretch=none&projection=SIMP&r=1&g=1&b=1&advoption=NO&info=NO&resolution=512&scale=0.11845&imageTopX=-42582.9869173467&imageTopY=1379653.2409451902 view] is |
| − | right of Hercules. It has a bright, round protuberance high on its north wall. The Clementine [http://www.mapaplanet.org/explorer-bin/explorer.cgi?map=Moon&layers=moon_clementine_base_v2&west=39.06&south=44.44&east=40.47&north=45.15&center_lat=&center=39.765&defaultcenter=on&grid=none&stretch=none&projection=SIMP&r=1&g=1&b=1&advoption=NO&info=NO&resolution=512&scale=0.11845&imageTopX=-42582.9869173467&imageTopY=1379653.2409451902 view] is | + | not as dramatic as Damian's, but suggests the bright feature is a huge outcrop of the existing country |
| − | not as dramatic as Damian's, but suggests the bright feature is a huge outcrop of the existing country | + | rock exposed by the excavation of the crater. |
| − | rock exposed by the excavation of the crater.<br /> | + | <br /> |
<br /> | <br /> | ||
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | ||
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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
| − | Rükl plate [ | + | Rükl plate [https://the-moon.us/wiki/R%C3%BCkl_14 14]<br /> |
Damian's [http://www.damianpeach.com/ website]<br /> | Damian's [http://www.damianpeach.com/ website]<br /> | ||
<br /> | <br /> | ||
<hr /> | <hr /> | ||
| + | <p><b>Yesterday's LPOD:</b> [[May 20, 2011|Page One of a Lunar Alphabet Book]] </p> | ||
| + | <p><b>Tomorrow's LPOD:</b> [[May 22, 2011|Our Daily Moon]] </p> | ||
| + | <!-- End of content --> | ||
| + | {{wiki/ArticleFooter}} | ||
Latest revision as of 18:53, 13 October 2018
Ignoring the Heroes
image by Damian Peach
Did you know Hercules G - the crater on the lava-covered floor of Hercules - was a banded crater?
I didn't either until I saw Damian's great image. Being banded is not exceptional, and looking at
earlier images I found that it was captured previously in a wonderful high Sun view, but I never
noticed it before. The rim of G seems low just where the dark band reaches it, and if you look carefully (or take the image into Photoshop and jack up the brightness) you will see that the bright band
of ejecta surrounding the crater is widest towards the north. Enlarge the high-Sun LRO mosaic and
you will see that the bright area corresponds exactly to the distribution of G's secondary craters.
I suppose that G formed as an oblique impact. The two craters on the walls of Hercules were probably
standard near-vertical impacts, but because they occurred on inward-sloping walls the craters were
elongated in the downhill direction. Finally, notice Hercules D, the fresh, small-floored crater to the
right of Hercules. It has a bright, round protuberance high on its north wall. The Clementine view is
not as dramatic as Damian's, but suggests the bright feature is a huge outcrop of the existing country
rock exposed by the excavation of the crater.
Chuck Wood
Note: Oh yes, for Danny, there is a small bright rayed, oblique impact crater above Atlas.
Technical Details
May 10, 2011, 19:44 UT. C14.
Related Links
Rükl plate 14
Damian's website
Yesterday's LPOD: Page One of a Lunar Alphabet Book
Tomorrow's LPOD: Our Daily Moon
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