Difference between revisions of "October 26, 2011"
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<em>LRO NAC mosaic from [http://target.lroc.asu.edu/da/qmap.html QuickMap]</em><br /> | <em>LRO NAC mosaic from [http://target.lroc.asu.edu/da/qmap.html QuickMap]</em><br /> | ||
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| − | Do you recognize this famous 3.5 km wide crater? It was first noticed as being unusual in the early 1670s when observers didn't readily detect such small craters. Being so small it could only be famous for being bright, and this image shows that it does have a very sharp rim and appears quite young. You may notice something else about this image - the shadow in the middle doesn't belong there - apparently the automatic (I assume) compositing of Narrow Angle Camera images to make the QuickMap mosaic included one with a low Sun angle. But back to the actual crater, not the depicted one - have you figured it out yet? It is Cassini's Bright Spot on the floor of Deslandres. A peculiar aspect of CBS is that the bright ejecta is all to the east of the crater - see the upper right corner of [http://lpod. | + | Do you recognize this famous 3.5 km wide crater? It was first noticed as being unusual in the early 1670s when observers didn't readily detect such small craters. Being so small it could only be famous for being bright, and this image shows that it does have a very sharp rim and appears quite young. You may notice something else about this image - the shadow in the middle doesn't belong there - apparently the automatic (I assume) compositing of Narrow Angle Camera images to make the QuickMap mosaic included one with a low Sun angle. But back to the actual crater, not the depicted one - have you figured it out yet? It is Cassini's Bright Spot on the floor of Deslandres. A peculiar aspect of CBS is that the bright ejecta is all to the east of the crater - see the upper right corner of [http://www2.lpod.org/wiki/August_30,_2008 this] Minsk color image. Look closely at the Minsk view and you will see that the bright rays make a Vee opening to the east but other ray material goes in other directions. [http://www.mapaplanet.org/explorer-bin/explorer.cgi?map=Moon&layers=moon_clementine_multi&west=352.77&south=-34.44&east=358.4&north=-31.62&center_lat=&center=355.585&defaultcenter=on&grid=none&stretch=none&projection=SIMP&advoption=NO&info=NO&resolution=128 Here] is a confirmatory Clementine view. The Vee-shaped pattern suggests an oblique impact (and the elongated 4.2 km east- west diameter hints at that) but rays open up in the downrange direction for an oblique impact and the bright rays here are in the wrong direction. Perhaps there is more happening here. The LRO image shows very bright material exposed in the eastern wall of CBS, and more to the southwest where the wall isn't covered by later gray talus. Is it possible that the CBS crater impacted into a geologic boundary with very bright material only on the east side? But why aren't there similar [http://www.mapaplanet.org/explorer-bin/explorer.cgi?map=Moon&layers=moon_clementine_multi&west=352.77&south=-34.44&east=358.4&north=-31.62&center_lat=&center=355.585&defaultcenter=on&grid=none&stretch=none&projection=SIMP&advoption=NO&info=NO&resolution=128 length] gray rays? This mystery isn't solved yet. <br /> |
<br /> | <br /> | ||
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | ||
Latest revision as of 08:35, 28 October 2018
Zone of Avoidance Rays
LRO NAC mosaic from QuickMap
Do you recognize this famous 3.5 km wide crater? It was first noticed as being unusual in the early 1670s when observers didn't readily detect such small craters. Being so small it could only be famous for being bright, and this image shows that it does have a very sharp rim and appears quite young. You may notice something else about this image - the shadow in the middle doesn't belong there - apparently the automatic (I assume) compositing of Narrow Angle Camera images to make the QuickMap mosaic included one with a low Sun angle. But back to the actual crater, not the depicted one - have you figured it out yet? It is Cassini's Bright Spot on the floor of Deslandres. A peculiar aspect of CBS is that the bright ejecta is all to the east of the crater - see the upper right corner of this Minsk color image. Look closely at the Minsk view and you will see that the bright rays make a Vee opening to the east but other ray material goes in other directions. Here is a confirmatory Clementine view. The Vee-shaped pattern suggests an oblique impact (and the elongated 4.2 km east- west diameter hints at that) but rays open up in the downrange direction for an oblique impact and the bright rays here are in the wrong direction. Perhaps there is more happening here. The LRO image shows very bright material exposed in the eastern wall of CBS, and more to the southwest where the wall isn't covered by later gray talus. Is it possible that the CBS crater impacted into a geologic boundary with very bright material only on the east side? But why aren't there similar length gray rays? This mystery isn't solved yet.
Chuck Wood
Related Links
Rükl plate 65
Yesterday's LPOD: Big & Little
Tomorrow's LPOD: Mare Exemplum
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