Difference between revisions of "June 24, 2012"
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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+6 6]<br /> |
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<p><b>Yesterday's LPOD:</b> [[June 23, 2012|Mauve Clouds On the Mare]] </p> | <p><b>Yesterday's LPOD:</b> [[June 23, 2012|Mauve Clouds On the Mare]] </p> |
Revision as of 19:25, 18 August 2018
Is a Half Crater Better Than None?
image from LRO QuickMap
Notice anything unusual about this feature? Assuming it was a crater, half of it is missing. On the upper right is a well defined rim rising
about 2 km above the floor; a circular crater with that rim arc would be about 70 km in diameter. On the opposite side there is no evidence
of a rim, instead there is a mass with textured surface looking very much like the material outside the rim at the top. Note that the 40 km
crater just to the left of Petermann Y is also mostly filled with what looks to be the same material. If this were near the Orientale Basin we
would marvel at how ejecta could be so massive. But this is close (76°N, 90°E) to the North Pole, about 110° of latitude away from Orientale
and about the same in longitude. The rough textured material is thick - 1.5 to 2 km where it fills the half crater. This area is only about 20°
north of the center of the Humboldtianum Basin and the massive material may be from there. This area is just inside the limit of Humboldtianum
ejecta mapped by Baerbel Lucchitta in 1978. The floor of the half crater is almost completed surrounded by rilles/fractures like a floor-fractured crater, and an adjoining crater to its left has smooth, mare-like material on its floor - it does not look like an impact melt pond.
Tomorrow we will see other deposits that make the Humboldtianum origin less likely.
Chuck Wood
Related Links
Rükl plate 6
Yesterday's LPOD: Mauve Clouds On the Mare
Tomorrow's LPOD: Mini-Schiller
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