Difference between revisions of "October 29, 2010"
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<em>Apollo 16 image AS16-121-19449 from [http://images.jsc.nasa.gov/luceneweb/caption_direct.jsp?photoId=AS16-121-19449 JSC Digital Image Collection]</em><br /> | <em>Apollo 16 image AS16-121-19449 from [http://images.jsc.nasa.gov/luceneweb/caption_direct.jsp?photoId=AS16-121-19449 JSC Digital Image Collection]</em><br /> | ||
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| + | <td><!-- ws:start:WikiTextHeadingRule:3:<h3> --><h3 id="toc1"><!-- ws:end:WikiTextHeadingRule:3 -->COMMENTS?</h3> | ||
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===COMMENTS?=== | ===COMMENTS?=== | ||
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Revision as of 21:13, 2 January 2015
Eastern Rays
Apollo 16 image AS16-121-19449 from JSC Digital Image Collection
I love views from unfamiliar perspectives because they force me to look freshly at the areas shown. This image
taken by Apollo 16 astronauts doesn't disappoint. As the astronauts flew over the eastern limb they took this
photo looking across Mare Fecunditatis to Mare Nectaris and the bright lunar highlands beyond. High solar
illumination (and unsharp mask in Photoshop!) highlighted the strong albedo contrasts of dark maria material and
bright crater rays. The crater Langrenus is at the bottom of the image (mouse over) with its grayish radiating rays.
To the south (left) is the 33 km wide crater Petavius B, whose Proclus-like vee-shaped ray pattern demonstrates
was formed by an oblique impact. On the right side of the image is the familiar pair Messier and Pickering (oops -
that's an old designation, the crater with the parallel railway track-like rays is now called Messier A). Notice that
you can also see the butterfly wing rays extending out from Messier itself. These rays, perpendicular to the Mes-
sier A ones, are harder to see, but are characteristic of a very low angle oblique impact. Back to the left half of
the image you can see at least four sets of rays that converge outside the frame on one or the other of the two
amazingly bright (and small) ray craters, Stevinus A and Furnerius A. Another bright ray swath comes eastward
from Rosse in the middle of Nectaris. This particular ray is peculiar because it so large. Some people have sug-
gested that it is actually a ray from Tycho. Other rays here appear to be orphans. Two roughly parallel rays passing
near McClure and Crosier have no obvious source crater, as is true for a long ray passing perpendicular to a line
joining Langrenus and Messier. Looking at the ray-crossed surfaces of Fecunditatis and Nectaris makes it easy to
understand how dark mare material gets lightened over time. Some mare deposits have been completely veneered
by rays and other ejecta so that we can only detect them by small dark halo craters that excavate underlying dark
mare. Such slightly buried mare are called cryptomare.
Chuck Wood
Technical Details
This is a rerun of a LPOD classic from April 16, 2004.
Related Links
Rükl plate 48
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