Rotating Moon. Best viewed at 50% speed.
https://www.youtube.com/watch?v=sNUNB6CMnE8
If you know how to put the above video on continuous loop please tell me.
http://lroc.sese.asu.edu/posts/707
A huge payoff from the longevity of the Lunar Reconnaissance Orbiter mission (LRO) is the repeat coverage obtained by the LRO Wide Angle Camera (WAC). What to do? Easy – simply take 36 nearly complete global mosaics (110,000 WAC images) and determine an equation that describes how changes in Sun angle and view angle result in reflectance changes. Next step, for each pixel in those 110,000 WAC images compute the solar angle and the viewpoint angle (using the GLD100 to correct for local slopes), and adjust the measured brightness to common angles everywhere on the Moon. For this mosaic the LRO Team used the 643 nm band, a solar angle 10° from vertical (nearly noon), and a viewing angle straight down. Well, perhaps easy is a bit of an exaggeration!
GLD100 is the global topography model from the LRO.
The mare appear as they do because of their high abundance of iron (iron in minerals such as pyroxene, and iron metal as a product of space weathering), and in many areas titanium (in the mineral ilmenite). Both elements are strongly absorbing in visible wavelengths. Crater rays are generally composed of the same materials upon which they rest, but they have not undergone as much space weathering, yielding a reflectance contrast. Space weathering lowers the reflectance over time, so wait long enough and Tycho’s rays will disappear.
More images at http://lroc.sese.asu.edu/posts
Vikram lander found. http://lroc.sese.asu.edu/posts/1131 The Chandrayaan 2 Vikram lander was targeted for a highland smooth plain about 600 kilometers from the south pole; unfortunately the Indian Space Research Organisation (ISRO) lost contact with their lander shortly before the scheduled touchdown (7 September). Despite the loss, getting that close to the surface was an amazing achievement.