Oblique view facing south of a small, fresh impact crater within the larger daguerre crater, mare nectaris, the moon. The crater is called daguerre 66 in the caption of 16-mm magazine 1196-b on the apollo 14 flight journal video index. This image is similar to figure 111 of apollo over the moon: a view from orbit (nasa sp-362), which has the following caption:
for easier viewing, this picture is oriented with north at the bottom of the page. It shows the striking bilateral symmetry of the rays of a small (2-km diameter) crater in the floor of the large crater daguerre in mare nectaris. Continuous areas and narrow filaments of light-gray ejecta extend from the crater across the dark mare surface through 270°, but are entirely absent in the southern 90° sector. Within the crater, dark material occurs on the southern crater wall while the remaining walls are bright. (the reader may wonder about the material whose reflectivity cannot be observed because it lies in shadow on the east wall of this crater. Until the area is observed under high sun conditions, we are forced to make the simplifying assumption that it is bright because most of the materials visible elsewhere in the walls are bright. ) this crater probably resulted from the impact of a projectile traveling from south to north along an oblique trajectory. Its pattern of ejecta distribution is similar to that of small craters produced by the impact of missiles along oblique trajectories at the white sands missile range, n. Mex. Some observers postulate that the dark material is a talus deposit of mare material that has fallen into the crater. -h. J. M. Another geological explanation is that the unusual pattern may be due to an intrinsic characteristic of the local terrain, probably an abrupt lateral change in the composition of the bedrock within the area that was excavated. F. E. -b. Date: 1972.
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