NASA NTRS · 19770035475
Selenodetic control network
Abstract
Details for identifying the first 66 reference points of a selenodetic control network are presented. These reference points consist of craters having diameters larger than 8 km and which are therefore detectable on most plates used so far in lunar photogrammetric studies. The distribution of the adopted 211 reference points on Blagg-Mueller (1935) maps is given along with the Blagg-Mueller catalog number of each crater. The correspondence is indicated among the Blagg-Mueller number, the Lunar and Planetary Laboratory Catalog number, and the frame number of Lunar Orbiter IV photographs on which the craters have been studied.
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Moutsoulas, M., Kinsler, D. C.. 1976-07-01. Selenodetic control network. https://ntrs.nasa.gov/citations/19770035475
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