That is a very similar book which has images and a chart for each lunar region. If you are looking for a moon atlas book, also have a look at The Clementine Moon Atlas. Melted ejecta material lies radially around the outside of the crater. The Cambridge Photographic Moon Atlas is a great moon atlas and very up to date with each image looking very impressive.
40 km, 16.5°S, 27.2°W) has been practically completely submerged by lava, only a few individual peaks stick up above the surface of the lava.Ī very conspicuous crater, 60 km in diameter, with terraced inner crater walls and a central mountain with multiple peaks. The former crater wall of Lubiniezky E (c. Northwest of Lubiniezky lie the two craters Lubiniezky A and E. The maximum difference in height between the crater's wall and the floor amounts to just 770 m. The southeastern crater wall is open to the lava surface of Mare Nubium. Mare Nubium offers a multitude of interesting surface features for both visual and photographic observation.Īn almost completely lava-filled crater, 44 km in diameter, similar to Keis, lying northwest of Bullialdus. It has a diameter of roughly 750 km and the lava covers an area of about 250 000 km 2. It is possibly part of the enormous lava flow to which Mare Cognitum, Mare Insularum and parts of Oceanus Procellarum belong. Mare Nubium (‘Sea of Clouds’) is irregular, roughly round in shape, with no distinct boundaries anywhere, such as those found with other maria, typically in the form of sections of wall.
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