IWLOP #056 - Dorsum von Cotta & Dorsum Buckland
Prominent wrinkle ridges at the southeastern edge of Mare Serenitatis caused by subsidence.
Location: 24.0 N 12.0 E Origin: Tectonic Size: 220 km (Dorsum von Cotta), 159 km (Dorsum Buckland) Rukl: 23 Type: Wrinkle Ridges (WR)
Objects: Dorsum von Cotta, Dorsum Buckland, Sulpicious Galla, Menelaus, Dorsa Owen, Dorsa Gast, Rimae Menelaus
Others Identified : Bobillier, Linné, Tacquet
Location: Home R1: Sulpicious Gallus was located on the SW shore of Mare Serenitatis. Dorsum Buckland and Dorsum von Cotta were located north of the crater on the mare floor. C1: The shadows of Dorsa Owen and Dorsa Gast on the west shore of Mare Serenitatis were barely visible between the shore and Dorsum von Cotta. Rimae Menelaus could just be seen - Menelaus to the east and Tacquet in the west. Rimae Sulpicius Gallus not seen in this observation session. Note: Linné at top of Dorsa von Cotta appeared as a white circular fuzz; could not see the crater. |