Casma Group
The Casma Group (Spanish: Grupo Casma) is a stratigraphic group of Mesozoic-aged sedimentary formations exposed along the coast and within the Cordillera Occidental near Casma, Peru.
The sediments of the Casma Group reflect deposition in two distinct environments of the West Peruvian Basin. Some sediments were deposited near the Casma Volcanic Arc in an intra-cratonic sedimentary basin that was occasionally connected to the ocean. Other sediments were deposited in what was once a continental platform bounded by reefs and with anoxic pockets.[1]
Together with the Morro Solar and Imperial Groups, the Morro Solar Group contains clastic volcanosedimentary material derivative of the Mesozoic Casma Volcanic Arc.[2] The folding of the Casma Group sediments is the result of the Cretaceous Mochica Phase of the Andean orogeny.[2]
The Casma Group include the following lithologies: gypsum, limestone, marl, tuff, lava flows, sandstone and conglomerate.[1]
References
- 1 2 Compare, Dominique; Adline, Ghilaine; Romani, Maurice; Angeles, Carlos (1983). "Contribución al estudio de las formaciones volcánicas y sedimentarias del Grupo Casma en la transversal del río Huara, Cuenca oeste-peruana" (PDF). Bulletin de l'Institut français d'études andines (in Spanish) XII (1–2): 75–89. Retrieved 30 December 2015.
- 1 2 Pfiffner, Adrian O.; Gonzalez, Laura (2013). "Mesozoic–Cenozoic Evolution of the Western Margin of South America: Case Study of the Peruvian Andes". Geoscience 3: 262–310. doi:10.3390/geosciences3020262.