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The AAPG/Datapages Combined Publications Database

Tulsa Geological Society


Tulsa Geological Society Digest
Vol. 29 (1961), Pages 120-120

Middle Permian Evaporites in Southwestern Oklahoma: Abstract

William E. Ham1


The two thickest outcrop sections of evaporites in the Midcontinent region of the United States are in the Blaine and Cloud Chief formations of southwestern Oklahoma. Each is composed mainly of gypsum at the outcrop and of anhydrite in subsurface.

The earlier sequence is the Blaine, of Late Leonardian or Early Guadalupean age. It has maximum thickness of 250 feet and consists of four principal cycles. Each cycle is a three-fold division beginning with dolomite less than 5 feet thick, continuing upward with white gypsum normally 15-30 feet thick, and ending with reddish-brown shale 10-30 feet thick.

The upper half of the Blaine formation is 90 feet thick and is made up of massive gypsum containing as many as four thin dolomite beds but practically no shales, thus representing a composite of several incomplete normal cycles. Northward in subsurface this evaporite unit grades into nearly pure halite.

Four hundred feet above the Blaine is the thickest single evaporite body in the Midcontinent region. It is in the lower part of the Cloud Chief formation, of probable Late Guadalupean age, and consists of gypsum and anhydrite 120 feet thick with no interbedded shale or dolomite. Extensive core drilling has shown that the Cloud Chief evaporite body is massive and non-cyclic. By Cloud Chief time the position of the evaporite basin had shifted markedly eastward, as it was then situated over the shoreward or clastic facies of the Blaine. The Cloud Chief gypsum also is noteworthy for containing marginal tongues of strontium minerals, chiefly celestite, and for containing in the massive gypsum a few small nodules of the borate mineral probertite.


Acknowledgments and Associated Footnotes

1 Associate Director, Oklahoma Geological Survey

2Presented before International Geological Congress, 1960.

Copyright © 2006 by the Tulsa Geological Society