Skip Links

USGS - science for a changing world

Water-Resources Investigations Report 84-4314

Chemical and Isotopic Characteristics of Brines from Three Oil- and Gas-Producing Sandstones in Eastern Ohio, with Applications to the Geochemical Tracing of Brine Sources

By Kevin J. Breen, Clifford G. Angelo, Robert W. Masters, and Alan C. Sedam

Thumbnail of and link to report PDF (3.1 MB)Abstract

Chemical and isotopic characteristics of selected inorganic constituents are reported for brines from the Berea Sandstone of Mississippian age, the "Clinton" sandstone (drillers term) in the Albion Sandstone of Silurian age, and the Rose Run sandstone (informal term) in the equivalent of the Knox Dolomite of Cambrian and Ordovician age in 24 counties in eastern Ohio.

Ionic concentrations of dissolved constituents in brine from the three sandstones generally fall in the following ranges: (in millimoles per kilogram of brine): Na, Cl > 1,000; 100 > Ca, Mg <1,000; 1 > K, Br, Sr, Li, Fe, SO4 <100; Mn, Zn, Al, I, HCO3, SiO2 <1. Mean ionic concentrations of Ca, Mg, Na, Cl, K, S04, and Br, and mean values of density and dissolved solids are significantly different at the 95-percent confidence level in each sandstone. Only potassium has a unique concentration range in each sandstone (millimoles per kilogram): 0.3 - 12 (Berea), 13 - 57 ("Clinton"), and 81 - 92 (Rose Run).

For applications involving brine contamination, selected concentration ratios are identified as potential indicators for geochemical tracing of brines having some history of dilution. The K:Na ratios work best for identifying the source sandstone of an unidentified brine. These ranges are K:Na, 0.0002 - 0.0185 (Berea); 0.0073 - 0.0238 ("Clinton"); 0.0230 - 0.0462 (Rose Run). Other constituent ratios may prove useful for differentiating one brine from the other two. "Clinton" and Rose Run brines have no statistical difference in mean values for Ca:Mg, Na:Ca, Na:Cl, Mg:K, Ca:K, Cl:Ca, Mg:Br, and Na:Br. These ratios, in combination with K:Br and Cl:Br, may be used to identify Berea brines.

With respect to isotopic characteristics of hydrogen, oxygen, and sulfate sulfur, a moderate range of δD (-48.0 to -13.5 permil) and δ18O (-5.45 to -1.25 permil) indicate a meteoric water origin for the water matrix in Ohio brines. δD and δ18O values are not useful for differentiating brines from the three formations. The δ34S (SO42-) values for Ohio brines range between +4.6 to +28.4 permil. The heaviest sulfate sulfur is in brine from the Cambrian and Ordovician Rose Run sandstone. A single Berea brine sample was determined to have the lightest δ34S (SO42-) value. "Clinton" brines have δ34S (SO42-) intermediate between those of the Rose Run and Berea sandstones. Sulfur isotopes may have utility for differentiating the isotopically heavy sulfate found in brines from the isotopically light sulfate found in oxidizing ground water.

First posted December 10, 2010

Revised September 18, 2013

For additional information contact:
Director, Ohio Water Science Center
U.S. Geological Survey
6480 Doubletree Avenue
Columbus, Ohio 43229-1111
http://oh.water.usgs.gov/

Part or all of this report is presented in Portable Document Format (PDF); the latest version of Adobe Reader or similar software is required to view it. Download the latest version of Adobe Reader, free of charge.


Suggested citation:

Breen, K.J., Angelo, C.G., Masters, R.W., and Sedam, A.C., 1985, Chemical and isotopic characteristics of brines from three oil- and gas-producing sandstones in eastern Ohio, with applications to the geochemical tracing of brine sources (ver. 1.1, September 18, 2013): U.S. Geological Survey Water-Resources Investigations Report 84–4314, 58 p.



Contents

Abstract

Introduction

Chemical characteristics of brines

Isotopic characteristics

Summary

Conclusions

Selected references


Accessibility FOIA Privacy Policies and Notices

USA.gov logo U.S. Department of the Interior | U.S. Geological Survey
URL: https://pubs.usgs.gov/wri/1984/4314/
Page Contact Information: Contact USGS
Page Last Modified: Wednesday, December 07, 2016, 01:38:47 PM