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Abstract

AAPG Bulletin, V. 96, No. 10 (October 2012), P. 17851811.

Copyright copy2012. The American Association of Petroleum Geologists. All rights reserved.

DOI:10.1306/03161211093

Determining the source and genetic fingerprint of natural gases using noble Previous HitgasNext Hit geochemistry: A northern Appalachian Basin case study

Andrew G. Hunt,1 Thomas H. Darrah,2 Robert J. Poreda3

1Department of Earth and Environmental Sciences, 227 Hutchison Hall, University of Rochester, Rochester, New York; present address: U.S. Geological Survey, Noble Previous HitGasNext Hit Laboratory, MS 963, Denver, Colorado; [email protected]
2Department of Earth and Environmental Sciences, 227 Hutchison Hall, University of Rochester, Rochester, New York; present address: Division of Earth and Ocean Sciences, Nicholas School of the Environment, Duke University, Durham, North Carolina; [email protected]
3Department of Earth and Environmental Sciences, 227 Hutchison Hall, University of Rochester, Rochester, New York; [email protected]

ABSTRACT

Silurian and Devonian natural Previous HitgasNext Hit reservoirs present within New York state represent an example of unconventional Previous HitgasNext Hit accumulations within the northern Appalachian Basin. These unconventional energy resources, previously thought to be noneconomically viable, have come into play following advances in drilling (i.e., horizontal drilling) and extraction (i.e., hydraulic fracturing) capabilities. Therefore, efforts to understand these and other domestic and global natural Previous HitgasNext Hit reserves have recently increased. The suspicion of fugitive mass migration issues within current Appalachian production fields has catalyzed the need to develop a greater understanding of the genetic grouping (source) and migrational history of natural gases in this area. We introduce new noble Previous HitgasNext Hit data in the context of published hydrocarbon carbon (C1,C2+) (delta13C) data to explore the genesis of thermogenic gases in the Appalachian Basin. This study includes natural gases from two distinct genetic groups: group 1, Upper Devonian (Marcellus shale and Canadaway Group) gases generated in situ, characterized by early mature (Delta13C[C1 minus C2][delta13C1minusdelta13C2]: lt–9permil), isotopically light methane, with low (4He) (average, 1 times 10minus3 cc/cc) elevated 4He/40Arast and 21Neast/40Arast (where the asterisk denotes excess radiogenic or nucleogenic production beyond the atmospheric ratio), and a variable, atmospherically (air-saturated–water) derived noble Previous HitgasNext Hit component; and group 2, a migratory natural Previous HitgasNext Hit that emanated from Lower Ordovician source rocks (i.e., most likely, Middle Ordovician Trenton or Black River group) that is currently hosted primarily in Lower Silurian sands (i.e., Medina or Clinton group) characterized by isotopically heavy, mature methane (Delta13C[C1 – C2] [delta13C1minusdelta13C2]: gt3permil), with high (4He) (average, 1.85 times 10minus3 cc/cc) 4He/40Arast and 21Neast/40Arast near crustal production levels and elevated crustal noble Previous HitgasNext Hit content (enriched 4He, 21Neast, 40Arast). Because the release of each crustal noble Previous HitgasTop (i.e., He, Ne, Ar) from mineral grains in the shale matrix is regulated by temperature, natural gases obtain and retain a record of the thermal conditions of the source rock. Therefore, noble gases constitute a valuable technique for distinguishing the genetic source and post-genetic processes of natural gases.

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