Using Venus’ Cratering History to Estimate the Hydrocarbon Production Potential of Buried Terrestrial Impact Structures
Abstract
Herein lies an attempt to determine the economic, and ultimately
scientific, value of buried, petroliferous astroblemes underlying the world’s
continents. First, an estimate of the total number and size of impact events on
Earth since the Cambrian Period is derived using the surface of Venus as an
Earth
analog
. That estimate is then reduced to continental structures based on
statistical analyses of cratering dynamics and physical differences between
Earth and Venus. Using accepted crater scaling parameters, the cumulative
volume of displaced and altered rock within the hypothetical craters is
calculated. Next, an in-depth analysis of the Red Wing Creek structure in
North Dakota, a productive astrobleme nearing the end of its secondary
recovery phase, is performed in order to ascertain the reservoir characteristics
of impacted strata. After comparing the derived parameters to historical
production volumes at Red Wing Creek and two other producing astroblemes,
the values were adjusted and applied to the total displaced volume so that the
original oil in place (OOIP) and expected ultimate recovery (EUR) could be
estimated. The study finds that a conservative estimate for OOIP at currently
undiscovered impact structures is 400 billion barrels, with an EUR of 30
billion barrels.
AAPG Datapages/Search and Discovery Article #90357 ©2019 AAPG Rocky Mountain Section Meeting, Cheyenne, Wyoming, September 15-18, 2019
