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Tectonic stability of the San Luis Hills, Northern Rio Grande Rift, Colorado: Evidence from paleomagnetic measurements
Author(s) -
Brown Laurie L.,
Golombek Matthew P.
Publication year - 1997
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/97gl00127
Subject(s) - geology , paleomagnetism , rift , clockwise , structural basin , paleontology , horst , neogene , tectonics , seismology , geomorphology , fold (higher order function) , mechanical engineering , engineering
The San Luis Basin is the largest of four tilted, fault bounded Neogene basins of the northern Rio Grande rift in New Mexico and Colorado. It formed during the second of two episodes of extension beginning in middle Oligocene and extending to the present. The San Luis Hills are an intrarift horst of Oligocene intermediate and basalt rocks preserved in the middle of the San Luis Basin. Previous paleomagnetic and structural studies in the Espanola Basin to the south indicate counterclockwise rotation of that region during the most recent extension. Paleomagnetic samples from the two exposed formations in the San Luis Hills yield a mean direction of inclination=55.6° and declination=347.2° (α 95 =6.8°, N=23) that is coincident with the expected Oligocene direction for North America. These rocks show no indication of rotation or severe tilting during rift extension.