Late Cenozoic tectonics of the northern Los Angeles fault system, California

Citation
H. Tsutsumi et al., Late Cenozoic tectonics of the northern Los Angeles fault system, California, GEOL S AM B, 113(4), 2001, pp. 454-468
Citations number
74
Categorie Soggetti
Earth Sciences
Journal title
GEOLOGICAL SOCIETY OF AMERICA BULLETIN
ISSN journal
00167606 → ACNP
Volume
113
Issue
4
Year of publication
2001
Pages
454 - 468
Database
ISI
SICI code
0016-7606(200104)113:4<454:LCTOTN>2.0.ZU;2-A
Abstract
The northern Los Angeles fault system along the southern range front of the Santa Monica Mountains includes potentially seismogenic faults directly be neath the Los Angeles metropolitan area. For a better assessment of seismic hazards, we mapped late Cenozoic faults and folds in the northern Los Ange les basin using an extensive set of oil-well and surface geologic data. The northern Los Angeles fault system developed through early to late Miocene transrotational and transtensional regimes and a Pliocene and Quaternary tr anspressional regime. The Santa Monica, San Vicente, and Las Cienegas fault s are early to late Miocene normal faults that were later reactivated as re verse faults, suggesting that the orientation of reverse faults is largely controlled by Miocene extensional tectonics rather than by the post-Miocene stress field. Tectonic inversion occurred at the beginning of Pliocene tim e with the reactivation of Miocene normal faults and initiation of reverse faults. Many Pliocene contractile structures became inactive by the middle Pleistocene, and younger deformation is taken up by new active structures, including the West Beverly Hills lineament and an active strand of the Sant a Monica fault. The West Beverly Hills lineament is the northernmost segmen t of the Newport-Inglewood fault zone, which may have propagated northward to the Santa Monica Mountains in Quaternary time. The lineament acts as a s egment boundary for the active left-lateral Santa Monica-Hollywood fault sy stem and bounds the Hollywood basin to the west. Uplift of an oxygen-isotop e substage 5e marine terrace north of the city of Santa Monica and an assum ed dip of >45 degrees for the Santa Monica Mountains thrust fault underlyin g and uplifting the Santa Monica Mountains suggest that an average dip-slip rate for the fault is <1.3 mm/yr, Crustal shortening across the northern L os Angeles fault system accounts for less than a third of the current rate of shortening between the San Gabriel Mountains and Pales Verdes Hills base d on global positioning system observations.