Thermal structure and exhumation history of the Lesser Himalaya in central Nepal -: art. no. TC5015

被引:178
作者
Bollinger, L
Avouac, JP
Beyssac, O
Catlos, EJ
Harrison, TM
Grove, M
Goffé, B
Sapkota, S
机构
[1] CEA, Lab Detect & Geophys, F-91680 Bruyeres Le Chatel, France
[2] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[3] Ecole Normale Super, Geol Lab, F-75005 Paris, France
[4] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA
[5] Natl Seism Ctr, Dept Mines & Geol, Kathmandu, Nepal
关键词
Himalaya; thermal structure; underplating; duplex; metamorphism; thermochronology;
D O I
10.1029/2003TC001564
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
[1] The Lesser Himalaya (LH) consists of metasedimentary rocks that have been scrapped off from the underthrusting Indian crust and accreted to the mountain range over the last similar to 20 Myr. It now forms a significant fraction of the Himalayan collisional orogen. We document the kinematics and thermal metamorphism associated with the deformation and exhumation of the LH, combining thermometric and thermochronological methods with structural geology. Peak metamorphic temperatures estimated from Raman spectroscopy of carbonaceous material decrease gradually from 520degrees - 550 degreesC below the Main Central Thrust zone down to less than 330 degreesC. These temperatures describe structurally a 20degrees - 50 degreesC/km inverted apparent gradient. The Ar muscovite ages from LH samples and from the overlying crystalline thrust sheets all indicate the same regular trend; i.e., an increase from about 3 -4 Ma near the front of the high range to about 20 Ma near the leading edge of the thrust sheets, about 80 km to the south. This suggests that the LH has been exhumed jointly with the overlying nappes as a result of overthrusting by about 5 mm/yr. For a convergence rate of about 20 mm/yr, this implies underthrusting of the Indian basement below the Himalaya by about 15 mm/yr. The structure, metamorphic grade and exhumation history of the LH supports the view that, since the mid-Miocene, the Himalayan orogen has essentially grown by underplating, rather than by frontal accretion. This process has resulted from duplexing at a depth close to the brittle-ductile transition zone, by southward migration of a midcrustal ramp along the Main Himalayan Thrust fault, and is estimated to have resulted in a net flux of up to 150 m(2)/yr of LH rocks into the Himalayan orogenic wedge. The steep inverse thermal gradient across the LH is interpreted to have resulted from a combination of underplating and post metamorphic shearing of the underplated units.
引用
收藏
页码:TC50151 / 19
页数:19
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