Development of the Indus Fan and its significance for the erosional history of the Western Himalaya and Karakoram

被引:0
|
作者
Clift, PD [1 ]
Shimizu, N
Layne, GD
Blusztajn, JS
Gaedicke, C
Schlüter, HU
Clark, MK
Amjad, S
机构
[1] Woods Hole Oceanog Inst, Dept Geol & Geophys, Woods Hole, MA 02543 USA
[2] Bundesanstalt Geowissensch & Rohstoffe, D-30655 Hannover, Germany
[3] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA
[4] Natl Inst Oceanog, Karachi 75600, Pakistan
关键词
Arabian Sea; Himalaya; Indian Ocean; Indus Fan; isotopes; provenance;
D O I
10.1130/0016-7606(2001)113<1039:DOTIFA>2.0.CO;2
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Correlation of new multichannel seismic profiles across the upper Indus Fan and Murray Ridge with a dated industrial well on the Pakistan shelf demonstrates that similar to 40% of the Indus Fan predates the middle Miocene, and similar to 35% predates uplift of the Murray Ridge (early Miocene, similar to 22 Ma). The Arabian Sea, in addition to the Makran accretionary complex, was therefore an important repository of sediment from the Indus River system during the Paleogene. Channel and levee complexes are most pronounced after the early Miocene, coincident with an increase in sedimentation rates. Middle Eocene sandstones from Deep Sea Drilling Project Site 224 an the Owen Ridge yield K-feldspars whose Pb isotopic composition, measured by in situ ion microprobe methods, indicates an origin in, or north of, the Indus suture zone. This observation requires that India-Asia collision had occurred by this time and that an Indus River system, feeding material from the suture zone into the basin, was active soon after collision. Pleistocene provenance was similar to that during the Eocene, albeit with greater contribution from the Karakoram. A mass balance of the erosional record on land with deposition in the fan and associated basins suggests that only similar to 40% of the Neogene sediment in the fan is derived from the Indian plate.
引用
收藏
页码:1039 / 1051
页数:13
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