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1.
Nature ; 543(7643): 44-45, 2017 03 01.
Artigo em Inglês | MEDLINE | ID: mdl-28252060
3.
Science ; 381(6665): 1423-1425, 2023 Sep 29.
Artigo em Inglês | MEDLINE | ID: mdl-37769098

RESUMO

Highlights from the Science family of journals.

4.
5.
Science ; 375(6585): 1140-1142, 2022 Mar 11.
Artigo em Inglês | MEDLINE | ID: mdl-35271313

RESUMO

Highlights from the Science family of journals.

9.
Nature ; 434(7036): 1008-11, 2005 Apr 21.
Artigo em Inglês | MEDLINE | ID: mdl-15846343

RESUMO

Recent convergence between India and Eurasia is commonly assumed to be accommodated mainly along a single fault--the Main Himalayan Thrust (MHT)--which reaches the surface in the Siwalik Hills of southern Nepal. Although this model is consistent with geodetic, geomorphic and microseismic data, an alternative model incorporating slip on more northerly surface faults has been proposed to be consistent with these data as well. Here we present in situ cosmogenic 10Be data indicating a fourfold increase in millennial timescale erosion rates occurring over a distance of less than 2 km in central Nepal, delineating for the first time an active thrust fault nearly 100 km north of the surface expression of the MHT. These data challenge the view that rock uplift gradients in central Nepal reflect only passive transport over a ramp in the MHT. Instead, when combined with previously reported 40Ar-39Ar data, our results indicate persistent exhumation above deep-seated, surface-breaking structures at the foot of the high Himalaya. These results suggest that strong dynamic interactions between climate, erosion and tectonics have maintained a locus of active deformation well to the north of the Himalayan deformation front.

10.
Science ; 374(6568): 704-706, 2021 Nov 05.
Artigo em Inglês | MEDLINE | ID: mdl-34735247

RESUMO

Highlights from the Science family of journals.

11.
Sci Robot ; 2(7)2017 06 21.
Artigo em Inglês | MEDLINE | ID: mdl-33157896

RESUMO

Modern telerobotic technologies offer astronaut scientists real-time presence on planetary surfaces without the risk and cost of putting them all the way there.

13.
Sci Adv ; 6(45)2020 11.
Artigo em Inglês | MEDLINE | ID: mdl-33148656
14.
Sci Adv ; 6(28)2020 Jul.
Artigo em Inglês | MEDLINE | ID: mdl-32937548
15.
Science ; 370(6517): 672-673, 2020 11 06.
Artigo em Inglês | MEDLINE | ID: mdl-33154133
16.
Sci Adv ; 1(1): e1400050, 2015 Feb.
Artigo em Inglês | MEDLINE | ID: mdl-26601128

RESUMO

Quantitative constraints on the ages of melt-forming impact events on the Moon are based primarily on isotope geochronology of returned samples. However, interpreting the results of such studies can often be difficult because the provenance region of any sample returned from the lunar surface may have experienced multiple impact events over the course of billions of years of bombardment. We illustrate this problem with new laser microprobe (40)Ar/(39)Ar data for two Apollo 17 impact melt breccias. Whereas one sample yields a straightforward result, indicating a single melt-forming event at ca. 3.83 Ga, data from the other sample document multiple impact melt-forming events between ca. 3.81 Ga and at least as young as ca. 3.27 Ga. Notably, published zircon U/Pb data indicate the existence of even older melt products in the same sample. The revelation of multiple impact events through (40)Ar/(39)Ar geochronology is likely not to have been possible using standard incremental heating methods alone, demonstrating the complementarity of the laser microprobe technique. Evidence for 3.83 Ga to 3.81 Ga melt components in these samples reinforces emerging interpretations that Apollo 17 impact breccia samples include a significant component of ejecta from the Imbrium basin impact. Collectively, our results underscore the need to quantitatively resolve the ages of different melt generations from multiple samples to improve our current understanding of the lunar impact record, and to establish the absolute ages of important impact structures encountered during future exploration missions in the inner Solar System.

17.
Sci Rep ; 5: 12076, 2015 Jul 15.
Artigo em Inglês | MEDLINE | ID: mdl-26174578

RESUMO

The highest elevation of the Tibetan Plateau, lying 5,700 m above sea level, occurs within the part of the Lhasa block immediately north of the India-Tibet suture zone (Yarlung Zangbo suture zone, YZSZ), being 700 m higher than the maximum elevation of more northern parts of the plateau. Various mechanisms have been proposed to explain this differentially higher topography and the rock uplift that led to it, invoking crustal compression or extension. Here we present the results of structural investigations along the length of the high elevation belt and suture zone, which rather indicate flexural bending of the southern margin of the Lhasa block (Gangdese magmatic belt) and occurrence of an adjacent foreland basin (Kailas Basin), both elements resulting from supra-crustal loading of the Lhasa block by the Zangbo Complex (Indian plate rocks) via the Great Counter Thrust. Hence we interpret the differential elevation of the southern margin of the plateau as due originally to uplift of a forebulge in a retro foreland setting modified by subsequent processes. Identification of this flexural deformation has implications for early evolution of the India-Tibet continental collision zone, implying an initial (Late Oligocene) symmetrical architecture that subsequently transitioned into the present asymmetrical wedge architecture.

18.
Sci Adv ; 5(10): eaaz5011, 2019 10.
Artigo em Inglês | MEDLINE | ID: mdl-31616798
20.
Science ; 356(6341): 918-919, 2017 Jun 02.
Artigo em Inglês | MEDLINE | ID: mdl-28572368
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