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Discovery of Meso- to Neoproterozoic magmatism and metamorphism in the eastern Himalaya: Implications for assembly of the Rodinia supercontinent

Abstract:
The Himalayan orogen formed following the Cenozoic India-Asia collision, and contains many exposures of Precambrian rocks that reveal the pre-collisional geological evolution of India and its behavior during the assembly and breakup of the Rodinia supercontinent. Here we present new geochronological and geochemical data for amphibolites and orthogneisses from the eastern Himalayan orogen, which record the first identification of Late Mesoproterozoic arc-related magmatism and Early Neoproterozoic metamorphism in the region. Magmatic zircon cores from amphibolites and orthogneisses yield mean 207Pb/206Pb ages of 1200–1140 Ma, whereas metamorphic zircon rims give mean 206Pb/238U ages of 940–920 Ma. These rocks have fractionated REE patterns, LILE enrichments, and negative Nb, Ta, and Ti anomalies. The amphibolites have high zircon εHf(t) values of + 2.6 to + 11.5 and whole-rock εNd(t) values of −0.80 to + 4.06, and low whole-rock 87Sr/86Sr(i) ratios, while the orthogneisses have low zircon εHf(t) values of −15.1 to −0.4 and whole-rock εNd(t) values of −7.66 to −3.88, and high whole-rock 87Sr/86Sr(i) ratios. These compositions suggest that the amphibolite protoliths were derived from partial melting of depleted mantle, and the orthogneiss protoliths were derived from remelting of more ancient crustal rocks during Mesoproterozoic accretionary orogeny. These records are consistent with Grenvillian tectonothermal events of the Rayner-Eastern Ghats orogen, implying that a huge Meso- to Neoproterozoic accretionary to collisional system operated along the eastern Indian margin during the assembly of Rodinia. These findings also suggest that the Lhasa terrane was situated along the northern Indian margin during the Neoproterozoic, supporting hypotheses that the Lhasa terrane previously drifted away from the Indian continent before they were combined again during the Cenozoic. These new data thus constrain Neoproterozoic plate tectonic reconstructions and paleogeographic models of Rodinia supercontinent formation.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1016/j.precamres.2026.108146

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Earth Sciences
Oxford college:
St Cross College
Role:
Author
ORCID:
0000-0002-6959-0462


More from this funder
Funder identifier:
https://ror.org/04wtq2305
Grant:
DD20221630
More from this funder
Funder identifier:
https://ror.org/02kxqx159
Grant:
2025ZD1004705
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Funder identifier:
https://ror.org/01h0zpd94
Grant:
U2244203


Publisher:
Elsevier
Journal:
Precambrian Research More from this journal
Volume:
441
Article number:
108146
Publication date:
2026-05-14
Acceptance date:
2026-05-09
DOI:
EISSN:
1872-7433
ISSN:
0301-9268


Language:
English
Keywords:
Pubs id:
2428628
Local pid:
pubs:2428628
Source identifiers:
W7161135994
Deposit date:
2026-09-09
ARK identifier:

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