Journal article
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
Actions
Access Document
- Files:
-
-
(Preview, Accepted manuscript, pdf, 192.7KB, Terms of use)
-
- Publisher copy:
- 10.1016/j.precamres.2026.108146
Authors
+ China Geological Survey
More from this funder
- Funder identifier:
- https://ror.org/04wtq2305
- Grant:
- DD20221630
+ Ministry of Natural Resources
More from this funder
- Funder identifier:
- https://ror.org/02kxqx159
- Grant:
- 2025ZD1004705
+ National Natural Science Foundation of China
More from this funder
- 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:
Terms of use
- Copyright holder:
- Elsevier B.V.
- Copyright date:
- 2026
- Rights statement:
- © 2026 Elsevier B.V. All rights are reserved, including those for text and data mining, AI training, and similar technologies.
- Notes:
- The author accepted manuscript (AAM) of this paper has been made available under the University of Oxford's Open Access Publications Policy, and a CC BY public copyright licence has been applied.
- Licence:
- CC Attribution (CC BY)
If you are the owner of this record, you can report an update to it here: Report update to this record