Limited crustal contamination in large igneous province basalts: Sr-Nd-Pb-Os isotope evidence from the Western Ghats, Deccan Traps
• Os-Sr-Nd-Pb isotopic data constrain origin of Deccan basalts. • Small contribution from sub-continental lithospheric mantle sulfides. • Os isotopic data suggest negligible to minor amounts of crustal contamination for most Deccan and Phanerozoic Large Igneous Provinces. • (Very) low degrees of crustal contamination in LIPs related to magma emplacement mechanism and rates. The origin of basalts from the Western Ghats lava sequences of the Deccan large igneous province (LIP) was investigated through combined major and trace element and isotopic analysis. Sr-Nd-Pb isotopic compositions are strongly variable and show a time-related shift from enriched, crustal-like values for the late Cretaceous Kalsubai and Lonavala Subgroup basalts to more depleted mantle-like values for the early Paleogene Wai Subgroup basalts. By contrast, Os isotopic data are relatively uniform from base to top of the Western Ghats (initial 187 Os/ 188 Os i at 66 Ma: 0.12-0.21) and generally similar to those of the present-day Réunion mantle plume. The basalts from the Wai Subgroup Ambenali Formation ( 187 Os/ 188 Os i 0.120) may show a moderate contribution from the sub-continental lithospheric mantle. In general, the combined isotopic and trace element compositions, and 187 Os/ 188 Os i in particular, show that assimilation of the Proterozoic to Archean Indian crust was generally low (<3 wt.% of starting magma) and did not exceed 8 wt.% in any of the studied lavas. Similar results have been previously reported for other Phanerozoic LIPs. Therefore, we suggest that the emplacement of LIPs as short-lived eruptive pulses interrupted by relatively longer hiatus periods possibly hindered effective and prolonged heating of the basement rocks above their solidus temperature. Most likely, this obstacle to crustal contamination was particularly effective for the Wai basalts, which are interlayered with numerous sedimentary or paleosol layers probably formed during periods of volcanic quiescence when the crustal basement may have returned to low sub-solidus temperatures.
Authors
- Andrea Marzoli (ORCID: https://orcid.org/0000-0003-0093-2759)
- Massimo Chiaradia (ORCID: https://orcid.org/0000-0003-4943-2480)
- Andrea Boscaini (ORCID: https://orcid.org/0000-0002-0216-5904)
- David J. Velinsky (ORCID: https://orcid.org/0000-0001-9011-1318)
- Laurie Reisberg (ORCID: https://orcid.org/0000-0002-9551-7752)
- Sara Callegaro (ORCID: https://orcid.org/0000-0003-3932-7935)
- Manfredo Capriolo (ORCID: https://orcid.org/0000-0002-2750-2436)
- T. Becker
- S. Self
- C.M. Meyzen
Institutions
- University of Geneva (CH)
- Centre National de la Recherche Scientifique (FR)
- Planetary Science Institute (US)
- Berkeley Geochronology Center (US)
- University of Padua (IT)
- Université du Québec à Montréal (CA)
- Centre de Recherches Pétrographiques et Géochimiques (FR)
- Drexel University (US)
- University of Birmingham (GB)
- University of Bologna (IT)
- University of California, Berkeley (US)
Publication Details
- Journal
- Earth and Planetary Science Letters
- Published
- 2026-01-14
- DOI
- https://doi.org/10.1016/j.epsl.2026.119847
- Primary Topic
- Geological and Geochemical Analysis
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Science Foundation
- Norges Forskningsråd