Publication | Closed Access
Water/rock interactions and the origin of H <sub>2</sub> O in granitic batholiths
625
Citations
75
References
1977
Year
VolcanologyEngineeringWater-rock InteractionGranitic BatholithsEarth ScienceδD ValuesFluid GeochemistryWater/rock InteractionsHigh Temperature GeochemistryGeochronologyCrustal MeltingMagmatismIgneous PetrogenesisGeologyRock PropertiesTectonicsO\ 16Low δ 18Economic GeologyEarth SciencesGeochemistryIgneous PetrologyPetrology
Large meteoric‑hydrothermal convection systems formed in the epizonal zones of batholiths, producing low δ18O feldspars during subsolidus exchange. Isotopic data reveal that granitic batholiths acquire their primary water from lower‑crustal or subducted lithosphere, with δ18O values indicating substantial input from high‑18O metasedimentary or altered volcanic rocks, and low δD values reflecting meteoric‑hydrothermal exchange in epizonal zones.
D\H and 18 O\ 16 O data have now been obtained on a wide variety of granitic batholiths of various ages. The primary δD values of the biotites and hornblendes are remarkably constant at about –50 to –85, identical to the values in regional metamorphic rocks, marine sediments and greeenstones, and most weathering products in temperate climates. Therefore the primary H 2 O in these igneous rocks is probably not ‘juvenile’, but is ultimately derived by dehydration and/or partial melting of the lower crust or subducated lithosphere. Most granitic rocks have δ 18 O = + 7.0 to +10.0, probably indicating significant involvement of high - 18 O metasedimentary or altered volcanic rocks in the melting process; such an origin is required for many other granodiorites and tonaloites that have δ 18 O = + 10 to +13. Gigantic meteoric-hydrothermal convective circulation systems were established in the epizonal portions of all batholiths, locally producing very low δ 18 O values (particularly in feldspars) during subsolidus exchange. Some granitic plutons in such environments also were emplaced as low- 18 O magmas probably formed by melting or assimilation of hydrothermally altered roofrocks. However, the water/rockratios were typically low enough that over wide areas the only evidence for meteoric H 2 O exchange in the batholiths is given by low D/H ratios (δD as low as –180); for example, because of latitudinal isotopic variations in meteoric waters, as one moves from through the Cordilleran batholiths of western North America an increasingly higher proportion of the granitic rocks haves δD values lower than –120. The lowering of δD values commonly correlates
| Year | Citations | |
|---|---|---|
Page 1
Page 1