MbrlCatalogueTitleDetail

Do you wish to reserve the book?
Radiogenic Heating as the Thermal Driver of Himalayan Crustal Heating During Prolonged Thickening
Radiogenic Heating as the Thermal Driver of Himalayan Crustal Heating During Prolonged Thickening
Hey, we have placed the reservation for you!
Hey, we have placed the reservation for you!
By the way, why not check out events that you can attend while you pick your title.
You are currently in the queue to collect this book. You will be notified once it is your turn to collect the book.
Oops! Something went wrong.
Oops! Something went wrong.
Looks like we were not able to place the reservation. Kindly try again later.
Are you sure you want to remove the book from the shelf?
Radiogenic Heating as the Thermal Driver of Himalayan Crustal Heating During Prolonged Thickening
Oops! Something went wrong.
Oops! Something went wrong.
While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Title added to your shelf!
Title added to your shelf!
View what I already have on My Shelf.
Oops! Something went wrong.
Oops! Something went wrong.
While trying to add the title to your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
Radiogenic Heating as the Thermal Driver of Himalayan Crustal Heating During Prolonged Thickening
Radiogenic Heating as the Thermal Driver of Himalayan Crustal Heating During Prolonged Thickening

Please be aware that the book you have requested cannot be checked out. If you would like to checkout this book, you can reserve another copy
How would you like to get it?
We have requested the book for you! Sorry the robot delivery is not available at the moment
We have requested the book for you!
We have requested the book for you!
Your request is successful and it will be processed during the Library working hours. Please check the status of your request in My Requests.
Oops! Something went wrong.
Oops! Something went wrong.
Looks like we were not able to place your request. Kindly try again later.
Radiogenic Heating as the Thermal Driver of Himalayan Crustal Heating During Prolonged Thickening
Radiogenic Heating as the Thermal Driver of Himalayan Crustal Heating During Prolonged Thickening
Journal Article

Radiogenic Heating as the Thermal Driver of Himalayan Crustal Heating During Prolonged Thickening

2025
Request Book From Autostore and Choose the Collection Method
Overview
The thermal evolution of the crust during continental collision evolves from cold to hot with time, which impacts crustal reworking and differentiation. However, it remains elusive as to the mechanism driving the crust to be hot during the protracted collision. Here, we describe crust thermal evolution via detailed petrographic and geochronological analyses, and P−T calculations on different metamorphic rocks from east‐central Himalaya, which record a wide range of P−T conditions and ages from the early to the late collision stage. The Eocene (ca. 44 Ma) metamorphism, represented by the Kangmar garnet amphibolite, exhibits P = ∼12 kbar, T = 670°−690°C, and a geothermal gradient of 17.0°–17.4°C/km. Rocks in the Tsona area yield metamorphic ages of 39–36 Ma and peak P−T conditions of 13.0–14.5 kbar and 760°−770°C (16.0°−17.9°C/km). Mafic granulites recorded variable peak conditions of 18–25 kbar and 720°−870°C (8.72°−14.6°C/km) and were overprinted by granulite‐facies metamorphism of ∼8 kbar, 916°−932°C (∼33.3°C/km) at ∼15 Ma. These results indicate that the Himalayas exhibited elevated thermal gradients during protracted collisions. Given the thick felsic crust and high rate of heat production, thermal modeling results indicate that radiogenic heating during prolonged collision caused the Himalayan crust to be hot, even to ultra‐high temperature conditions, and led to the elevated geothermal gradients. As a premier example of continental orogenesis, the Himalaya is distinctly hotter than the cold Alpine‐type orogens. This thermal difference could stem from a reduced convergence rate, low‐angle underthrusting, vigorous felsic magmatism, and persistent shear heating.

MBRLCatalogueRelatedBooks