Formation of the Greater Caucasus by two-stage closure of a relict ocean basin and the transition from soft to hard Arabia-Eurasia collision

Eric Cowgill(Planetary Science Institute), Tea Godoladze(Ilia State University), Nikolas Midttun, Dylan A. Vasey(Tufts University), Nathan A. Niemi(University of Michigan), Elaine Young, Alexander Tye(Jet Propulsion Laboratory), Charles C. Trexler(Planetary Science Institute), Z. Javakhishvili(Ilia State University), Giorgi Boichenko, Adam M. Forte(Louisiana State University)
EGUGA
April 1, 2018
Cited by 0

Related Papers

Constraints on the volatile distribution within Shackleton crater at the lunar south pole
|Nature|2012|204
Relict basin closure and crustal shortening budgets during continental collision: An example from Caucasus sediment provenance
|Tectonics|2016|127
The age of lunar south circumpolar craters Haworth, Shoemaker, Faustini, and Shackleton: Implications for regional geology, surface processes, and volatile sequestration
|Icarus|2015|61
Low variability runoff inhibits coupling of climate, tectonics, and topography in the Greater Caucasus
|Earth and Planetary Science Letters|2022|25
Sedimentary response to a collision orogeny recorded in detrital zircon provenance of Greater Caucasus foreland basin sediments
|Basin Research|2020|23