Postdoctoral Research Opportunity at the University of Hawaii: Fluid migration in Titan’s ice shell
As part of the new NASA Astrobiology Institute (NAI) project “Habitability of Hydrocarbon Worlds: Titan and Beyond”, we are investigating the mechanisms and pathways by which biosignature-hosting materials might be transported from a habitable ocean environment to the surface, where they could be recognized by remote sensing instruments. These mechanisms might include cryovolcanism, solid state convection in the ice shell, fracture/fault propagation, and the formation of subsurface fluid reservoirs that might facilitate fluid migration to the surface. See nai.nasa.gov/teams/can-8/jpl-titan/ for a more detailed description of the overall project.
An opportunity exists in this area for a postdoctoral researcher to develop a proposal for the NASA Astrobiology Postdoctoral Program, for a project to be pursued at the University of Hawaii. The desired candidate will have a solid physics, math, or geology/geophysics background, and interests/expertise in numerical modeling, cryomagmatism, ice physics, Titan and/or other icy satellites. The next deadlines for this program are November 1 and March 1. If the proposal is selected for funding, the anticipated start dates would be spring/summer 2019 or fall 2019, respectively. More details are available at nai.nasa.gov/funding/postdoctoral-fellowship-program
Please contact Sarah Fagents at [email protected] for more information.