Pluto’s glaciers

Dr Matt Telfer (Plymouth)
“Pluto’s ‘desert’: Methane ice dunes on a glacier on an airless world”

As well as the deserts of Earth, dunes have been identified on Venus, Mars and Saturn’s moon Titan. Tantalizingly dune-like features were described from the atmosphereless comet 67P Churyamov-Gerasimenko from the ESA’s Rosetta orbiter, but prior to New Horizon’s 2015 flyby of Pluto, so little was known of the geology of this world that predictions of its surface were extremely difficult. When images from Pluto revealed landforms startlingly similar to dunes from Earth’s deserts, the question of how it was possible to have dunes with an atmosphere only 1/100,000th that of Earth (~ 1 Pa) arises. Here we describe the spectral, spatial and image analysis, which, together with numerical modelling, solved this puzzle.

Organised By
Institute of Physics Lancashire and Cumbria Branch
Date/Time
12 Jun 2019 18:00 to 20:00
Location
Cavendish Colloquium Room
Lancaster University
Lancaster
Lancashire
UK
LA1 4YB
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