Video by Elaine Walker (EPO, HMP, Mars Institute)
Copyright 2010 Mars Institute
This blog is courtesy of Haughton Mars Project (HMP)
For more information please visit www.marsonearth.org
Kelsey Young is a geologist in the School of Earth and Space Exploration at Arizona State University. Kelsey earned her undergraduate degree in geology from the University of Notre Dame where she studied Earth-based analogs for Mars. Specifically, she conducted fieldwork to study the interactions of lava and water in conjunction with examining similar features on the surface of Mars. While completing this work, she became interested in using terrestrial analogs to work on issues associated with manned space exploration. Kelsey is now working on her Ph.D. in geology, and is pursuing this interest by combining geology with the logistics of planetary surface exploration.
Working in terrestrial analog sites like Haughton Mars Project gives her first-hand experience on active processes happening on other planetary surfaces. While at HMP- 2010, Kelsey will be collecting impact breccia samples from inside the crater in order to date the age of the impact using (U-Th)/He thermochronology.
Kelsey is currently working under one of NASA’s Graduate Student Researcher Program’s (GSRP) Fellowships, so she is working closely with NASA Johnson Space Center on incorporating a spectrometer into the Desert RATS field test (another analog test run by NASA). She will be supporting D-RATS as both a member of the sciencebackroom, and as one of four geologist crewmembers for the test.
School of Earth and Space Exploration
Arizona State University