The Mars 2020 Rover Mission: EISD Participation in Mission Science and ExplorationThe Mars 2020 Rover mission will search for potential biosignatures on the martian surface, use new techniques to search for and identify tracelevel organics, and prepare a cache of samples for potential return to Earth. Identifying trace organic compounds is an important tenet of searching for potential biosignatures. Previous landed missions have experienced difficulty identifying unambiguously martian, unaltered organic compounds, possibly because any organic species have been destroyed on heating in the presence of martian perchlorates and/or other oxidants. The SHERLOC instrument on Mars 2020 will use ultraviolet (UV) fluorescence and Raman spectroscopy to identify trace organic compounds without heating the samples.
Document ID
20150001632
Acquisition Source
Johnson Space Center
Document Type
Presentation
Authors
Fries, M. (NASA Johnson Space Center Houston, TX, United States)
Bhartia, R. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Beegle, L. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Burton, A. S. (NASA Johnson Space Center Houston, TX, United States)
Ross, A. (NASA Johnson Space Center Houston, TX, United States)
Date Acquired
February 13, 2015
Publication Date
November 18, 2014
Subject Category
Lunar And Planetary Science And ExplorationGround Support Systems And Facilities (Space)