Geological Society of America

T167 Robotic Exploration of Planetary Surfaces: The G.K. Gilbert Award Session

Tuesday, 11 October 2011
8:00 AM - 12:00 PM
Room L100H-J

MEPAG RECOMMENDATIONS FOR A 2018 MARS SAMPLE RETURN CACHING LANDER – SAMPLE TYPES, NUMBER, AND SIZES

Paper number: T167-10
Program: Technical Sessions
Time: 10:15 AM – 10:30 AM

Authors

Carlton C. Allen Presenting Author
Houston, TX
Steve Symes
University of Tennessee, Knoxville, TN
Mark Sephton
Imperial College, London, N/A
Scott M. McLennan
Stony Brook Research Foundation, Stony Brook, NY
David W. Beaty
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA
Penny Boston
New Mexico Institute of Mining and Technology, Socorro, NM
Monica Grady
Open University, Milton Keynes
Veronika Heber
Univ. of California Los Angeles, Los Angeles, CA
Christopher D. K. Herd
University of Alberta, Edmonton, AB
Steven Ruff
Arizona State University, Tempe, AZ

Abstract

The return to Earth of geological & atmospheric samples from the surface of Mars is among the highest priority objectives of planetary science. The MEPAG Mars Sample Return (MSR) End-to-End International Science Analysis Group (MEPAG E2E-iSAG) was chartered to propose scientific objectives & priorities for returned sample science, & to map out the implications of these priorities, including for the proposed joint ESA-NASA 2018 mission that would be tasked with the crucial job of collecting & caching the samples.

The E2E-iSAG identified four overarching scientific aims that relate to understanding: A) the potential for life & its pre-biotic context, B) the geologic processes that have affected the martian surface, C) planetary evolution of Mars & its atmosphere, D) potential for future human exploration.

The types of samples deemed most likely to achieve the science objectives are, in priority order:

1A. Subaqueous or hydrothermal sediments

1B. Hydrothermally altered rocks or low temperature fluid-altered rocks (equal priority)

2. Unaltered igneous rocks

3. Regolith, including airfall dust

4. Present-day atmosphere & samples of sedimentary-igneous rocks containing ancient trapped atmosphere

Collection of geologically well-characterized sample suites would add considerable value to interpretations of all collected rocks. To achieve this, the total number of rock samples should be about 30-40.

In order to evaluate the size of individual samples required to meet the science objectives, the E2E-iSAG reviewed the analytical methods that would likely be applied to the returned samples by preliminary examination teams, for planetary protection (i.e., life detection, biohazard assessment) and, after distribution, by individual investigators. It was concluded that sample size should be sufficient to perform all high-priority analyses in triplicate. In keeping with long-established curatorial practice of extraterrestrial material, at least 40% by mass of each sample should be preserved to support future scientific investigations. Samples of 15-16 grams are considered optimal. The total mass of returned rocks, soils, blanks & standards should be approximately 500 grams. Atmospheric gas samples should be the equivalent of 50 cm³ at 20 times Mars ambient atmospheric pressure.

Coauthors: The MEPAG E2E-iSAG Team