NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Connecting Community Scientific Hypotheses to Mars Sample ScienceThe proposed Mars Sample Return (MSR) program seeks to bring back to Earth a set of specially curated samples from the surface of Mars. The first segment of the MSR program is presently under-way; the Mars 2020 rover Perseverance has, to date, collected 24 samples of martian rock, regolith, and at-mosphere within Jezero crater. Its geologically diverse rock sample set can provide insight into the time evolu-tion of the Jezero environment, including the possible preservation of ancient biosignatures. Presently, a cache of 10 samples has been deposited in the Three Forks region on the floor of Jezero crater. These sam-ples, deemed scientifically return worthy by the Mars science community [1], are intended as a contingency sample set, as Perseverance has subsequently obtained more samples, and is therefore storing a more compre-hensive and scientifically valuable set of samples that will grow as the rover ascends to the rim of Jezero crater.
The return of samples from Mars has been identi-fied as the highest priority planetary mission in the past three National Academies Decadal Surveys [2-4]. Sub-stantial work has gone into establishing science objec-tives for an MSR program, an overall framework for sample retrieval and analysis, and the expected impact on future Mars science and exploration (e.g., [5]). These objectives have been established at a relatively high level, e.g., “Interpret the primary geologic pro-cesses and history that formed the martian geologic rec-ord, with an emphasis on the role of water.” (Objective 1 in [5]) and are designed to encapsulate the broad sci-entific priorities of, and lay the groundwork for, inves-tigation strategies and measurements to be conducted by a future MSR program. It is from this overarching framework that the Connecting Community Scientific Hypotheses to Mars Sample Science workshop (‘The Workshop’) was conceived, with the purpose of distil-ling these high-level scientific objectives into discrete, testable hypotheses across a range of scientific disci-plines. The output of the workshop is meant to be a ‘hy-pothesis document’ serving as a starting point for cata-loging and condensing specific hypotheses for consid-eration by the scientific community. The template for this approach is based on the “driving hypotheses” de-veloped by the OSIRIS-REx team as part of their Sam-ple Analysis Plan [6].
Document ID
20240005601
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Michael A Mischna
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Victoria E Hamilton
(Southwest Research Institute San Antonio, United States)
Philipp Heck
(Field Museum of Natural History Chicago, United States)
Yang Liu
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Lydia Hallis
(University of Glasgow)
Justin Filiberto
(Johnson Space Center Houston, United States)
Brandi Carrier
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Date Acquired
May 3, 2024
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: Tenth International Conference on Mars
Location: Pasadena, CA
Country: US
Start Date: July 22, 2024
End Date: July 25, 2024
Sponsors: Universities Space Research Association, Lunar and Planetary Institute
Funding Number(s)
WBS: 811073
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
No Preview Available