Scientific Investigations To Prepare For The Potential Human Exploration Of Mars
Abstract
In order for human missions to the martian system to be successful and safe, we need a certain minimum set of knowledge. Comparison of what we need to know with what we already know defines what we refer to as "Strategic Knowledge Gaps (SKGs)". The SKG list needs to be the driving force behind the robotic precursor program. The Mars SKG list was first constructed by the Precursor Strategy Analysis Group (P-SAG) in 2012. It consisted of 17 SKGs that could be addressed by about 60 gap-filling activities (GFA). These GFAs were split into three groups based on where and how they could be carried out: requires a Mars flight/mission, addressed on Earth, or technology demonstration. Those GFAs that require a Mars mission were incorporated into the revision of the 2012 Goals Document of the Mars Exploration Program Analysis Group (MEPAG) as "investigations" under Goal IV: Prepare for Human Exploration. In 2015, MEPAG updated the Goals Document, and comparison of the 2012 and 2015 versions shows that significant and encouraging overall progress has been made on a number of the investigations. We note three specific kinds of changes: 1) Complete retirement of several investigations, 2) Decreased investigation priority based on partial progress, and 3) Addition of a few new investigations. Some of these changes are detailed below: Retired: • Simultaneous spectra of solar energetic particles in space and ion the surface • Spectra of galactic cosmic rays on the surface • Trace gas abundances • Determine traction/cohesion in martian regolith • Determine vertical variation in regolith • High spatial resolution maps of mineral composition and abundance • High spatial resolution maps of subsurface ice depth and concentration Decreased Priority: • Making long-term measurements of winds and wind directions (improvements in EDL technologies have decreased the importance of this measurement) • Profile the near-surface winds (improvements in EDL technologies have decreased the importance of this measurement) • Dust physical, chemical and electrical properties (rover data from multiple locations has provided sufficient information on these properties) New: • Measure solar energetic particles at the martian surface throughout the ~11 year solar cycle to characterize "extreme conditions" • Test ISRU atmospheric processing system to measure resilience with respect to dust and other environmental challenge performance parameters. • Identify and map a set of candidate water resource deposits that have the potential to be relevant for future human exploration. What would it take to respond to the remaining SKGs? Missions such as Mars 2020, a future orbiter (with potential instruments such as those detailed by the Next Orbiter Science Analysis Group), potential sample return and precursor missions (including an EDL pathfinder and resource prospectors) would reduce the priority of most of the remaining SKGs, or retire them entirely.
- Publication:
-
41st COSPAR Scientific Assembly
- Pub Date:
- July 2016
- Bibcode:
- 2016cosp...41E.814H