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Revolutionizing Access to the Mars Surface
A workshop hosted by the W.M. Keck Institute for Space Studies led by:Chris Culbert Abby Fraeman Bethany Ehlmann
Presenter: International Planetary Probe WorkshopZach Putnam Mars Exploration SessionUniversity of Illinois at Urbana-Champaign July 8, 2021
Motivation
Many key science goals can only be accomplished in situand many benefit enormously from surface mobility
Mars, the Nearest Habitable World October 2020 MASWG III. Findings
27
to the destination, or independently launched spacecraft that take advantage of emerging small launch capabilities.
We will use the term Small-Spacecraft class (SSc) to mean spacecraft having a full life-cycle cost in the range of ~$100M–300M. SSc using present-day technology/capabilities could make high-priority scientific measure-ments from orbit (e.g., for study of atmosphere processes and climate). They could also pro-vide a platform for other types of science meas-urements (e.g., network landers for geophysics, subsurface ice detection, or boundary layer processes) utilizing technologies that could be developed in the next 5–10 years. Small-space-craft capabilities relative to cost, requirements, and performance need to be addressed pro-grammatically to realize their full potential. Existing challenges to implementing Mars small spacecraft science missions include early identification of rideshare launch opportunities as well as enhanced technological capabilities in the specific areas of propulsion, communica-tion, and entry descent and landing. More detail on the programmatic opportunity of small
spacecraft during sample return is provided in Section IV.B. Finding 7: Affordable access to the surface.
A critical scientific need for Mars explo-ration is affordable access to multiple places on the Martian surface with adequate pay-load/mobility to make the measurements that would revolutionize our understanding of the Mars system.
Rationale: The Mars program has reached a point where many of the most pressing meas-urements for key science topics can only be ad-dressed in situ (see Figure III-1). These include (see Sections II.E and VI) ancient environmen-tal diversity (cm-scale petrology and stratigra-phy), modern climate variability (cm-scale analysis at the polar caps), biogeochemical cy-cles (isotopic measurements of volatiles in rocks), solar system chronology (in situ iso-topes), and life detection (in situ organics) (e.g., Ehlmann et al. [2016]). Our growing knowledge from orbiters has pinpointed key lo-cations that in several instances (e.g., ancient environments exploration, geochronology)
Figure III-1. Traceability match from science goal mission element to Small Spacecraft (SSc), Discovery (DSc), New Frontiers (NFc), and Flagship (FLG) class missions. The numbers in the M-Arc column refer to the mission “arcs” (sequences of mission types) defined and described in Section VI.B.
MASWG Nov. 2020 Reporthttps://mepag.jpl.nasa.gov/reports/MASWG%20NASA%20Final%20Report%202020.pdf
July 8, 2021 Revolutionizing Access to the Mars Surface 1
Motivation1. Can we fit PI-competed
surface missions in Discovery/small spacecraft mission classes, including mobility systems?
2. Can small sat approaches and technology feed forward to Mars?
3. Can CLPS approaches and technology feed forward to Mars?
July 8, 2021 Revolutionizing Access to the Mars Surface 2Image credit: NASA
Workshop GoalsOverarching Goal: Determine how to substantially reduce the cost associated with landed scientific missions to Mars. How? Three primary goals: 1. Identify most important measurements related to Decadal survey
science questions that require access to Martian surface and instruments/platforms/mobility required to achieve them.
2. Conceive mission architecture(s) and technologies to access the Martian surface (e.g. EDL) and conduct efficient operations of multiple Mars assets.
3. Identify how/if emerging small satellite approaches, commercial lunar capabilities, or other innovative approaches can break the mass-cost dependency for Mars surface missions and enable access at lower price point.
July 8, 2021 Revolutionizing Access to the Mars Surface 3
In Situ Science Measurement Needs• Atmosphere: measurements in lowest scale height not
available from orbit; concurrent measurements provide additional science value• Geology: local and regional-scale measurements needed; long
traverses provide geological comparison• Geophysics: multiple landing sites (network) and/or mobility
needed
July 8, 2021 Revolutionizing Access to the Mars Surface 4
Multiple landers and/or mobility systems needed to address high-priority science goals across multiple science disciplines.
Improving Surface Access: [some] Tall Tent Poles
Cultural and Programmatic• Current community risk
posture• Make “smaller science” okay• The “cost=mass” mentality• Limited mission opportunities
Technology• EDL system• Surface mobility• Payload SWaP• Manufacturing, ATLO
July 8, 2021 Revolutionizing Access to the Mars Surface 5
EDL Systems and Cost• Current paradigm: each EDL system is bespoke…and expensive.• Options for reducing EDL cost:• Eliminate subsystems (e.g. remove landing system à hard lander)• Miniaturization• Additive manufacturing• Block buys and builds
• Potential EDL contributions to mission cost reduction• Deployables for rideshare packaging and/or improved performance• High-g landing systems• Use more mass to reduce cost (e.g. larger aeroshells)
July 8, 2021 Revolutionizing Access to the Mars Surface 6
Continuing Workshop Efforts• 4 study groups investigating high-priority areas:
1. Programmatic changes to Mars exploration program2. The “Culture Club”3. $200M Medium Mobile Mission (or MMM…)4. Architecture trade study for small networks
• Second workshop meeting in September
• Final report to follow
July 8, 2021 Revolutionizing Access to the Mars Surface 7
Acknowledgements
Sam Albert – University of Colorado BoulderDon Banfield – Cornell UniversityJon Bapst – JPLKevin Bonnet – University of ColoradoJoel Burdick – CaltechWendy Calvin – University Nevada – Reno Barbara Cohen – NASA Goddard Tim Crain – Intuitive Chris Culbert – NASA JSC Charles (Chad) Edwards - JPL Bethany Ehlmann – Caltech Giusy Falcone – University of Illinois Abby Fraeman – JPL Elizabeth Frank – First Mode Andrew Horchler – Astrobotic
Mark Johnson – Lockheed MartinBrett Kennedy – JPLLaura Kerber – JPLDavid Masten – Masten Space Systems Larry Matthies – JPL Michelle Munk NASA Langley Research Center David Murrow – Lockheed Martin Paul Niles – NASA JSC Mark Panning – JPL Zachary (Zach) Putnam – University of Illinois Eva Scheller – Caltech Nathan Stein – CaltechRachel Sheppard – JPLSkylar Wei – Caltech Ryan Woolley – JPLPaul Wooster – SpaceX
W.M. Keck Institute for Space Studies for hosting the workshop.
Participants:
July 8, 2021 Revolutionizing Access to the Mars Surface 8