NASA has selected research teams through its Solar System Exploration Research Virtual Institute (SSERVI) Cooperative Agreement Notices, bringing researchers together in a collaborative virtual setting to focus on questions concerning space science and human space exploration.
SSERVI teams address scientific and technology development questions pertaining to the Moon, near-Earth asteroids, the Martian moons Phobos and Deimos, and their near space environments. Although primarily addressing plans described in their proposals, they also partner with other SSERVI teams and SSERVI international partners to create cross-disciplinary efforts beyond their original efforts.
Based and managed at NASA’s Ames Research Center at Moffett Field, Calif., the institute supports scientific research to complement and extend existing NASA science and technology programs. SSERVI represents an expansion of NASA’s Lunar Science Institute, established at Ames in 2008, to include other solar system human exploration destinations.
The selected SSERVI member teams are:
– Center for Lunar and Asteroid Surface Science (CLASS); principal investigator Dan Britt, University of Central Florida (UCF) in Orlando.
Focus: Regolith of the Moon and asteroids, specifically looking at the physical properties and resources of regolith and its behavior in the space environment. CLASS also will create soil simulants that will help other teams and the broader science community in this research area.
– Interdisciplinary Consortium for Evaluating Volatile Origins (ICE FIVE-O); principal investigator Jeffrey Gillis-Davis, at Washington University.
Focus: Remote sensing of airless bodies and how things weather in space. Modeling the physical, chemical, and isotopic signatures around the Moon’s polar regions. ICE FIVE-O will address curation protocols for sample return and the evolution of volatiles, or low-boiling point compounds, and minerals within long-duration, curated samples.
- Remote, In Situ, and Synchrotron Studies for Science and Exploration 2 (RISE2); principal investigator Timothy Glotch, Stony Brook University in New York.
Focus: This team will investigate how planetary environments impact human health by looking at the chemical reactivity of regolith in association with animal cells and tissues. RISE2 also will analyze how remote sensing datasets can be confirmed through laboratory experiments, analyses, and field deployments.
– Resource Exploration and Science of OUR Cosmic Environment (RESOURCE); principal investigator Jennifer Heldmann, NASA’s Ames Research Center in California’s Silicon Valley.
Focus: This team focuses on determining what volatiles are available on the Moon for in-situ resource utilization. It will assess the quantity and availability of resources on the Moon, test the technology required for processing those resources, and field test the concepts of operations required for sustained human lunar presence.
- Institute for Modeling Plasmas, Atmospheres, and Cosmic Dust (IMPACT); principal investigator Mihaly Horanyi, University of Colorado Boulder.
Focus: This team will measure micron-sized dust impacts in icy regolith using the world’s fastest “dust impact” facility, and they will develop hardware to determine secondary particle generation and examine how that hardware degrades over time. IMPACT also will use laboratory experiments to help validate theories of dust and volatile mobility and modeling efforts being completed by other SSERVI teams.
- Lunar Environment And Dynamics for Exploration Research (LEADER); principal investigator Rosemary Killen, NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
Focus: This team will focus on plasma interactions with airless bodies and determine the effects of the space environment on robotic and human assets at various geographic locations on the Moon. The team also will model the radiation environments and related effects associated with space exploration.
– Center for Lunar Science and Exploration (CLSE); principal investigator David Kring, Lunar and Planetary Institute in Houston.
Focus: Through modeling and geochemical analyses, this team will track the distribution and form of volatiles from the early solar system to the formation of the Moon and subsequent evolution to today. This team will analyze the volatile cycle on the Moon to determine overall source and loss mechanisms and how we can use these resources.
- Geophysical Exploration Of the Dynamics and Evolution of the Solar System (GEODES); principal investigator Nicholas Schmerr, University of Maryland in College Park.
Focus: This team will use geophysical modeling and laboratory techniques to characterize the overall evolution, stability, and volatile content of the Moon and asteroid subsurfaces. GEODES will test its theories through analog field campaigns in conjunction with other NASA/SSERVI instrument testing efforts.
– Network for Exploration and Space Science (NESS); principal investigator Jack Burns, University of Colorado in Boulder, CO.
Focus: Conducting research in robotics, cosmology, astrophysics and heliophysics.
– Exploration Science Pathfinder Research for Enhancing SS Observations (ESPRESSO); principal investigator Alex Parker, Southwest Research Institute in Boulder, CO.
Focus: A range of science and operations objectives relevant to characterizing target surfaces and mitigating hazards that create risk for robotic and human explorers.
– Toolbox for Research and Exploration (TREX); principal investigator Amanda Hendrix, Planetary Science Institute in Tucson, AZ.
Focus: Laboratory spectral measurements and experiments, data analysis, surface characteristics & ISRU on airless bodies.
– Radiation Effects on Volatiles and Exploration of Asteroids & Lunar Surfaces (REVEALS); principal investigator Thomas Orlando, Georgia Institute of Technology in Atlanta, GA.
Focus: Radiation chemistry, volatile formation, volatile sequestration and transport, regolith and composite materials.
– Institute for the Science of Exploration Targets (ISET); principal investigator William Bottke, Southwest Research Institute in Boulder CO.
Focus: Formation of terrestrial planets and asteroid belt, modeling of the Moon’s origin and Phobos/Deimos, history of NEAs and lunar bombardment, NEA origins, identification and characterization
– Center for Lunar and Asteroid Surface Science (CLASS); principal investigator Daniel Britt, University of Central Florida in Orlando FL.
Focus: Studies of physical properties of regoliths: geotechnical properties, microgravity effects, impact ejecta, dynamics, hydration and weathering of NEAs, charging and mobilization of dust
– Volatiles, Regolith and Thermal Investigations Consortium for Exploration and Science (VORTICES); principal investigator Andy Rivkin, Johns Hopkins University Applied Physics Laboratory in Laurel MD.
Focus: Volatiles sources/sinks/processes and interaction with regoliths, evolution of regoliths on all target bodies, identification and exploitation of resources
– Dynamic Response of Environments at Asteroids, the Moon, and moons of Mars (DREAM2); principal investigator William Farrell, NASA Goddard Space Flight Center in Greenbelt MD. Focus: Plasma interactions, exospheres, Radiation of exposed materials, space weathering, solar storms/solar wind
– Remote, In Situ and Synchrotron Studies for Science and Exploration (RIS4E); principal investigator Timothy Glotch, Stony Brook University, NY.
Focus: Remote sensing of airless bodies, field operations and metrics for human exploration, reactivity and toxicity of regoliths, synchrotron analyses of samples, volcanics and impact crater analog research
– Field Investigations to Enable Solar System Science and Exploration (FINESSE); principal investigator Jennifer Heldmann, NASA Ames Research Center, CA. Focus: Field operations and metrics for human exploration and analog research.
– Institute for Modeling Plasma, Atmospheres and Cosmic Dust (IMPACT); principal investigator Mihaly Horanyi, University of Colorado in Boulder CO.
Focus: Small scale impact studies/regolith gardening, plasma charging and mobilization of dust, near surface plasma environments, new advancements on dust accelerator facility
– Inner Solar System Impact Processes; principal investigator David Kring, Lunar and Planetary Institute in Houston TX.
Focus: Impact history and processes, geochemistry of regoliths, age dating of regolith materials, NEA identification and characterization
– Evolution and Environment of Exploration Destinations: Science and Engineering Synergism (SEEED); principal investigator Carle Pieters, Brown University in Providence RI.
Focus: Thermal/chemical evolution of planetary bodies, origin and evolution of volatiles, remote sensing, space weathering of regoliths