Instrument Development Enables Planetary Exploration
This laser-interrogated microfluidic chip (10 centimeters in diameter) is one of the new planetary instrument technologies that NASA and other space agencies are developing to search for chemical indicators of life on other worlds. In this lab-on-a-chip device, a laser excites labeled amino acid molecules as they pass through a microchannel. Different amino acid types pass through the channel at well-defined speeds, enabling their identification. (Image Credit: Fernanda Mora and Amanda Stockton, Microdevices Laboratory, Jet Propulsion Laboratory, California Institute of Technology)
The scientific knowledge gained from future planetary exploration missions will depend critically on the capabilities of instruments (cameras, spectrometers, magnetometers, thermal sensors, seismometers, remote laboratories, and other robotic tools) that acquire sensory information in lieu of human explorers. The flight opportunities available to planetary instrument developers depend on a complex interplay among mission science requirements; technology capabilities; mass, power, and volume constraints; planetary geometries; and funding availability.
Last October, more than 195 engineers, scientists, technologists, and program managers, representing 12 countries, met in California for the third workshop in a series that began in 2012 at the Goddard Space Flight Center and has been held every 2 years since.
The workshop provided a forum for collaboration, team building, exchange of ideas and information, and the presentation of status reports for instruments, subsystems, and other payload-related technologies needed to address planetary science questions. Oral and poster sessions were based on 136 submitted abstracts.
Panel sessions were organized around three themes:
- perspectives on the future of planetary exploration
- bridging the gap between planetary scientists and instrument developers
- lessons learned for instrument development at various technology readiness levels (TRL 1–9)
The “perspectives” panel addressed planetary science priorities and opportunities over the next several decades for planetary instruments on missions to Mars, the Moon, Mercury, Venus, small bodies, and the outer planets. Panel participants strongly supported existing technology development programs, including NASA’s Planetary Instrument Concepts for the Advancement of Solar System Observations (PICASSO) and Maturation of Instruments for Solar System Exploration (MatISSE).
The panel emphasized that innovative approaches enhance mission science return, but new technology development efforts must effectively address cost and technical risk concerns, provide clear advantages over currently existing capabilities, and take into account mission schedules. They agreed that emerging low-cost demonstration platforms (e.g., planetary CubeSats and SmallSats) provide invaluable opportunities to help new planetary instrument technologies mature and reduce the development risk in transitioning them to larger missions.
The “bridging the gap” panel emphasized the importance of scientists, technologists, and engineers connecting at meetings. These groups must be willing to consider partnerships with private industry, learn new roles, and become fluent in disciplines outside of their formal training.
End-of-workshop feedback mentioned the difficulty in getting scientists and instrument engineers together at the traditional conferences and recommended that the community should seek ways to expand networking opportunities. For example, instrument talks could be incorporated into the annual Lunar and Planetary Science Conference.
More details on the presentations are available in the workshop abstracts. The workshop also produced an open-source online instrument database to facilitate ongoing input from developers.
The workshop was sponsored by the Lunar and Planetary Institute. The next workshop in this series is tentatively scheduled to take place in Berlin, Germany, in the fall of 2018.
—Sabrina M. Feldman, David Beaty, and James W. Ashley (email: james.w.ashley@jpl.nasa.gov), Jet Propulsion Laboratory, California Institute of Technology, Pasadena
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