The Johns Hopkins Applied Physics Laboratory has submitted a proposal to NASA outlining a daring New Frontiers-class mission concept that would use an instrumented, radioisotope-powered dual-quadcopter to explore potential habitable sites where life could be developed on Saturn’s largest moon, Titan.
“Seems pretty straightforward,” quipped Dragonfly project manager Peter Bedini in a video presentation of the proposal.
The concept, called Dragonfly, would capitalize on the rapid advances made in recent years to autonomous aerial systems—sometimes referred to as the “drone revolution.” The increased reliability and capability these systems would enable Dragonfly to make numerous flights, moving from one geologic setting to another on the moon’s surface.
Titan has diverse, carbon-rich chemistry on a surface dominated by water ice, as well as an interior ocean. It is one of a number of “ocean worlds” in our solar system that hold the ingredients for life, and the rich organic material that covers the moon is undergoing chemical processes that might be similar to those on early Earth. Dragonfly would take advantage of Titan’s dense, flight-enabling atmosphere to visit multiple sites by landing on safe terrain, and then carefully navigate to more challenging landscapes.
“This is the kind of experiment we can’t do in the laboratory because of the time scales involved,” said APL’s Elizabeth Turtle, principal investigator for the Dragonfly mission. “Mixing of rich, organic molecules and liquid water on the surface of Titan could have persisted over very long timescales. Dragonfly is designed to study the results of Titan’s experiments in prebiotic chemistry.”
With Titan’s dense atmosphere and low gravity, flight is substantially easier than on Earth, giving Dragonfly a very broad range of capability. While there is enough sunlight at Titan’s surface to see, there is not enough to use solar power efficiently, so Dragonfly would be powered by a Multi-Mission Radioisotope Thermoelectric Generator, or MMRTG.
Measuring Titan’s Habitability
At each site, Dragonfly would sample the surface and atmosphere with a suite of carefully selected science instruments that will characterize the habitability of Titan’s environment, investigate how far prebiotic chemistry has progressed, and search for chemical signatures indicative of water- and/or hydrocarbon-based life. These measurements include:
- Mass spectrometry, which would reveal the composition of the surface and the atmosphere;
- Gamma-ray spectrometry, which would measure the composition of the shallow sub-surface;
- Meteorology and geophysics sensors, which would measure atmospheric conditions such as wind, pressure, temperature, as well as seismic activity and other factors; and
- A camera suite that would characterize the geologic and physical nature of the moon’s surface, and help find subsequent landing sites.
“We could take a lander, put it on Titan, take these four measurements at one place, and significantly increase our understanding of Titan and similar moons,” said Bedini. “However, we can multiply the value of the mission if we add aerial mobility, which would enable us to access a variety of geologic settings, maximizing the science return and lowering mission risk by going over or around obstacles.”
Later this fall, NASA is expected to select a few of the New Frontiers mission proposals for further study. Only one will be chosen for flight as the fourth mission in the planetary exploration program; the APL-led New Horizons mission to Pluto and the Kuiper Belt was the first New Frontiers mission ever selected. Final mission selection is expected in mid-2019.
This article was provided by John Hopkins University. Materials may have been edited for clarity and brevity.