In 2015, the New Horizons spacecraft provided our first up-close look at Pluto and its moons, helping to transform our knowledge about these small, cold worlds in the outer fringes of the solar system. The only downside, if there were one, was that it was a flyby mission, meaning New Horizons would zip past Pluto and then continue on deeper into the Kuiper Belt. Since then, there has been growing advocacy for a return mission such as an orbiter, or perhaps even a lander.
This week – at the NASA Innovative Advanced Concepts (NIAC) Symposium (September 25-27, 2017) in Denver, Colorado – Global Aerospace Corporation (GAC) presented a concept mission for a Pluto lander. As currently envisioned, the probe would land on Pluto using drag from the super-thin atmosphere and a few pounds of propellant. Then, it could explore the surface further by hopping from one location to another, using Pluto’s low gravity. The probe would be capable of traveling tens or even hundreds of kilometers at a time and features of interest could be studied up close at many different locations. The entrycraft, as it is called, would need to be almost the size of a football field in order to bring the lander to the surface.
According to GAC, the mission could be launched as soon as 12 years from now.
Benjamin Goldman, principal investigator of the Phase I NIAC effort, said:
Pluto’s surface pressure is just 10 millionths of Earth’s, but its atmosphere is extremely spread out, extending about 1,000 miles above the surface. This extended and ultra-low-density atmosphere is ideal for dissipating large amounts of kinetic energy by means of aerodynamic drag, but the key is making the drag area very large while keeping system weight at a minimum.
Some goals of the mission would be to:
– Shed new light on its origins and relationship to other Kuiper Belt objects and other planets.
– Characterize the dynamics between the subsurface and the atmosphere by investigating outgassing processes such as cryovolcanism.
– Expand the understanding of surface geomorphology from multiple locations (on approach, during descent, and at the surface).
– Use in-situ sampling to study the nature of the its crust and search for hypothesized liquid water oceans.
– Validate New Horizons measurements including atmospheric pressure and temperature profiles.
New Horizons was an exciting mission, even if it only offered a brief look at the Pluto system. But that brief glimpse showed that Pluto is an active world, with nitrogen ice seas and glaciers, water ice mountains with methane snow, tall spikes of ice, ancient rivers and lakes of liquid nitrogen, a hazy atmosphere and possible cryovolcanoes (ice volcanoes). There may even be a subsurface ocean of water. Pluto’s largest moon, Charon, also appears to have had a subsurface ocean, but it is completely frozen now. It is a bizarre and intriguing place, begging for a return mission to explore its mysteries further. An orbiter would be a phenomenal follow-up to New Horizons, and a lander even more so. Pluto was once just a tiny point of light only visible to the largest telescopes, but now it is an incredible world just waiting to be explored in-depth.
Paul Scott Anderson has had a passion for space exploration that began when he was a child when he watched Carl Sagan’s Cosmos. While in school he was known for his passion for space exploration and astronomy. He started his blog The Meridiani Journal in 2005, which was a chronicle of planetary exploration. In 2015, the blog was renamed as Planetaria. While interested in all aspects of space exploration, his primary passion is planetary science. In 2011, he started writing about space on a freelance basis, and now currently writes for AmericaSpace and Futurism (part of Vocal). He has also written for Universe Today and SpaceFlight Insider, and has also been published in The Mars Quarterly and has done supplementary writing for the well-known iOS app Exoplanet for iPhone and iPad.