Author(s): Elizabeth Turtle
Panel Selection: Satellites
Institution: Johns Hopkins University/Applied Physics Laboratory
The Jovian moon Io is likely the most geologically active body in the solar system, offering insight into tidal heating, volcanic processes, and other phenomena. However, its location within Jupiter''s radiation belt presents significant engineering challenges that must be addressed to enable future missions to Io. Under the direction of NASA, and with direct guidance from the National Research Council''s (NRC''s) Satellites Panel, the Jet Propulsion Laboratory''s (JPL''s) Advanced Project Design Team (Team X) looked at the feasibility of a remote observational mission to Io as a possible future New Frontiers concept.

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