HR: 16:30h
AN: P54A-03    [Abstracts]
TI: Europa Geophysical Explorer Mission Concept Studies
AU: * Green, J R
EM: jacklyn.r.green@jpl.nasa.gov
AF: Jet Propulsion Laboratory/California Institute of Technology, Mail Stop 301-170S 4800 Oak Grove Drive, Pasadena, CA 91109 United States
AU: Abelson, R D
EM: robert.d.abelson@jpl.nasa.gov
AF: Jet Propulsion Laboratory/California Institute of Technology, Mail Stop 301-170S 4800 Oak Grove Drive, Pasadena, CA 91109 United States
AU: Smythe, W
EM: william.smythe@jpl.nasa.gov
AF: Jet Propulsion Laboratory/California Institute of Technology, Mail Stop 301-170S 4800 Oak Grove Drive, Pasadena, CA 91109 United States
AU: Spilker, T R
EM: thomas.r.spilker@jpl.nasa.gov
AF: Jet Propulsion Laboratory/California Institute of Technology, Mail Stop 301-170S 4800 Oak Grove Drive, Pasadena, CA 91109 United States
AU: Shirley, J H
EM: james.h.shirley@jpl.nasa.gov
AF: Jet Propulsion Laboratory/California Institute of Technology, Mail Stop 301-170S 4800 Oak Grove Drive, Pasadena, CA 91109 United States
AB: The Strategic Road Map for Solar System Exploration recommended in May 2005 that NASA implement the Europa Geophysical Explorer (EGE) as a Flagship mission early in the next decade. This supported the recommendations of the National Research Council's Solar System Decadal Survey and the priorities of the Outer Planets Assessment Group (OPAG). The Europa Geophysical Explorer would: (1) Characterize tidal deformations of the surface of Europa and surface geology, to confirm the presence of a subsurface ocean; (2) Measure the three-dimensional structure and distribution of subsurface water; and (3) Determine surface composition from orbit, and potentially, prebiotic chemistry, in situ. As the next step in Europa exploration, EGE would build on previous Europa Orbiter concepts, for example, the original Europa Orbiter and the Jupiter Icy Moons Orbiter (JIMO). As well, a new set of draft Level One Requirements, provided by NASA sponsors, guided the concept development. These requirements included: (1) Earliest Launch: 2012; (2) Launch Vehicle: Delta IV Heavy or Atlas V; (3) Primary Propulsion: Chemical; (4) Power: Radioisotope Power System (RPS); (4) Orbital Mission: 30 days minimum to meet orbital science objectives; and (5) Earth Gravity Assists: Allowed. The previous studies and the new requirements contributed to the development of several scientifically capable and relatively mass-rich mission options. In particular, Earth-gravity assists (EGA) were allowed, resulting in an increased delivered mass. As well, there have been advances in radiation-hardened components and subsystems, due to the investments from the X-2000 technology program and JIMO. Finally, developments in radioisotope power systems (RPS) have added to the capability and reliability of the mission. Several potential mission options were explored using a variety of trade study methods, ranging from the work of the JPL EGE Team of scientists and engineers in partnership with the OPAG Europa Sub-Group Advisory Team, JPL's Team X, and parametric modeling and simulation tools. We explored the system impacts of selecting different science payloads, power systems, mission durations, Deep Space Network (DSN) architectures, trajectory types, and launch vehicles. The comparisons show that there are feasible mission options that provide potentially available mass for enhanced spacecraft margins and science return, in addition to a 150-kg orbiter science instrument payload mass. This presentation describes high-priority science objectives for an EGE mission, results of the recent studies, and implementation options.
DE: 6221 Europa
DE: 6297 Instruments and techniques
SC: Planetary Sciences [P]
MN: Fall Meeting 2005