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Title: Astrodynamics Research and Analysis Funding
Primary Author: Nathan J. Strange
Secondary Author(s): Daniel Scheeres, Ryan Russell, Kathleen Howell, James Longuski, Victoria Coverstone, David B. Spencer, Cesar Ocampo, Belinda Marchand, Terry Alfriend, John Junkins, Daniele Mortari, John Crassidis, Landis Markley, David Folta, John Dankanich, Shyam Bhaskaran, Dennis Byrnes, Kim Reh, Martin Lo, Jon Sims, John C. Smith, Brent Buffington, Anastassios Petropoulos, Damon Landau, Fernando Abilleira, Ryan Park, Jeffrey Parker, Julie Bellerose, Stefano Campagnola, Andrew Klesh,
Nitin Arora, Diane Craig Davis, Kevin Kloster, Alfred Lynam, Geoff Wawrzyniak
Institution: Jet Propulsion Laboratory
Date: September 15, 2009
Summary: Funding for astrodynamics research has been largely limited to the development and operations phases of missions. Early funding for astrodynamics research would produce new techniques prior to formulation of missions, which could lead to novel and exciting concepts.
Panel Selection: Inner Planets: Mercury, Venus, and the Moon.
Mars: Not Phobos and Deimos.
Giant Planets: Jupiter, Saturn, Uranus, Neptune, and exoplanets, including rings and magnetic fields, but not their satellites.
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets.
Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust.
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These documents have been prepared in coordination with the National Academies of Science in support of the National Academies Planetary Science Decadal Survey. These documents are being made available for information purposes only, and any views and opinions expressed herein do not necessarily state or reflect those of NASA, JPL, or the California Institute of Technology.