41st Lunar and Planetary Science Conference (2010) 1633.pdf HALL: A PHOBOS AND DEIMOS SAMPLE RETURN MISSION. Pascal Lee1,2,3, Joseph Veverka4, Julie Bel- lerose5, Marc Boucher1, John Boynton6, Stephen Braham1,7, Ralf Gellert8, Alan Hildebrand9, David Manzella10, Greg Mungas6, Steven Oleson10, Robert Richards11, Peter C. Thomas4, and Michael D. West1,12. 1Mars Institute, 2SETI Institute, 3NASA Ames Research Center,
[email protected], 4Cornell Univ., 5Carnegie Mellon Univ. 6Firestar Engineering, 7Simon Fraser University, 8Univ. of Guelph, 9Univ. of Calgary, 10NASA Glenn Research Cen- ter, 11Optech, 12The Australian National Univ. Introduction: Hall is a proposed NASA-led inter- types of primitive asteroids, but their surfaces also national robotic lander and sample return mission present lateral variations in albedo and color, suggest- (SRM) to explore and return samples from the two ing possible variations in the composition and/or moons of Mars, Phobos and Deimos. The mission will weathering state of their regolith. address the outstanding issues of the origin, nature, and Samples from Phobos and Deimos, if they were to evolution of both Phobos and Deimos, as well as pro- include soils as well, would allow detailed investiga- vide unique insights into early solar system processes, tions of the nature and evolution of their regolith. In planetary formation, and the evolution of Mars itself. this regard, an intriguing prospect is that their regolith Hall is being developed as a New Frontiers-class mis- should include meteoritic signatures from Mars [7-9, 11], asteroids, comets, and interplanetary dust particles sion and will use solar electric propulsion. Hall is (IDPs). Sampling Phobos’s regolith could therefore named after American astronomer Asaph Hall who, in provide access to a wide variety of martian and other 1877, discovered the two moons of Mars.