P11B-2087
The Main-belt Asteroid and NEO Tour with Imaging and Spectroscopy (MANTIS)

Monday, 14 December 2015
Poster Hall (Moscone South)
Andrew Rivkin1, Barbara A Cohen2, Olivier S Barnouin3, Nancy L Chabot1, Carolyn M Ernst4, Rachel L Klima3, Jorn Helbert5, Zoltan Sternovsky6 and The MANTIS team, (1)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (2)NASA Marshall Space Flight Center, Huntsville, AL, United States, (3)JHU Applied Physics Lab, Laurel, MD, United States, (4)The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)German Aerospace Center DLR Berlin, Berlin, Germany, (6)Colorado Univ, Boulder, CO, United States
Abstract:
The asteroids preserve information from the earliest times in solar system history, with compositions in the population reflecting the material in the solar nebula and experiencing a wide range of temperatures. Today they experience ongoing processes, some of which are shared with larger bodies but some of which are unique to their size regime. They are critical to humanity’s future as potential threats, resource sites, and targets for human visitation. However, over twenty years since the first spacecraft encounters with asteroids, they remain poorly understood. The mission we propose here, the Main-belt Asteroid and NEO Tour with Imaging and Spectroscopy (MANTIS), explores the diversity of asteroids to understand our solar system’s past history, its present processes, and future opportunities and hazards.

MANTIS addresses many of NASA’s highest priorities as laid out in its 2014 Science Plan and provides additional benefit to the Planetary Defense and Human Exploration communities via a low-risk, cost-effective tour of the near-Earth and inner asteroid belt. MANTIS visits the materials that witnessed solar system formation and its earliest history, addressing the NASA goal of exploring and observing the objects in the solar system to understand how they formed and evolve. MANTIS measures OH, water, and organic materials via several complementary techniques, visiting and sampling objects known to have hydrated minerals and addressing the NASA goal of improving our understanding of the origin and evolution of life on Earth. MANTIS studies the geology and geophysics of nine diverse asteroids, with compositions ranging from water-rich to metallic, representatives of both binary and non-binary asteroids, and sizes covering over two orders of magnitude, providing unique information about the chemical and physical processes shaping the asteroids, addressing the NASA goal of advancing the understanding of how the chemical and physical processes in our solar system operate, interact, and evolve. Finally, the set of measurements carried out by MANTIS at near-Earth and main-belt asteroids will by definition characterize objects in the solar system that pose threats to Earth or offer resources for human exploration, a final goal in the NASA Science Plan.

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