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BILLIARDS: A Demonstration Mission for Hundred-Meter Class Near-Earth Asteroid DisruptionCollisions from near-Earth asteroids (NEAs) have the potential to cause widespread harm to life on Earth. The hypervelocity nature of these collisions means that a relatively small asteroid (about a quartermile in diameter) could cause a global disaster. Proposed strategies for deflecting or disrupting such a threatening asteroid include detonation of a nuclear explosive device (NED) in close proximity to the asteroid, as well as intercepting the asteroid with a hypervelocity kinetic impactor. NEDs allow for the delivery of large amounts of energy to a NEA for a given mass launched from the Earth, but have not yet been developed or tested for use in deep space. They also present safety and political complications, and therefore may only be used when absolutely necessary. Kinetic impactors require a relatively simple spacecraft compared to NEDs, but also deliver a much lower energy for a given launch mass. To date, no demonstration mission has been conducted for either case, and such a demonstration mission must be conducted prior to the need to utilize them during an actual scenario to ensure that an established, proven system is available for planetary defense when the need arises. One method that has been proposed to deliver a kinetic impactor with impact energy approaching that of an NED is the "billiard-ball" approach. This approach would involve capturing an asteroid approximately ten meters in diameter with a relatively small spacecraft (compared to the launch mass of an equivalent direct kinetic impactor), and redirecting it into the path of an Earth-threatening asteroid. This would cause an impact which would disrupt the Earth-threatening asteroid or deflect it from its Earth-crossing trajectory. The BILLIARDS Project seeks to perform a demonstration of this mission concept in order to establish a protocol that can be used in the event of an impending Earth/asteroid collision. In order to accomplish this objective, the mission must (1) rendezvous with a small (less than 10m), NEA (hereinafter "Alpha"), (2) maneuver Alpha to a collision with a approx. 100 m NEA (hereinafter "Beta"), and (3) produce a detectable deflection or disruption of Beta. In addition to these primary objectives, the BILLIARDS project will contribute to the scientific understanding of the physical properties and collision dynamics of asteroids, and provide opportunities for international collaboration.
Document ID
20150022449
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Marcus, Matthew
(Maryland Univ. College Park, MD, United States)
Sloane, Joshua
(Maryland Univ. College Park, MD, United States)
Ortiz, Oliver
(Maryland Univ. College Park, MD, United States)
Barbee, Brent William
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Date Acquired
December 8, 2015
Publication Date
April 13, 2015
Subject Category
Space Sciences (General)
Lunar And Planetary Science And Exploration
Report/Patent Number
GSFC-E-DAA-TN22363
Report Number: GSFC-E-DAA-TN22363
Meeting Information
Meeting: IAA Planetary Defense Conference
Location: Frascati
Country: Italy
Start Date: April 13, 2015
End Date: April 17, 2015
Sponsors: International Academy of Astronautics
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
Asteroid
Asteroid Redirection
Planetary Defense
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