Planetary Defense Mission Using Guided Collision of Near-Earth Objects
The Baseline Instrumented Lithology Lander, Inspector, and Asteroid Redirection Demonstration System is a proposed demonstration mission to characterize a small asteroid less than 10 m in diameter and redirect it to collide with a larger asteroid hundreds of meters in diameter. This collision will d...
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Veröffentlicht in: | Journal of spacecraft and rockets 2017-09, Vol.54 (5), p.985-992 |
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creator | Marcus, Matthew L Sloane, Joshua B Ortiz, Oliver B Barbee, Brent W |
description | The Baseline Instrumented Lithology Lander, Inspector, and Asteroid Redirection Demonstration System is a proposed demonstration mission to characterize a small asteroid less than 10 m in diameter and redirect it to collide with a larger asteroid hundreds of meters in diameter. This collision will disrupt the larger asteroid or alter its trajectory, thereby demonstrating a capability to prevent such an asteroid from colliding with Earth. The concept of redirecting a smaller asteroid into a larger asteroid is attractive for this type of mission because it uses natural kinetic energy available beyond Earth’s gravity well for the majority of the energy delivered to the larger asteroid. By contrast, a kinetic impactor launched directly from Earth to its target must have all of its mass lifted out of Earth’s gravity well. The proposed architecture allows for an impact energy of several terajoules without the use of nuclear devices. This work presents a novel approach to this type of kinetic impactor mission. In the proposed concept of operations, a spacecraft performs a controlled rendezvous and capture of the smaller asteroid. It then uses solar electric propulsion to redirect the asteroid over time onto a collision course. A high-thrust terminal guidance system is used to perform final trajectory adjustments in the hours leading to collision with the larger asteroid, ensuring a successful interception. |
doi_str_mv | 10.2514/1.A33753 |
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This collision will disrupt the larger asteroid or alter its trajectory, thereby demonstrating a capability to prevent such an asteroid from colliding with Earth. The concept of redirecting a smaller asteroid into a larger asteroid is attractive for this type of mission because it uses natural kinetic energy available beyond Earth’s gravity well for the majority of the energy delivered to the larger asteroid. By contrast, a kinetic impactor launched directly from Earth to its target must have all of its mass lifted out of Earth’s gravity well. The proposed architecture allows for an impact energy of several terajoules without the use of nuclear devices. This work presents a novel approach to this type of kinetic impactor mission. In the proposed concept of operations, a spacecraft performs a controlled rendezvous and capture of the smaller asteroid. It then uses solar electric propulsion to redirect the asteroid over time onto a collision course. 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Published by the American Institute of Aeronautics and Astronautics, Inc., with permission. All requests for copying and permission to reprint should be submitted to CCC at ; employ the ISSN (print) or (online) to initiate your request. See also AIAA Rights and Permissions .</rights><rights>Copyright © 2017 by Matthew Marcus, Joshua Sloane, Oliver Ortiz, and Brent Barbee. Published by the American Institute of Aeronautics and Astronautics, Inc., with permission. All requests for copying and permission to reprint should be submitted to CCC at www.copyright.com; employ the ISSN 0022-4650 (print) or 1533-6794 (online) to initiate your request. 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source | Alma/SFX Local Collection |
subjects | Asteroid deflection Collision dynamics Earth gravitation Energy consumption Gravitation Interception Kinetic energy Lithology Measuring instruments Near-Earth Objects Nuclear devices Planetary defense Solar electric propulsion Space rendezvous Terminal guidance Trajectories |
title | Planetary Defense Mission Using Guided Collision of Near-Earth Objects |
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