Energy requirements and payload masses for near-Earth objects hazard mitigation

Abstract The effectiveness of various high energy density sources and their coupling coefficients are evaluated in terms of the required payload mass necessary to change the orbit of a Earth-threatening near-Earth object (NEO) by 6 m/s. Included in the analysis are high explosive, high speed projectiles, nuclear explosives and their radiations, high intensity lasers and concentrated solar energy. It is shown that a given velocity change will be equal to the product of the payload energy and the coupling coefficient divided by the mass of the NEO which superficially portrays a linear relationship. Factors upon which the coupling coefficient depends are discussed. An overall review of the sequential process to mitigate a potentially hazardous NEO is presented.

[1]  S. Ostro The Role of Groundbased Radar in Near-Earth-Object Hazard Identification and Mitigation , 1993 .

[2]  B. G. Marsden,et al.  The NEO confirmation page , 1998 .

[3]  G. Maise,et al.  High‐Performance Ultra‐light Nuclear Rockets for Near‐Earth Objects Interaction Missions a , 1997 .

[4]  John L. Remo,et al.  Near-earth objects : the United Nations international conference , 1997 .

[5]  Pasquale M. Sforza,et al.  Propulsion options for missions to near-Earth objects , 1996 .

[6]  John L. Remo,et al.  Ablation scaling laws for laser space debris clearing , 1998, Other Conferences.

[7]  Richard P. Binzel,et al.  Physical Properties of Near-earth Asteroids: Implications for the Hazard Issue , 1994 .

[8]  John L. Remo Policy perspectives from the UN international conference on near-Earth objects , 1996 .

[9]  C. M. Snell,et al.  Momentum Coupling to NEOs , 1997 .

[10]  H. J. Haubold The Issues of Space Debris and Near-Earth Objects at the United Nations , 1998 .

[11]  Pasquale M. Sforza,et al.  Subsurface momentum coupling analysis for near-earth-object orbital management , 1995 .

[12]  B. G. Marsden Overview of Orbits , 1997 .

[13]  John L. Remo High-power-pulsed 1054-nm laser-induced shock pressure and momentum, and energy coupling to iron-nickel and stony meteorites , 1999 .

[14]  J. Greenberg,et al.  Comets as Porous Aggregates of Interstellar Dust , 1997, Annals of the New York Academy of Sciences.

[15]  R. P. Young,et al.  Experimental hypervelocity impact effects on simulated planetesimal materials , 1994 .

[16]  R. Gertsch,et al.  Near‐Earth Resources , 1997 .

[17]  John L. Remo,et al.  Experimental and computational results for 1054-nm laser-induced shock effects in confined meteorite and metallic targets , 2000, SPIE High-Power Laser Ablation.

[18]  Steven J. Ostro,et al.  Radar Reconnaissance of Near‐Earth Objects at the Dawn of the Next Millennium a , 1997 .

[19]  W. Benz,et al.  Disruption of kilometre-sized asteroids by energetic collisions , 1998, Nature.

[20]  John L. Remo,et al.  Neo interaction with nuclear radiation , 1995 .