Quantifying the Risk Posed by Potential Earth Impacts

Predictions of future potential Earth impacts by near-Earth objects (NEOs) have become commonplace in recent years, and the rate of these detections is likely to accelerate as asteroid survey efforts continue to mature. In order to conveniently compare and categorize the numerous potential impact solutions being discovered we propose a new hazard scale that will describe the risk posed by a particular potential impact in both absolute and relative terms. To this end, we measure each event in two ways, first without any consideration of the event's time proximity or its significance relative to the so-called background threat, and then in the context of the expected risk from other objects over the intervening years until the impact. This approach is designed principally to facilitate communication among astronomers, and it is not intended for public communication of impact risks. The scale characterizes impacts across all impact energies, probabilities and dates, and it is useful, in particular, when dealing with those cases which fall below the threshold of public interest. The scale also reflects the urgency of the situation in a natural way and thus can guide specialists in assessing the computational and observational effort appropriate for a given situation. In this paper we describe the metrics introduced, and we give numerous examples of their application. This enables us to establish in rough terms the levels at which events become interesting to various parties.

[1]  M. Carpino,et al.  Error statistics of asteroid optical astrometric observations , 2003 .

[2]  Dennis V. Byrnes,et al.  The Discovery and Orbit of 1993 (243)1 Dactyl , 1996 .

[3]  Farquhar,et al.  Estimating the mass of asteroid 253 mathilde from tracking data during the NEAR flyby , 1997, Science.

[4]  J. Rahe,et al.  Properties of Cometary Nuclei , 1994 .

[5]  Patrick Michel,et al.  Dynamics of Eros , 1998 .

[6]  David Morrison,et al.  Impacts on the Earth by asteroids and comets: assessing the hazard , 1994, Nature.

[7]  R. Binzel The Torino Impact Hazard Scale , 2000 .

[8]  S. Chesley,et al.  Asteroid close encounters with Earth: risk assessment , 2000 .

[9]  G. Michalak,et al.  Determination of asteroid masses , 2000 .

[10]  Veverka,et al.  Radio science results during the NEAR-shoemaker spacecraft rendezvous with eros , 2000, Science.

[11]  A. W. Harris The H-G Asteroid Magnitude System: Mean Slope Parameters , 1989 .

[12]  Grzegorz Michalak,et al.  Determination of asteroid masses --- I. (1) Ceres, (2) Pallas and (4) Vesta , 2000 .

[13]  D. Yeomans,et al.  Predicting Close Approaches and Estimating Impact Probabilities for Near Earth Objects , 1999 .

[14]  G. Duvert,et al.  Discovery of a moon orbiting the asteroid 45 Eugenia , 1999, Nature.

[15]  Eugene M. Shoemaker,et al.  ASTEROID AND COMET BOMBARDMENT OF THE EARTH , 1983 .

[16]  P. W. Chodas,et al.  2000 SG344: the story of a potential Earth impactor , 2001 .

[17]  S. Chesley,et al.  Asteroid Close Approaches: Analysis and Potential Impact Detection , 2002 .

[18]  Martin A. Slade,et al.  Radar Observations of Binary Asteroid 2000 DP107 , 2001 .

[19]  Veverka,et al.  Estimating the mass of asteroid 433 eros during the NEAR spacecraft flyby , 1999, Science.

[20]  D. J. Tholen,et al.  Physical properties of Aten, Apollo and Amor asteroids. , 1989 .

[21]  P. Chodas,et al.  Orbit Determination and Estimation of Impact Probability for Near Earth Objects , 1999 .

[22]  E. Opik,et al.  Interplanetary encounters: Close-range gravitational interactions , 1976 .

[23]  Alan W. Harris,et al.  Application of photometric models to asteroids. , 1989 .

[24]  Patrick Michel,et al.  Dynamical evolution of two near-Earth asteroids to be explored by spacecraft: (433) Eros and (4660) Nereus. , 1996 .