|  |  | 
   Foreword
 
 
 
  
    | The Earth orbits the Sun in a sort of cosmic shooting
    gallery, subject to impacts from comets and asteroids.
 It is only fairly recently that we have come to appreciate that
    these impacts
 by asteroids and comets (often called Near Earth Objects, or
    NEOs)
 pose a significant hazard to life and property.
 
 Although the annual probability of the Earth being struck
 by a large asteroid or comet is extremely small,
 the consequences of such a collision are so catastrophic
 that it is prudent to assess the nature of the threat and prepare
    to deal with it.
 
 Studies have shown that the risk from cosmic impact increases
 with the size of the projectile.
 The greatest risk is associated with objects large enough to
    perturb
 the Earth's climate on a global scale
 by injecting large quantities of dust into the stratosphere.
 
 Such an event could depress temperatures around the globe,
 leading to massive loss of food crops and possible breakdown
    of society.
 Such global catastrophes are qualitatively different from other
    more common hazards
 that we face (excepting nuclear war), because of their potential
    effect
 on the entire planet and its population.
 
 Various studies have suggested that the minimum mass impacting
    body
 to produce such global consequences is several tens of billions
    of tons,
 resulting in a groundburst explosion with energy
 in the vicinity of a million megatons of TNT.
 The corresponding threshold diameter for NEOs is between 1 and
    2 km.
 Smaller objects (down to tens of meters diameter) can cause severe
    local damage
 but pose no global threat.
 David Morrison
 
 September 1998
 
 |  |