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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
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