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First International Conference on MOLDAVIAN RISKS – FROM ...

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<str<strong>on</strong>g>First</str<strong>on</strong>g> <str<strong>on</strong>g>Internati<strong>on</strong>al</str<strong>on</strong>g> <str<strong>on</strong>g>C<strong>on</strong>ference</str<strong>on</strong>g> <strong>on</strong> <strong>MOLDAVIAN</strong> <strong>RISKS</strong> - <strong>FROM</strong> GLOBAL TO LOCAL SCALE<br />

16-19 May 2012, Bacau, Romania<br />

THE HAZARD OF IMPACTS <strong>FROM</strong> SPACE<br />

Michael Purucker<br />

Planetary Geodynamics Laboratory, GSFC/NASA, Greenbelt, MD USA<br />

Corresp<strong>on</strong>ding author: Michael Purucker, Michael.E.Purucker@nasa.gov<br />

Abstract: Near-earth objects (NEOs) have been implicated in mass extincti<strong>on</strong>s in Earth<br />

history. The most recent mass extincti<strong>on</strong> occurred at the End-Cretaceous, and is associated<br />

with the Chixulub impact structure in Mexico and the Deccan traps in India. NEOs<br />

comprise both the much more abundant asteroid comp<strong>on</strong>ent, with orbits between 0.98 and<br />

1.3 astr<strong>on</strong>omical units, and the much rarer cometary comp<strong>on</strong>ent. NASA has now cataloged<br />

90% of NEOs larger than 1 km (civilizati<strong>on</strong> ending) and has begun the task of identifying<br />

those larger than 140 m (city killers). NEOs are identified by earth-based telescope, but an<br />

infra-red space-based telescope in an orbit between the Earth and Venus would offer<br />

superior viewing geometry for these dim objects. NEOs have no substantial gravity well,<br />

and hence are ideal targets for both NASA’s robotic and human explorati<strong>on</strong> program. The<br />

natural history of NEOs suggests that they originate via planetary res<strong>on</strong>ances from the<br />

main asteroid belt and the trans-Neptunian disk, and that their dynamical lifetimes are <strong>on</strong><br />

the order of 10 Myr. Once identified, their threat can be assessed via precise orbit<br />

determinati<strong>on</strong>, and steps might be c<strong>on</strong>sidered to re-direct them away from Earth. However,<br />

the complex interacti<strong>on</strong> of science, psychology, politics, and m<strong>on</strong>ey has hindered attempts<br />

at an integrated global approach to the problem. The threat from NEOs was much more<br />

comm<strong>on</strong> in the deep past, in what is termed the Late heavy bombardment 4 billi<strong>on</strong> years<br />

ago. This is a period when most of the Mo<strong>on</strong>’s largest impact basins were formed, and by<br />

inference the largest impact basins <strong>on</strong> Mercury and Mars.<br />

Key words: impacts, hazard, extincti<strong>on</strong>, planetary defense.<br />

16

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