Secular evolution of the orbit distance and asteroid hazard

Details Secular evolution of the orbit distance and asteroid hazard Secular evolution of the orbit distance and asteroid hazard

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1472g&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1472

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Computation

Scientific paper

We introduce two methods to estimate an interval J of possible future crossing times between the orbit of an asteroid and the one of the Earth. They are based on the computation of the secular evolution of the orbit distance [4]. With the results of this work we can compile a priority list of asteroids to be processed to assess their collision risk with our planet.

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