Astrometric recovery and follow-up of near-Earth asteroids

Details Astrometric recovery and follow-up of near-Earth asteroids Astrometric recovery and follow-up of near-Earth asteroids

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994p%26ss...42..611t&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 42, no. 8, p. 611-621

Astronomy and Astrophysics

Astronomy

5

Asteroid Belts, Asteroids, Astrometry, Evolution (Development), Orbital Mechanics, Solar System, Stellar Orbits, Charge Coupled Devices, Density Distribution, Sky Surveys (Astronomy), Trajectories

Scientific paper

We discuss the astrometric observation of minor solar system bodies from Victoria with particular reference to 40 recently monitored near-Earth asteroids. The future encounter circumstances over the next 50 years have been calculated for some interesting individuals of this group. 1991 JW, whose orbit is the most similar to Earth's of any sizeable (greater than 0.5 km) asteroid yet discovered, shows appreciable orbital evolution within this time interval.

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