Dynamical Characteristics of Hungaria Asteroids

Details Dynamical Characteristics of Hungaria Asteroids Dynamical Characteristics of Hungaria Asteroids

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010pobeo..90...11k&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, vol. 90, pp. 11-18

Astronomy and Astrophysics

Astronomy

Scientific paper

Due to the favorable observing conditions, the Hungaria asteroids may soon become the best known asteroid subgroup of the asteroid population. We have built a large catalog of accurate synthetic proper elements in order to study the dynamical properties of the Hungaria region, both within a purely gravitational model and also accounting for the non-gravitational effects. In the present paper we extend our previous study to more closely investigate the occurrence of close approaches of Hungaria asteroids to Mars, and we present a refined analysis of the dynamics of close couples found in the region.

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