On the dynamical structure of the Trojan group of asteroids

Details On the dynamical structure of the Trojan group of asteroids On the dynamical structure of the Trojan group of asteroids

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acm..proc..671z&link_type=abstract

In Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991 p 671-674 (SEE N93-19113 06-90)

Physics

Asteroids, Librational Motion, Motion Stability, Eccentricity, Frequency Distribution, Inclination

Scientific paper

Using a semi-analytical approach, domains of possible motion for Trojan
asteroids were established. It is shown that stable librating motion is
possible for both high inclination and high eccentricity. Frequency
distributions were also produced for real Trojan asteroids, against
differing libration amplitudes and libration periods.

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