Publication Date:
2013-08-31
Description:
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.
Keywords:
ASTROPHYSICS
Type:
Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991; p 671-674
Format:
application/pdf
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