Abstract
In this paper we considered the Mars–Jupiter system to study the behaviour of Near Earth Asteroids (NEAs) as most of the NEAs originate in the main asteroid belt located between Mars and Jupiter. The materials obtained from NEAs are very useful for space industrialisation. The variations in orbital parameters, such as eccentricity, inclination, longitude of pericenter and longitude of ascending node of Mars and Jupiter were investigated for a time span of 200,000 years centered on J2000 (January 2000) using secular perturbation theory. We considered the Sun oblateness and studied the effect of Sun oblateness on orbital parameters of Mars and Jupiter. Moreover, we determined the orbital parameters for asteroids moving under the perturbation effect of Mars and Jupiter by using a secular solution of Mars–Jupiter system.
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Vaishwar, A., Kushvah, B.S. & Mishra, D.P. Secular Effect of Sun Oblateness on the Orbital Parameters of Mars and Jupiter. Few-Body Syst 59, 4 (2018). https://doi.org/10.1007/s00601-017-1325-z
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DOI: https://doi.org/10.1007/s00601-017-1325-z