Trajectories to the outer planets using aero-gravity assist flybys of Venus and Mars

Details Trajectories to the outer planets using aero-gravity assist flybys of Venus and Mars Trajectories to the outer planets using aero-gravity assist flybys of Venus and Mars

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992asdy.conf.1809b&link_type=abstract

IN: Astrodynamics 1991; Proceedings of the AAS/AIAA Astrodynamics Conference, Durango, CO, Aug. 19-22, 1991. Pt. 3 (A92-43251 18

Astronomy and Astrophysics

Astronomy

Aeroassist, Flyby Missions, Grand Tours, Interplanetary Trajectories, Spacecraft Trajectories, Mars (Planet), Outer Planets Explorers, Planetary Atmospheres, Venus (Planet)

Scientific paper

The trajectory concept used here is to flyby Venus and then Mars with moderately high speeds expecting to use both gravity and aeroassisted (wave rider) turns in the atmospheres of the planets in order to form fast trajectories to the planets beyond Jupiter. The first part of the paper contains a description of the development of earth-Venus-Mars trajectories yielding the required speeds at Mars in the interval 2001 to 2015. The second part consists in identifying cases in which Mars is at the proper longitude for each target and obtaining trajectories. Trajectories to Saturn, Uranus, Neptune, and Pluto have been found.

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