A suggested trajectory for a Venus-sun, earth-sun Lagrange points mission, Vela

Astronomy and Astrophysics – Astronomy

Scientific paper

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Asteroids, Interplanetary Trajectories, Lagrangian Equilibrium Points, Mission Planning, Planetary Orbits, Vela Satellites, Astronomical Models, Ecliptic, Flight Optimization, Graphs (Charts), Orbital Mechanics, Trajectory Analysis, Venus (Planet)

Scientific paper

The possibility is suggested of investigating the existence of small, as-yet undiscovered, asteroids orbiting in the solar system near the earth-sun or Venus-sun stable Lagrange points by means of a spacecraft which traverses these regions. The type of trajectory suggested lies in the ecliptic plane and has a period of 5/6 years and a perihelion at the Venus orbital distance. The regions in which stable orbits associated with the earth and with Venus may lie are estimated to be a thin and tadpole-shaped area extending from 35 deg to 100 deg from the planet. Crossings of the regions by the trajectory are described, and the requirements for detecting the presence of 1 km sized asteroids are presented and shown to be attainable.

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