Efficiency-study of obervatories located in the Lagrangian points L4 and L5 (sun-earth system) for improving tajectory calculations of "near earth asteroids"

Sigfried Eggl

01.03.2004 -

Abstract

Regarding the special geometry of two observatories located near the Lagrangian points L4 and L5 of the sun-earth system, new possibilities of trajectory determination arise. These are compared against existing ones, and tested for their feasibility respectively.

Neue Bahnbestimmungsmethoden, die sich aus der speziellen Geometrie der in den Lagrangepunkten L4 und L5 des Systems Erde-Sonne stationierten Observatorien ergeben, werden mit derzeitigen Möglichkeiten verglichen, und auf ihre Tauglichkeit getestet.