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Trojan asteroids are minor planets that share the orbit of a planet about theSun and librate around the L4 or L5 Lagrangian points of stability. They areimportant because they carry information on early Solar System formation, whencollisions between bodies were more frequent. Discovery and study ofterrestrial planet Trojans will help constrain models for the distribution ofbodies and interactions in the inner Solar System.  We present models that constrain optimal search areas, and strategies forsurvey telescopes to maximize the probability of detecting inner planetTrojans. We also consider implications for detection with respect to the Gaiasatellite, and limitations of Gaia's observing geometry.

Search strategies for Trojan asteroids in the inner Solar System