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Given the tendency of planets to form in multiples, and the observationalevidence in support of the existence of potential planet-hosting stars inbinaries or clusters, it is expected that extrasolar terrestrial planes aremore likely to be found in multiple body systems. This paper discusses theprospects of the detection of terrestrial/habitable planets in multibodysystems by presenting the results of a study of the long-term stability ofthese objects in systems with multiple giant planets (particularly those ineccentric and/or in mean-motion resonant orbits), systems with close-inJupiter-like bodies, and systems of binary stars. The results of simulationsshow that while short-period terrestrial-class objects that are captured innear mean-motion resonances with migrating giant planets are potentiallydetectable via transit photometry or the measurement of the variations of thetransit-timing due to their close-in Jovian-mass planetary companions, theprospect of the detection of habitable planets with radial velocity techniqueis higher in systems with multiple giant planets outside the habitable zone andbinary systems with moderately separated stellar companions.

The Stability and Prospects of the Detection of Terrestrial/Habitable Planets in Multiplanet and Multiple Star Systems