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Published online by Cambridge University Press: 13 November 2008
The success of projects aiming at the detection of Earth-like planetsorbiting nearby stars and the physical-chemical characterization ofthe terrestrial planet's atmospheres requires a careful selection ofthe target stars as well as a detailed knowledge of their propertiesand of the stellar environment. Both aspects have to be fulfilled withspecific observations. The conditions of Dome C for astronomicalobservations are very much appropriate to make a significantcontribution to these preparatory observations. Some examples arepresented here, in particular related to high-precision photometry andhigh spatial resolution observations.