Where Can We Find Super-Earths?

In recent years we have been witnessing the discovery of one extrasolar gas giant after another. Now the time has come to detect more low-mass planets like super-Earths and Earth-like objects. An interesting question to ask is: where should we look for them? We explore here the possibility of finding super-Earths in the close vicinity of gas giants, as a result of the early evolution of planetary systems. For this purpose, we have considered a young planetary system containing a super-Earth and a gas giant, both embedded in a protoplanetary disc. We have shown that, if the super-Earth is on the internal orbit relative to the gas giant, the planets can easily become locked in a mean motion resonance. This is no longer true, however, if the super-Earth is on the external orbit. In this case we have obtained that the low-mass planet is captured in a trap at the outer edge of the gap opened by the giant planet and no first order mean motion commensurabilities are expected. Our investigations might be particularly useful for the observational transit timing variation (TTV) technique.