Well, that's kind of the point! A more eccentric orbit will tend to give greater wobbles to the parent star, which gives greater doppler shifts for us to detect. This means that we could probably detect slightly lower mass planets in eccentric orbits than we could in circular orbits.<br /><br />Most important to detection, however, is the orbital period. Since we need to observe the star over a period of a couple of orbits, planets that orbit within a few days or weeks are a lot easier to find than those that have a longer period, like />10 years.