Significance The Solar System planets have near-circular orbits (i.e., unusually low eccentricity) compared with the known population of exoplanets, planets that orbit stars other than the Sun. This fact has been widely interpreted to indicate that the Solar System is an atypical member of the overall population of planetary systems. We find a strong anticorrelation of orbital eccentricity with the number of planets (multiplicity) in a system that extrapolates nicely to the eight-planet, Solar System case despite the fact that no more than two Solar System planets would be detectable in the sample in which the anticorrelation was discovered. Habitability may be more common in systems with a larger number of planets, which have lower typical eccentricities.