Originally Posted by DaveC426913
A quick calculation shows that the average eccentricity of our SS's 8 major planets is ~0.0606
while the average of the 345 extrasolar planets with known eccentricities is ~0.2181
or about 3.5 times more eccentric.
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The average does not give the complete picture. If you run the data through a frequency analysis, about 1/3 of the observed eccentricities are less than 0.05 (approximately the solar system average) and around 2/3 are less than 0.2.
The above doesn't take the distance of an exoplanet from its star into account and its conceivable that planets within different AU ranges could show different means. Furthermore, and this is purely conjecture on my part, it is possible that exoplanets with larger eccentricities are the larger gas giants and thus easier to observe. The data may be inherently biased by our current observational limitations.
In any case, if 30% of the observed exoplanets match the solar system average, then the solar system cannot be considered to be that unique.