orbital eccentricity
eccentricity

The orbital eccentricity is slightly lower than that of Mars.

This large range arises from the planet's high orbital eccentricity.

This effect can be shown to reduce orbital eccentricities.

It has an orbital eccentricity of 0.08, meaning that its orbit is very circular.

One reason for this stability is its low orbital eccentricity, .

The orbital eccentricity is about the same as Mars.

Such a violent beginning would also explain Titan's orbital eccentricity.

He also initially estimated the orbital eccentricity as 0.027.

At the time, it had the highest orbital eccentricity of any known extrasolar planet.

None of the planets display a significant orbital eccentricity.

It has the most orbital eccentricity orbit around Saturn.

Additionally, Kepler-12b has an almost totally circular orbit, with an orbital eccentricity of less than 0.01.

This object has a low orbital eccentricity and inclination.

This planet is a so-called eccentric Jupiter with an orbital eccentricity of 0.465.

Jupiter, in comparison, orbits the Sun with an orbital eccentricity of 0.016, which is far more circular.

Its primary mission is to study the effects of orbital eccentricity through the Earth's gravity gradient.

The asteroid has a relatively circular orbit, as its measured orbital eccentricity is 0.0933138.

The two stars orbit each other over a period of slightly more than eight days with an orbital eccentricity of about 0.5.

The point around which they librate is the same, irrespective of their mass or orbital eccentricity.

Taking interactions between the planets into account results in a near-zero orbital eccentricity.

These gaps are more sparingly populated with objects of higher orbital eccentricity.

Because of orbital eccentricity, the length of the solar day is not quite constant.

Conservation of L means that orbital eccentricity can be "traded for" inclination.

The residual precession is greater the closer the planet to the Sun and the larger its orbital eccentricity.

These corresponds to the orbital eccentricity of 0.48.