Such objects have relatively low eccentricities (e below 0.2) and orbit the Sun in much the same way the planets do.
This planet orbits 25% further from the star than Earth to the Sun with a low eccentricity.
One reason for this stability is its low orbital eccentricity, .
The planet's orbit has a low eccentricity, like most of the planets in our solar system.
The planet's orbit has a low eccentricity, similar to the planets in our solar system.
The latest models of the system which incorporate four planets give a lower eccentricity orbit.
The mass was only 18 times more than Earth or about same as Neptune with very low eccentricity.
A regime of eccentricity lower than the current value will last for about the next 100,000 years.
Using a statistical computer program, another team reinterpreted the same data for a lower eccentricity of 0.33.
This pair of stars complete an orbit every 3.4280 days and they have a low orbital eccentricity that is close to 0.0.
