As a planet's distance from its star increases, its orbital period lengthens, in accordance with Kepler's Third Law.
What is this relationship?
The slight variations in the ratio are likely due to the eccentricity of the orbits and the limitations of rounding in the given data. In an ideal Keplerian orbit, these ratios would be exactly the same, but in real planetary systems, there can be small deviations due to various factors, such as the gravitational influence of other planets and the shape of the orbit.
Overall, the relationship between a planet's mean distance from the star and its period of revolution in the Kepler-11 star system is that they are related in a predictable manner where the period of revolution grows with the mean distance from the star, following the pattern described by Kepler's Third Law.
Complete question:
The table shows data for the six planets in the Kepler-11 star system.
Kepler-11 is one of many star systems discovered by space satellites. Scientists find this system unusual because of its small size and its six planets, identified by letters b through g, that orbit relatively close to its central star. The central star, Kepler-11, has a surface temperature of 5663 K and a luminosity of 1.0.
9. Describe the relationship between a planet’s mean distance from this star and the period of revolution.