Two of Kepler's laws of planetary motion applied to Earth are that the radius vector from the Sun to Earth sweeps out equal areas in equal times and that Earth's orbit is an ellipse with the Sun at one focus.One consequence of these laws is that:

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Kepler's first law states that the radius vector from the Sun to a planet sweeps out equal areas in equal times, meaning that the planet moves faster when it is closer to the Sun and slower when it is farther away. Therefore, Earth moves at different orbital speeds at different times of the year because its orbit is not a perfect circle. This is also supported by Kepler's second law, which states that Earth's orbit is an ellipse with the Sun at one focus. The other choices are not consequences of Kepler's laws.

Two of Kepler's Laws of Planetary Motion Applied to Earth