Kepler's First Law: Elliptical Orbits

Kepler's First Law of Planetary Motion

Law of Elliptical Orbits

Orbit Parameters

0.50
5.0 units
1.0x

Kepler's First Law

Law of Orbits: All planets move in elliptical orbits with the Sun situated at one of the foci.

The ellipse is defined by its semi-major axis (a) and eccentricity (e). The closest point to the Sun is called perihelion, and the farthest point is aphelion.

Eccentricity ranges from 0 (perfect circle) to nearly 1 (highly elongated ellipse).

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