Semi-latus rectum in Kepler's First Law (given polar coordinates )

Formula

Semi-latus rectum in Kepler's First Law (given polar coordinates ) formula
p
the semi-latus rectum
r
the distance from the Sun to the planet
theta
angle with its vertex at the Sun from the location where the planet is closest to the Sun
epsilon
the eccentricity of the ellipse

Formula description

The orbit of every planet is an ellipse with the Sun at one of the two foci.

Calculator (how to use calculator?)

Semi-latus rectum in Kepler's First Law (given polar coordinates ) formula
r
theta
epsilon
p
Precision

Formula code

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References

  1. wikipedia: Semi-latus rectum in Kepler's First Law (Given polar coordinates ).

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