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








References

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

Comment or add more code

If you cannot find the formula or calculator you want, please tell us what you want and we will add it for you ASAP. If you want anything else or find any error on this page, please just let us know. If you know the formula in other languages, you are welcome to add it. Thanks for contributing to wikicalculator.com!
Please help us do better by providing your opinions(<= 500 characters):
Language:(<= 500 characters)