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# Semi-major axis

From CreationWiki, the encyclopedia of creation science

The **semi-major axis** of any ellipse is one-half of the axis of symmetry that passes through the foci of that ellipse.

In astrophysics, the semi-major axis of an orbit is the distance between the geometric center of the orbit and either apsis. It is a commonly reported orbital element that can determine the size and shape of an orbit.

## Calculations

The semi-major axis, usually labeled *a*, is the arithmetic mean of the two apsides:

a = (Q + q)/2

For this reason the semi-major axis is often cited as a "mean orbital radius."

The semi-major axis, together with the orbital eccentricity (*e*), can predict the periapsis and apoapsis:

Q = a(1+e)

q = a(1-e)

See orbital eccentricity for a detailed derivation.

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