Template talk:Earth orbits

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v=
\sqrt{\mu\left({2\over{r}}-{1\over{a}}\right)}

T = 2\pi\sqrt{a^3/\mu}

\epsilon = -{\mu \over{2a}}\,\!

where

μ= 398,600 km3s-2 (standard gravitational parameter for the Earth)

a\,\! is semi-major axis of the orbiting body.

Calculation examples:

The largest speed occurs in the orbit with the distance to the center of the earth ranging from the minimum to the maximum; the semi-major axis is the mean value of the two (for the LEO range: 7500 km). In this orbit the largest speed occurs at the lowest altitude.