Kepler's equation oor Fins
Kepler's equation
en
(mathematics, astronomy) the mathematical relationship between the mean anomaly (M) and the eccentric anomaly (E) of a planet in an elliptical orbit with eccentricity ( \textstyle \epsilon ). M = E - \epsilon \cdot \sin(E).
Vertalings in die woordeboek Engels - Fins
Keplerin yhtälö
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This mean position is refined by Kepler's equation to produce the true position.
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An initial 8-minute burn of the upper stage injected it, with Johannes Kepler, into a low orbit inclined at 51.6 degrees to the equator.
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2 sinne gevind in 2 ms. Hulle kom uit baie bronne en word nie nagegaan nie.