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True anomaly
Summary
- In astronomy, the true anomaly (T\,\!, also written v\ ) is the angle between the direction z-s of periapsis and the current position p of an object on its orbit, measured at the focus s of the ellipse (the point around which the object orbits).
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| | Soundex: T654 ( T6 A54 )
Metaphone: TRNML
Reference
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* This page is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "True anomaly".
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