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In celestial mechanics, true anomaly is an angular parameter that defines the position of a body moving along a Keplerian orbit. It is the angle between the direction of periapsis and the current position of the body, as seen from the main focus of the ellipse (the point around which the object orbits).
Formulas, Overview & Projective parameters and projective anomaly
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anomaly true position displaystyle projective body eccentric orbit orbits mean angular along equation parameters frac two parameter periapsis circular vector
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| True anomaly | is a | angular parameter that defines the position of a body moving along a Keplerian orbit | 0.90 | text |
| True anomaly | related to From state vectors | For | 0.60 | section |
| True anomaly | related to From the eccentric anomaly | The | 0.60 | section |
| True anomaly | related to From the mean anomaly | The | 0.60 | section |
| True anomaly | related to From the mean anomaly | Fourier | 0.60 | section |
| True anomaly | related to From the mean anomaly | Bessel | 0.60 | section |
| True anomaly | related to Radius from true anomaly | The | 0.60 | section |
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