solve_kepler_equation
このコンテンツはまだ日本語訳がありません。
Defined in: kepler.rs:25
fn solve_kepler_equation(mean_anomaly: f64, eccentricity: f64) -> f64
Solve Kepler’s equation M = E - e·sin(E) for eccentric anomaly E
using Newton-Raphson iteration.
Arguments
Section titled “Arguments”mean_anomaly- Mean anomaly M [rad]eccentricity- Orbital eccentricity (0 ≤ e < 1)
Returns
Section titled “Returns”Eccentric anomaly E [rad]