OrbitalElementsConvertTimeFromPeriapsisToEccentricAnomaly Method |
Converts the time from periapsis passage to eccentric anomaly. The value returned is signed and monotonic even for periodic orbits.
Namespace:
AGI.Foundation.Coordinates
Assembly:
AGI.Foundation.Core (in AGI.Foundation.Core.dll) Version: 24.2.419.0 (24.2.419.0)
Syntax public static double ConvertTimeFromPeriapsisToEccentricAnomaly(
double timeFromPeriapsis,
double radiusOfPeriapsis,
double eccentricity,
double gravitationalParameter
)
Public Shared Function ConvertTimeFromPeriapsisToEccentricAnomaly (
timeFromPeriapsis As Double,
radiusOfPeriapsis As Double,
eccentricity As Double,
gravitationalParameter As Double
) As Double
public:
static double ConvertTimeFromPeriapsisToEccentricAnomaly(
double timeFromPeriapsis,
double radiusOfPeriapsis,
double eccentricity,
double gravitationalParameter
)
static member ConvertTimeFromPeriapsisToEccentricAnomaly :
timeFromPeriapsis : float *
radiusOfPeriapsis : float *
eccentricity : float *
gravitationalParameter : float -> float
Parameters
- timeFromPeriapsis
- Type: SystemDouble
The time from periapsis passage (time). - radiusOfPeriapsis
- Type: SystemDouble
The radius of periapsis (distance). - eccentricity
- Type: SystemDouble
The eccentricity of the orbit. - gravitationalParameter
- Type: SystemDouble
The gravitational parameter (distance cubed per time squared).
Return Value
Type:
DoubleThe eccentric anomaly.
Exceptions Exception | Condition |
---|
ArgumentOutOfRangeException | Thrown when eccentricity is greater than or equal to one (indicating that the orbit is not closed), or if it is negative, or radiusOfPeriapsis or gravitationalParameter is negative or zero. |
ArithmeticException | Thrown when the iterative solution to Kepler's equation did not converge for elliptic or hyperbolic orbits. |
See Also