public final class KeplerianOrbit extends Orbit
The parameters used internally are the keplerian elements (see KeplerianParameters
for more information.
The instance KeplerianOrbit
is guaranteed to be immutable.
Orbit
,
CircularOrbit
,
CartesianOrbit
,
EquinoctialOrbit
,
Serialized FormConstructor and Description |
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KeplerianOrbit(double a,
double e,
double i,
double pa,
double raan,
double anomaly,
PositionAngle type,
Frame frame,
AbsoluteDate date,
double mu)
Creates a new instance.
|
KeplerianOrbit(IOrbitalParameters parametersIn,
Frame frame,
AbsoluteDate date)
Creates a new instance.
|
KeplerianOrbit(Orbit op)
Constructor from any kind of orbital parameters.
|
KeplerianOrbit(PVCoordinates pvCoordinates,
Frame frame,
AbsoluteDate date,
double mu)
Constructor from cartesian parameters.
|
Modifier and Type | Method and Description |
---|---|
protected double[][] |
computeJacobianEccentricWrtCartesian()
Compute the Jacobian of the orbital parameters with eccentric angle with respect to the Cartesian parameters.
|
protected double[][] |
computeJacobianMeanWrtCartesian()
Compute the Jacobian of the orbital parameters with mean angle with respect to the Cartesian parameters.
|
protected double[][] |
computeJacobianTrueWrtCartesian()
Compute the Jacobian of the orbital parameters with true angle with respect to the Cartesian parameters.
|
boolean |
equals(Object object)
Test for the equality of two orbits.
|
double |
getA()
Get the semi-major axis.
|
double |
getAnomaly(PositionAngle type)
Get the anomaly.
|
double |
getE()
Get the eccentricity.
|
double |
getEccentricAnomaly()
Get the eccentric anomaly.
|
double |
getEquinoctialEx()
Get the first component of the equinoctial eccentricity vector.
|
double |
getEquinoctialEy()
Get the second component of the equinoctial eccentricity vector.
|
double |
getHx()
Get hx = ix / (2 * cos(i/2)), where ix is the first component of the inclination vector.
|
double |
getHy()
Get hy = iy / (2 * cos(i/2)), where iy is the second component of the inclination vector.
|
double |
getI()
Get the inclination.
|
KeplerianParameters |
getKeplerianParameters()
Getter for underlying keplerian parameters.
|
double |
getLE()
Get the eccentric longitude argument.
|
double |
getLM()
Get the mean longitude argument.
|
double |
getLv()
Get the true longitude argument.
|
double |
getMeanAnomaly()
Get the mean anomaly.
|
double |
getN()
Get the mean motion.
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IOrbitalParameters |
getParameters()
Get underlying orbital parameters.
|
double |
getPerigeeArgument()
Get the perigee argument.
|
double |
getRightAscensionOfAscendingNode()
Get the right ascension of the ascending node.
|
double |
getTrueAnomaly()
Get the true anomaly.
|
OrbitType |
getType()
Get the orbit type.
|
int |
hashCode()
Get a hashCode for the orbit.
|
protected PVCoordinates |
initPVCoordinates()
Compute the position/velocity coordinates from the canonical parameters.
|
KeplerianOrbit |
interpolate(AbsoluteDate date,
Collection<Orbit> sample)
Get an interpolated instance.
|
protected KeplerianOrbit |
orbitShiftedBy(double dt)
Get a time-shifted orbit.
|
String |
toString() |
createInverseJacobian, ensurePseudoInertialFrame, fillHalfRow, fillHalfRow, fillHalfRow, fillHalfRow, fillHalfRow, fillHalfRow, getDate, getFrame, getJacobian, getJacobian, getJacobian, getJacobian, getJacobianWrtCartesian, getJacobianWrtParameters, getJacobianWrtParametersEccentric, getJacobianWrtParametersMean, getJacobianWrtParametersTrue, getKeplerianMeanMotion, getKeplerianPeriod, getKeplerianTransitionMatrix, getMu, getNativeFrame, getPVCoordinates, getPVCoordinates, getPVCoordinates, setJacobianWrtParametersEccentric, setJacobianWrtParametersMean, setJacobianWrtParametersTrue, shiftedBy
public KeplerianOrbit(IOrbitalParameters parametersIn, Frame frame, AbsoluteDate date)
parametersIn
- orbital parametersframe
- the frame in which the parameters are defineddate
- date of the orbital parameterspublic KeplerianOrbit(double a, double e, double i, double pa, double raan, double anomaly, PositionAngle type, Frame frame, AbsoluteDate date, double mu)
a
- semi-major axis (m), negative for hyperbolic orbitse
- eccentricity (e >= 0)i
- inclination (rad)pa
- perigee argument (ω, rad)raan
- right ascension of ascending node (Ω, rad)anomaly
- mean, eccentric or true anomaly (rad)type
- type of anomalyframe
- the frame in which the parameters are defineddate
- date of the orbital parametersmu
- central attraction coefficient (m3/s2)IllegalArgumentException
- if a and e don't match for hyperbolic orbits,
or v is out of range for hyperbolic orbitspublic KeplerianOrbit(PVCoordinates pvCoordinates, Frame frame, AbsoluteDate date, double mu)
pvCoordinates
- the PVCoordinates of the satelliteframe
- the frame in which are defined the PVCoordinates
date
- date of the orbital parametersmu
- central attraction coefficient (m3/s2)public KeplerianOrbit(Orbit op)
op
- orbital parameters to copypublic IOrbitalParameters getParameters()
getParameters
in class Orbit
public KeplerianParameters getKeplerianParameters()
public OrbitType getType()
public double getA()
Note that the semi-major axis is considered negative for hyperbolic orbits.
public double getE()
public double getI()
public double getPerigeeArgument()
public double getRightAscensionOfAscendingNode()
public double getAnomaly(PositionAngle type)
type
- type of the anglepublic double getTrueAnomaly()
public double getEccentricAnomaly()
public double getMeanAnomaly()
public double getEquinoctialEx()
getEquinoctialEx
in class Orbit
public double getEquinoctialEy()
getEquinoctialEy
in class Orbit
public double getHx()
public double getHy()
public double getLv()
public double getLE()
public double getLM()
public double getN()
protected PVCoordinates initPVCoordinates()
initPVCoordinates
in class Orbit
protected KeplerianOrbit orbitShiftedBy(double dt)
The orbit can be slightly shifted to close dates. This shift is based on a simple keplerian model. It is not intended as a replacement for proper orbit and attitude propagation but should be sufficient for small time shifts or coarse accuracy.
orbitShiftedBy
in class Orbit
dt
- time shift in secondspublic KeplerianOrbit interpolate(AbsoluteDate date, Collection<Orbit> sample)
Note that the state of the current instance may not be used in the interpolation process, only its type and non interpolable fields are used (for example central attraction coefficient or frame when interpolating orbits). The interpolable fields taken into account are taken only from the states of the sample points. So if the state of the instance must be used, the instance should be included in the sample points.
The interpolated instance is created by polynomial Hermite interpolation on Keplerian elements, without derivatives (which means the interpolation falls back to Lagrange interpolation only).
date
- interpolation datesample
- sample points on which interpolation should be doneprotected double[][] computeJacobianMeanWrtCartesian()
Element jacobian[i][j]
is the derivative of parameter i of the orbit with respect to Cartesian coordinate
j. This means each row correspond to one orbital parameter whereas columns 0 to 5 correspond to the Cartesian
coordinates x, y, z, xDot, yDot and zDot.
computeJacobianMeanWrtCartesian
in class Orbit
Orbit.computeJacobianEccentricWrtCartesian()
,
Orbit.computeJacobianTrueWrtCartesian()
protected double[][] computeJacobianEccentricWrtCartesian()
Element jacobian[i][j]
is the derivative of parameter i of the orbit with respect to Cartesian coordinate
j. This means each row correspond to one orbital parameter whereas columns 0 to 5 correspond to the Cartesian
coordinates x, y, z, xDot, yDot and zDot.
computeJacobianEccentricWrtCartesian
in class Orbit
Orbit.computeJacobianMeanWrtCartesian()
,
Orbit.computeJacobianTrueWrtCartesian()
protected double[][] computeJacobianTrueWrtCartesian()
Element jacobian[i][j]
is the derivative of parameter i of the orbit with respect to Cartesian coordinate
j. This means each row correspond to one orbital parameter whereas columns 0 to 5 correspond to the Cartesian
coordinates x, y, z, xDot, yDot and zDot.
computeJacobianTrueWrtCartesian
in class Orbit
Orbit.computeJacobianMeanWrtCartesian()
,
Orbit.computeJacobianEccentricWrtCartesian()
public boolean equals(Object object)
Orbits are considered equals if they have the same type and all their attributes are equals. In particular, the orbits frame are considered equals if they represent the same instance. If they have the same attributes but are not the same instance, the method will return false.
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