org.orekit.bodies

Class CR3BPSystem

java.lang.Object

org.orekit.bodies.CR3BPSystem

public class CR3BPSystem
extends Object

Class creating, from two different celestial bodies, the corresponding system with respect to the Circular Restricted Three Body problem hypotheses.

Since:

10.2

Author:

Vincent Mouraux, William Desprats

See Also:

"Dynamical systems, the three-body problem, and space mission design, Koon, Lo, Marsden, Ross"

Constructor Summary

Constructors

Constructor and Description
CR3BPSystem(CelestialBody primaryBody, CelestialBody secondaryBody, double a) Simple constructor.
CR3BPSystem(CelestialBody primaryBody, CelestialBody secondaryBody, double a, double mu) Simple constructor.

Method Summary

Modifier and Type	Method and Description
double	getDdim() Get the CR3BP distance between the two bodies.
double	getGamma(LagrangianPoints lagrangianPoint) Get the position of the Lagrangian point in the CR3BP Rotating frame.
Vector3D	getLPosition(LagrangianPoints lagrangianPoint) Get the position of the Lagrangian point in the CR3BP Rotating frame.
double	getMassRatio() Get the CR3BP mass ratio of the system mu2/(mu1+mu2).
String	getName() Get the name of the CR3BP system.
CelestialBody	getPrimary() Get the primary CelestialBody.
AbsolutePVCoordinates	getRealAPV(AbsolutePVCoordinates apv0, AbsoluteDate initialDate, Frame outputFrame) Get the AbsolutePVCoordinates from normalized units to standard units in an output frame.
Frame	getRotatingFrame() Get the CR3BP Rotating Frame.
CelestialBody	getSecondary() Get the secondary CelestialBody.
double	getTdim() Get the CR3BP orbital period of m2 around m1.
double	getVdim() Get the CR3BP orbital velocity of m2.

Methods inherited from class java.lang.Object

clone, equals, finalize, getClass, hashCode, notify, notifyAll, toString, wait, wait, wait

Constructor Detail

CR3BPSystem

public CR3BPSystem(CelestialBody primaryBody,
                   CelestialBody secondaryBody,
                   double a)

Simple constructor.

Standard constructor to use to define a CR3BP System. Mass ratio is calculated from JPL data.

Parameters:

primaryBody - Primary Body in the CR3BP System

secondaryBody - Secondary Body in the CR3BP System

a - Semi-Major Axis of the secondary body

CR3BPSystem

public CR3BPSystem(CelestialBody primaryBody,
                   CelestialBody secondaryBody,
                   double a,
                   double mu)

Simple constructor.

This constructor can be used to define a CR3BP System if the user wants to use a specified mass ratio.

Parameters:

primaryBody - Primary Body in the CR3BP System

secondaryBody - Secondary Body in the CR3BP System

a - Semi-Major Axis of the secondary body

mu - Mass ratio of the CR3BPSystem

Method Detail

getMassRatio

public double getMassRatio()

Get the CR3BP mass ratio of the system mu2/(mu1+mu2).

Returns:

CR3BP mass ratio of the system mu2/(mu1+mu2)

getDdim

public double getDdim()

Get the CR3BP distance between the two bodies.

Returns:

CR3BP distance between the two bodies(m)

getVdim

public double getVdim()

Get the CR3BP orbital velocity of m2.

Returns:

CR3BP orbital velocity of m2(m/s)

getTdim

public double getTdim()

Get the CR3BP orbital period of m2 around m1.

Returns:

CR3BP orbital period of m2 around m1(s)

getName

public String getName()

Get the name of the CR3BP system.

Returns:

name of the CR3BP system

getPrimary

public CelestialBody getPrimary()

Get the primary CelestialBody.

Returns:

primary CelestialBody

getSecondary

public CelestialBody getSecondary()

Get the secondary CelestialBody.

Returns:

secondary CelestialBody

getRotatingFrame

public Frame getRotatingFrame()

Get the CR3BP Rotating Frame.

Returns:

CR3BP Rotating Frame

getLPosition

public Vector3D getLPosition(LagrangianPoints lagrangianPoint)

Get the position of the Lagrangian point in the CR3BP Rotating frame.

Parameters:

lagrangianPoint - Lagrangian Point to consider

Returns:

position of the Lagrangian point in the CR3BP Rotating frame (-)

getGamma

public double getGamma(LagrangianPoints lagrangianPoint)

Get the position of the Lagrangian point in the CR3BP Rotating frame.

Parameters:

lagrangianPoint - Lagrangian Point to consider

Returns:

Distance between a Lagrangian Point and its closest primary.

getRealAPV

public AbsolutePVCoordinates getRealAPV(AbsolutePVCoordinates apv0,
                                        AbsoluteDate initialDate,
                                        Frame outputFrame)

Get the AbsolutePVCoordinates from normalized units to standard units in an output frame. This method ensure the constituency of the date of returned AbsolutePVCoordinate, especially when apv0 is the result of a propagation in CR3BP normalized model.

Parameters:

apv0 - Normalized AbsolutePVCoordinates in the rotating frame

initialDate - Date of the at the beginning of the propagation

outputFrame - Frame in which the output AbsolutePVCoordinates will be

Returns:

AbsolutePVCoordinates in the output frame [m,m/s]