Data Structures
struct	PlanetOBJModel

Public Types
enum	PlanetType { isStar, isPlanet, isMoon, isObserver, isArtificial, isAsteroid, isPlutino, isComet, isDwarfPlanet, isCubewano, isSDO, isOCO, isSednoid, isInterstellar, isUNDEFINED }
	numeric typecodes for the type descriptions in ssystem.ini

enum	PlanetOrbitColorStyle { ocsOneColor, ocsGroups, ocsMajorPlanets }

enum	ApparentMagnitudeAlgorithm { Mueller_1893, AstronomicalAlmanac_1984, ExplanatorySupplement_1992, ExplanatorySupplement_2013, MallamaHilton_2018, UndefinedAlgorithm, Generic }

enum	PositionQuality { Position, OrbitPlotting }
	enums to indicate for which purpose we check positional quality. More...

Public Types inherited from StelObject
enum	InfoStringGroupFlags { None = 0x00000000, Name = 0x00000001, CatalogNumber = 0x00000002, Magnitude = 0x00000004, RaDecJ2000 = 0x00000008, RaDecOfDate = 0x00000010, AltAzi = 0x00000020, Distance = 0x00000040, Elongation = 0x00000080, Size = 0x00000100, Velocity = 0x00000200, ProperMotion = 0x00000400, Extra = 0x00000800, HourAngle = 0x00001000, AbsoluteMagnitude = 0x00002000, GalacticCoord = 0x00004000, SupergalacticCoord = 0x00008000, OtherCoord = 0x00010000, ObjectType = 0x00020000, EclipticCoordJ2000 = 0x00040000, EclipticCoordOfDate = 0x00080000, IAUConstellation = 0x00100000, SiderealTime = 0x00200000, RTSTime = 0x00400000, SolarLunarPosition = 0x00800000, Script = 0x01000000, DebugAid = 0x02000000, NoFont = 0x04000000, PlainText = 0x08000000 }
	Used as named bitfield flags as specifiers to filter results of getInfoString. More...

Public Member Functions
	Planet (const QString &englishName, double equatorialRadius, double oblateness, Vec3f halocolor, float albedo, float roughness, const QString &texMapName, const QString &normalMapName, const QString &objModelName, posFuncType _coordFunc, Orbit anOrbitPtr, OsculatingFunctType osculatingFunc, bool closeOrbit, bool hidden, bool hasAtmosphere, bool hasHalo, const QString &pTypeStr)

virtual QString	getInfoString (const StelCore *core, const InfoStringGroup &flags) const Q_DECL_OVERRIDE
	Get a string with data about the Planet. More...

virtual QVariantMap	getInfoMap (const StelCore *core) const Q_DECL_OVERRIDE
	In addition to the entries from StelObject::getInfoMap(), Planet objects provide. More...

virtual double	getCloseViewFov (const StelCore *core) const Q_DECL_OVERRIDE
	Return the best FOV in degree to use for a close view of the object.

virtual double	getSatellitesFov (const StelCore *core) const Q_DECL_OVERRIDE
	Return the best FOV in degree to use for a global view of the object satellite system (if there are satellites)

virtual double	getParentSatellitesFov (const StelCore *core) const Q_DECL_OVERRIDE

virtual float	getVMagnitude (const StelCore *core) const Q_DECL_OVERRIDE
	Return object's apparent V magnitude as seen from observer, without including extinction.

virtual float	getSelectPriority (const StelCore *core) const Q_DECL_OVERRIDE
	Return a priority value which is used to discriminate objects by priority As for magnitudes, the lower is the higher priority.

virtual Vec3f	getInfoColor (void) const Q_DECL_OVERRIDE
	Get a color used to display info about the object.

virtual QString	getType (void) const Q_DECL_OVERRIDE
	Return object's type. It should be the name of the class.

virtual QString	getObjectType (void) const Q_DECL_OVERRIDE
	Return object's type. It should be English lowercase name of the type of the object.

virtual QString	getObjectTypeI18n (void) const Q_DECL_OVERRIDE
	Return object's type. It should be translated lowercase name of the type of the object.

virtual QString	getID (void) const Q_DECL_OVERRIDE
	Returns a unique identifier for this object. More...

virtual Vec3d	getJ2000EquatorialPos (const StelCore *core) const Q_DECL_OVERRIDE
	A Planet's own eclipticPos is in VSOP87 ref. More...

virtual QString	getEnglishName (void) const Q_DECL_OVERRIDE
	Return object's name in english.

virtual QString	getNameI18n (void) const Q_DECL_OVERRIDE
	Return translated object's name.

QString	getNativeName (void) const

QString	getNativeNameI18n (void) const

QString	getCommonEnglishName (void) const

QString	getCommonNameI18n (void) const

virtual double	getAngularRadius (const StelCore *core) const Q_DECL_OVERRIDE
	Get angular semidiameter, degrees. If planet display is artificially enlarged (e.g. Moon upscale), value will also be increased.

virtual bool	hasAtmosphere (void)

virtual bool	hasHalo (void)

bool	hasValidPositionalData (const double JDE, const PositionQuality purpose) const
	Returns whether planet positions are valid and useful for the current simulation time. More...

Vec2d	getValidPositionalDataRange (const PositionQuality purpose) const
	Returns JDE dates of presumably valid data for positional calculation or acceptable range for graphics. More...

float	getAxisRotation (void)

virtual void	translateName (const StelTranslator &trans)
	return axisRotation last computed in computeTransMatrix(). [degrees] More...

virtual void	draw (StelCore *core, float maxMagLabels, const QFont &planetNameFont)

double	getEquatorialRadius (void) const
	Get the equator radius of the planet in AU. More...

double	getOneMinusOblateness (void) const
	Get the value (1-f) for oblateness f=polarRadius/equatorialRadius.

double	getPolarRadius (void) const
	Get the polar radius of the planet in AU. More...

double	getSiderealDay (void) const
	Get duration of sidereal day (earth days, may come from rot_periode or orbit_period (for moons) from ssystem_*.ini)

virtual double	getSiderealPeriod (void) const
	Get duration of sidereal year [earth days].

void	setSiderealPeriod (const double siderealPeriod)
	set duration of sidereal year. More...

double	getMeanSolarDay (void) const
	Get duration of mean solar day, in earth days.

double	getAlbedo (void) const
	Get albedo.

const QString &	getTextMapName () const

const QString	getPlanetTypeString () const

PlanetType	getPlanetType () const

Orbit *	getOrbit () const

void	setNativeName (QString planet)

void	setNativeNameMeaning (QString planet)

void	setIAUMoonNumber (QString designation)
	set the IAU moon number (designation of the moon), if any.

float	getAbsoluteMagnitude () const
	Return the absolute magnitude (read from file ssystem.ini)

float	getMeanOppositionMagnitude () const
	Return the mean opposition magnitude, defined as V(1,0)+5log10(a(a-1)) A return value of 100 signals invalid result.

double	getSiderealTime (double JD, double JDE) const
	Compute the axial z rotation (daily rotation around the polar axis) [degrees] to use from equatorial to hour angle based coordinates. More...

Mat4d	getRotEquatorialToVsop87 (void) const
	return a rotation matrix from the planet's equatorial coordinate frame to the VSOP87 (ecliptical J2000) frame. More...

void	setRotEquatorialToVsop87 (const Mat4d &m)
	set a rotation matrix from the planet's equatorial coordinate frame to the VSOP87 (ecliptical J2000) frame. More...

const RotationElements &	getRotationElements (void) const

void	setRotationElements (const QString name, const double _period, const double _offset, const double _epoch, const double _obliquity, const double _ascendingNode, const double _ra0, const double _ra1, const double _de0, const double _de1, const double _w0, const double _w1)
	Set the rotational elements. More...

double	getRotAscendingNode (void) const
	Note: The only place where this is used is to build up orbits for planet moons w.r.t. the parent planet orientation.

double	getRotObliquity (double JDE) const
	return angle between axis and normal of ecliptic plane (or, for a moon, equatorial/reference plane defined by parent). More...

virtual void	computePosition (const double dateJDE, const Vec3d &aberrationPush)
	Compute the position and orbital velocity in the parent Planet coordinate system You can add the aberrationPush value according to Edot*lightTime in Explanatory Supplement (2013) formula 7.55.

virtual void	computePosition (const double dateJDE, Vec3d &eclPosition, Vec3d &eclVelocity) const
	Compute the position and orbital velocity in the parent Planet coordinate system, and return them in eclPosition and eclVelocity These may be preferred when we want to avoid setting the actual position (e.g., RTS computation)

void	computeTransMatrix (double JD, double JDE)
	Compute the transformation matrix from the local Planet coordinate to the parent Planet coordinate. More...

Vec4d	getRectangularCoordinates (const double longDeg, const double latDeg, const double altMetres=0.) const
	Retrieve planetocentric rectangular coordinates of a location on the ellipsoid surface, or with altitude altMetres above the ellipsoid surface. More...

double	getPhaseAngle (const Vec3d &obsPos) const
	Get the phase angle (radians) for an observer at pos obsPos in heliocentric coordinates (in AU)

double	getElongation (const Vec3d &obsPos) const
	Get the elongation angle (radians) for an observer at pos obsPos in heliocentric coordinates (in AU)

double	getSpheroidAngularRadius (const StelCore *core) const
	Get the angular radius (degrees) of the planet spheroid (i.e. without the rings)

float	getPhase (const Vec3d &obsPos) const
	Get the planet phase (illuminated fraction of the planet disk, [0=dark..1=full]) for an observer at pos obsPos in heliocentric coordinates (in AU)

QPair< Vec4d, Vec3d >	getSubSolarObserverPoints (const StelCore *core, bool jupiterGraphical=false) const
	Get planetographic coordinates of subsolar and sub-observer points. More...

bool	isRotatingRetrograde () const
	returns if planet has retrograde rotation

Vec3d	getEclipticPos (double dateJDE) const
	Get the Planet position in the parent Planet ecliptic coordinate in AU.

Vec3d	getEclipticPos () const
	Get the last computed Planet position in the parent Planet ecliptic coordinate in AU.

Vec3d	getHeliocentricEclipticPos () const
	Return the heliocentric ecliptical position.

Vec3d	getHeliocentricEclipticPos (double dateJDE) const

Vec3d	getHeliocentricPos (Vec3d p) const
	Return the heliocentric transformation for local (parentocentric) coordinate. More...

void	setHeliocentricEclipticPos (const Vec3d &pos)
	Propagate the heliocentric coordinates to parentocentric coordinates. More...

Vec3d	getEclipticVelocity () const
	Get the planet velocity around the parent planet in ecliptical coordinates in AU/d.

Vec3d	getHeliocentricEclipticVelocity () const
	Get the planet's heliocentric velocity in the solar system in ecliptical coordinates in AU/d. Required for aberration!

double	computeDistance (const Vec3d &obsHelioPos)
	Compute and return the distance to the given position in heliocentric ecliptical (J2000) coordinates (in AU) Preserves result for later retrieval by getDistance() As side effect, improve fps by juggling update frequency (deltaJDE) for asteroids and other minor bodies. More...

double	getDistance (void) const
	Return the last computed distance to the given position in heliocentric ecliptical (J2000) coordinates (in AU)

void	setRings (Ring *r)

void	setSphereScale (double s)

double	getSphereScale () const

const QSharedPointer< Planet >	getParent (void) const

virtual void	update (int deltaTime)

void	setFlagHints (bool b)

bool	getFlagHints (void) const

void	setFlagLabels (bool b)

bool	getFlagLabels (void) const

void	setFlagNativeName (bool b)

bool	getFlagNativeName (void) const

void	setFlagOrbits (bool b)

bool	getFlagOrbits (void) const

void	drawOrbit (const StelCore *)

QVector< const Planet * >	getCandidatesForShadow () const
	Return the list of planets which project some shadow on this planet.

Vec3d	getAberrationPush () const

virtual Vec4d	getRTSTime (const StelCore *core, const double altitude=0.) const Q_DECL_OVERRIDE
	Compute times of nearest rise, transit and set for a solar system object for current location. More...

void	resetTextures ()

void	replaceTexture (const QString &texName)

Public Member Functions inherited from StelObject
virtual SphericalRegionP	getRegion () const Q_DECL_OVERRIDE
	Default implementation of the getRegion method. More...

virtual Vec3d	getPointInRegion () const Q_DECL_OVERRIDE
	Default implementation of the getPointInRegion method. More...

Vec3d	getEquinoxEquatorialPos (const StelCore *core) const
	Get observer-centered equatorial coordinate at the current equinox The frame has its Z axis at the planet's current rotation axis At time 2000-01-01 this frame is almost the same as J2000, but ONLY if the observer is on earth.

Vec3d	getEquinoxEquatorialPosApparent (const StelCore *core) const
	Like getEquinoxEquatorialPos(core), but always adds refraction correction to the position.

Vec3d	getEquinoxEquatorialPosAuto (const StelCore *core) const
	Like getEquinoxEquatorialPos(core), but adds refraction correction to the position if atmosphere is active.

Vec3d	getGalacticPos (const StelCore *core) const
	Get observer-centered galactic coordinates.

Vec3d	getSupergalacticPos (const StelCore *core) const
	Get observer-centered supergalactic coordinates.

Vec3d	getSiderealPosGeometric (const StelCore *core) const
	Get observer-centered hour angle + declination (at current equinox) It is the geometric position, i.e. More...

Vec3d	getSiderealPosApparent (const StelCore *core) const
	Get observer-centered hour angle + declination (at current equinox) It is the apparent position, i.e. More...

Vec3d	getAltAzPosGeometric (const StelCore *core) const
	Get observer-centered alt/az position It is the geometric position, i.e. More...

Vec3d	getAltAzPosApparent (const StelCore *core) const
	Get observer-centered alt/az position It is the apparent position, i.e. More...

Vec3d	getAltAzPosAuto (const StelCore *core) const
	Get observer-centered alt/az position It is the automatic position, i.e. More...

float	getParallacticAngle (const StelCore *core) const
	Get parallactic angle, which is the deviation between zenith angle and north angle. [radians].

bool	isAboveHorizon (const StelCore *core) const
	Checking position an object above mathematical horizon for current location. More...

bool	isAboveRealHorizon (const StelCore *core) const
	Checking position an object above real horizon for current location. More...

float	getVMagnitudeWithExtinction (const StelCore *core) const
	Return object's apparent V magnitude as seen from observer including extinction. More...

virtual float	getAirmass (const StelCore *core) const
	Return airmass value for the object (for atmosphere-dependent calculations) More...

Static Public Member Functions
static void	init ()
	Initializes static vars. Must be called before creating first planet.

static ApparentMagnitudeAlgorithm	getApparentMagnitudeAlgorithm ()

static const QString	getApparentMagnitudeAlgorithmString ()

static void	setApparentMagnitudeAlgorithm (QString algorithm)

static void	setApparentMagnitudeAlgorithm (ApparentMagnitudeAlgorithm algorithm)

static float	getPAsun (const Vec3d &sunPos, const Vec3d &objPos)
	Get the position angle of the illuminated limb of a planet The result depends on the arguments' coordinate system which must be identical. More...

static void	setLabelColor (const Vec3f &lc)

static const Vec3f &	getLabelColor (void)

static void	setOrbitColor (const Vec3f &oc)

static const Vec3f &	getOrbitColor ()

static void	setMajorPlanetOrbitColor (const Vec3f &oc)

static const Vec3f &	getMajorPlanetOrbitColor ()

static void	setMoonOrbitColor (const Vec3f &oc)

static const Vec3f &	getMoonOrbitColor ()

static void	setMinorPlanetOrbitColor (const Vec3f &oc)

static const Vec3f &	getMinorPlanetOrbitColor ()

static void	setDwarfPlanetOrbitColor (const Vec3f &oc)

static const Vec3f &	getDwarfPlanetOrbitColor ()

static void	setCubewanoOrbitColor (const Vec3f &oc)

static const Vec3f &	getCubewanoOrbitColor ()

static void	setPlutinoOrbitColor (const Vec3f &oc)

static const Vec3f &	getPlutinoOrbitColor ()

static void	setScatteredDiscObjectOrbitColor (const Vec3f &oc)

static const Vec3f &	getScatteredDiscObjectOrbitColor ()

static void	setOortCloudObjectOrbitColor (const Vec3f &oc)

static const Vec3f &	getOortCloudObjectOrbitColor ()

static void	setCometOrbitColor (const Vec3f &oc)

static const Vec3f &	getCometOrbitColor ()

static void	setSednoidOrbitColor (const Vec3f &oc)

static const Vec3f &	getSednoidOrbitColor ()

static void	setInterstellarOrbitColor (const Vec3f &oc)

static const Vec3f &	getInterstellarOrbitColor ()

static void	setMercuryOrbitColor (const Vec3f &oc)

static const Vec3f &	getMercuryOrbitColor ()

static void	setVenusOrbitColor (const Vec3f &oc)

static const Vec3f &	getVenusOrbitColor ()

static void	setEarthOrbitColor (const Vec3f &oc)

static const Vec3f &	getEarthOrbitColor ()

static void	setMarsOrbitColor (const Vec3f &oc)

static const Vec3f &	getMarsOrbitColor ()

static void	setJupiterOrbitColor (const Vec3f &oc)

static const Vec3f &	getJupiterOrbitColor ()

static void	setSaturnOrbitColor (const Vec3f &oc)

static const Vec3f &	getSaturnOrbitColor ()

static void	setUranusOrbitColor (const Vec3f &oc)

static const Vec3f &	getUranusOrbitColor ()

static void	setNeptuneOrbitColor (const Vec3f &oc)

static const Vec3f &	getNeptuneOrbitColor ()

Data Fields
bool	flagNativeName

LinearFader	orbitFader

Vec3d	orbit [ORBIT_SEGMENTS+1]

double	deltaJDE

double	deltaOrbitJDE

bool	closeOrbit

Static Public Attributes
static const QString	PLANET_TYPE

static Vec3f	orbitColor

static Vec3f	orbitMajorPlanetsColor

static Vec3f	orbitMoonsColor

static Vec3f	orbitMinorPlanetsColor

static Vec3f	orbitDwarfPlanetsColor

static Vec3f	orbitCubewanosColor

static Vec3f	orbitPlutinosColor

static Vec3f	orbitScatteredDiscObjectsColor

static Vec3f	orbitOortCloudObjectsColor

static Vec3f	orbitCometsColor

static Vec3f	orbitSednoidsColor

static Vec3f	orbitInterstellarColor

static Vec3f	orbitMercuryColor

static Vec3f	orbitVenusColor

static Vec3f	orbitEarthColor

static Vec3f	orbitMarsColor

static Vec3f	orbitJupiterColor

static Vec3f	orbitSaturnColor

static Vec3f	orbitUranusColor

static Vec3f	orbitNeptuneColor

static PlanetOrbitColorStyle	orbitColorStyle

Static Public Attributes inherited from StelObject
static constexpr InfoStringGroup	AllInfo
	A pre-defined "all available" set of specifiers for the getInfoString flags argument to getInfoString. More...

static constexpr InfoStringGroup	DefaultInfo
	A pre-defined "default" set of specifiers for the getInfoString flags argument to getInfoString It appears useful to propose this set as post-install settings and let users configure more on demand. More...

static constexpr InfoStringGroup	ShortInfo = static_cast<InfoStringGroup>(Name\|CatalogNumber\|Magnitude\|RaDecJ2000)
	A pre-defined "shortest useful" set of specifiers for the getInfoString flags argument to getInfoString.

Protected Member Functions
virtual QString	getInfoStringName (const StelCore *core, const InfoStringGroup &flags) const

virtual QString	getInfoStringAbsoluteMagnitude (const StelCore *core, const InfoStringGroup &flags) const

virtual QString	getInfoStringExtraMag (const StelCore *core, const InfoStringGroup &flags) const
	Any flag=Extra information to be displayed after the magnitude strings.

virtual QString	getInfoStringSize (const StelCore *core, const InfoStringGroup &flags) const
	Any flag=Size information to be displayed.

virtual QString	getInfoStringEloPhase (const StelCore *core, const InfoStringGroup &flags, const bool withIllum) const
	Return elongation and phase angle when flags=Elongation.

virtual QString	getInfoStringPeriods (const StelCore *core, const InfoStringGroup &flags) const
	Return sidereal and synodic periods when flags=Extra.

virtual QString	getInfoStringExtra (const StelCore *core, const InfoStringGroup &flags) const
	Any flag=Extra information to be displayed at the end.

void	computeModelMatrix (Mat4d &result, bool solarEclipseCase) const
	Used in drawSphere() to compute shadows, and inside a function to derive eclipse sizes. More...

void	computeOrbit ()
	Update the orbit position values.

Vec3f	getCurrentOrbitColor () const

QString	getPlanetLabel () const
	Return the information string "ready to print".

void	draw3dModel (StelCore *core, StelProjector::ModelViewTranformP transfo, float screenRd, bool drawOnlyRing=false)
	Draw the 3d model. More...

bool	drawObjModel (StelPainter *painter, float screenRd)
	Draws the OBJ model, assuming it is available. More...

bool	drawObjShadowMap (StelPainter *painter, QMatrix4x4 &shadowMatrix)

bool	ensureObjLoaded ()
	Starts the OBJ loading process, if it has not been done yet. More...

void	drawSphere (StelPainter *painter, float screenRd, bool drawOnlyRing=false)
	Draw the 3D sphere.

void	drawSurvey (StelCore core, StelPainter painter)
	Draw the Hips survey.

void	drawHints (const StelCore *core, const QFont &planetNameFont)
	Draw the circle and name of the Planet.

PlanetOBJModel *	loadObjModel () const

Protected Member Functions inherited from StelObject
QString	getCommonInfoString (const StelCore *core, const InfoStringGroup &flags) const
	Format the positional info string containing J2000/of date/altaz/hour angle positions and constellation, sidereal time, etc. More...

virtual QString	getMagnitudeInfoString (const StelCore *core, const InfoStringGroup &flags, const int decimals=1) const
	Format the magnitude info string for the object. More...

QString	getSolarLunarInfoString (const StelCore *core, const InfoStringGroup &flags) const
	Add a section to the InfoString with just horizontal data for the Sun and Moon, when observed from Earth. More...

void	postProcessInfoString (QString &str, const InfoStringGroup &flags) const
	Apply post processing on the info string. More...

Protected Attributes
QString	englishName

QString	nameI18

QString	nativeName

QString	nativeNameMeaning

QString	nativeNameMeaningI18n

QString	texMapName

QString	normalMapName

RotationElements	re

double	siderealPeriod

double	equatorialRadius

double	oneMinusOblateness

Vec3d	eclipticPos

Vec3d	eclipticVelocity

Vec3d	aberrationPush

Vec3d	screenPos

Vec3f	haloColor

float	absoluteMagnitude

float	albedo

float	roughness

float	outgas_intensity

float	outgas_falloff

Mat4d	rotLocalToParent

float	axisRotation

StelTextureSP	texMap

StelTextureSP	normalMap

PlanetOBJModel *	objModel

QFuture< PlanetOBJModel * > *	objModelLoader

QString	objModelPath

HipsSurveyP	survey

Ring *	rings

double	distance

double	sphereScale

double	lastJDE

posFuncType	coordFunc

Orbit *	orbitPtr

OsculatingFunctType *const	osculatingFunc

QSharedPointer< Planet >	parent

QList< QSharedPointer< Planet > >	satellites

LinearFader	hintFader

LinearFader	labelsFader

bool	flagLabels

bool	hidden

bool	atmosphere

bool	halo

PlanetType	pType

bool	multisamplingEnabled_

QOpenGLFunctions *	gl

Static Protected Attributes
static StelTextureSP	texEarthShadow

static ApparentMagnitudeAlgorithm	vMagAlgorithm

static Vec3f	labelColor

static StelTextureSP	hintCircleTex

static const QMap< PlanetType, QString >	pTypeMap

static const QMap< ApparentMagnitudeAlgorithm, QString >	vMagAlgorithmMap

static bool	drawMoonHalo

static bool	drawSunHalo

static bool	permanentDrawingOrbits
	If true, planet orbits will be drawn even if planet is off screen.

static int	orbitsThickness

Friends
class	SolarSystem

Additional Inherited Members
Public Slots inherited from StelObject
virtual void	setExtraInfoString (const InfoStringGroup &flags, const QString &str)
	Allow additions to the Info String. More...

virtual void	addToExtraInfoString (const StelObject::InfoStringGroup &flags, const QString &str)
	Add str to the extra string. More...

QStringList	getExtraInfoStrings (const InfoStringGroup &flags) const
	Retrieve an (unsorted) QStringList of all extra info strings that match flags. More...

void	removeExtraInfoStrings (const InfoStringGroup &flags)
	Remove the extraInfoStrings with the given flags. More...

Member Enumeration Documentation

◆ PositionQuality

enum Planet::PositionQuality

Objects on KeplerOrbits may be too far from their epoch to provide useful data.

Member Function Documentation

◆ computeDistance()

double Planet::computeDistance ( const Vec3d & obsHelioPos )

They must be fast if close to observer, but can be slow if further away.

◆ computeModelMatrix()

void Planet::computeModelMatrix	(	Mat4d &	result,
		bool	solarEclipseCase
	)		const

protected

Parameters

solarEclipseCase For reasons currently unknown we must handle solar eclipses as special case.

◆ computeTransMatrix()

void Planet::computeTransMatrix	(	double	JD,
		double	JDE
	)

This requires both flavours of JD in cases involving Earth.

◆ draw3dModel()

void Planet::draw3dModel	(	StelCore *	core,
		StelProjector::ModelViewTranformP	transfo,
		float	screenRd,
		bool	drawOnlyRing = `false`
	)

protected

Call the proper functions if there are rings etc..

Parameters

screenRd radius in screen pixels

◆ drawObjModel()

bool Planet::drawObjModel	(	StelPainter *	painter,
		float	screenRd
	)

protected

Parameters

screenRd radius in screen pixels.

Returns: false if the model can currently not be drawn (not loaded)

◆ ensureObjLoaded()

bool Planet::ensureObjLoaded ( )

protected

Returns true when the OBJ is ready to draw

◆ getEquatorialRadius()

double Planet::getEquatorialRadius ( void ) const

inline

Returns: the equator radius of the planet in astronomical units.

◆ getHeliocentricPos()

Vec3d Planet::getHeliocentricPos ( Vec3d p ) const

p planetocentric rectangular ecliptical coordinate (J2000)
Returns
heliocentric rectangular ecliptical coordinates (J2000)

◆ getID()

virtual QString Planet::getID ( void ) const

inlinevirtual

The ID should be unique for all objects of the same type, but may freely conflict with IDs of other types, so getType() must also be tested.

With this it should be possible to at least identify the same object in a different instance of Stellarium running the same version, but it would even be better if the ID provides some degree of forward-compatibility. For some object types (e.g. planets) this may simply return getEnglishName(), but better candidates may be official designations or at least (stable) internal IDs.

An object may have multiple IDs (different catalog numbers, etc). StelObjectMgr::searchByID() should search through all ID variants, but this method only returns one of them.

Implements StelObject.

◆ getInfoMap()

virtual QVariantMap Planet::getInfoMap ( const StelCore * core ) const

virtual

distance
phase (result of getPhase)
illumination (=100*phase)
phase-angle (radians)
phase-angle-dms (formatted string; DMS)
phase-angle-deg (formatted string; degrees)
elongation (radians)
elongation-dms (formatted string; DMS)
elongation-deg (formatted string; degrees)
ecl-elongation (elongation in ecliptic longitude or Δλ; on Earth only; radians)
ecl-elongation-dms (elongation in ecliptic longitude or Δλ; on Earth only; formatted string; DMS)
ecl-elongation-deg (elongation in ecliptic longitude or Δλ; on Earth only; formatted string; degrees)
type (object type description)
velocity (formatted string)
heliocentric-velocity (formatted string)
scale
eclipse-obscuration (for Sun only)
eclipse-magnitude (for Sun only)
central_l (on Earth only; degrees)
central_b (on Earth only; degrees)
pa_axis (on Earth only; degrees)
subsolar_l (on Earth only; degrees)
subsolar_b (on Earth only; degrees)
libration_l (on Earth for Moon only; degrees)
libration_b (on Earth for Moon only; degrees)
colongitude (on Earth for Moon only; degrees)
penumbral-eclipse-magnitude (on Earth for Moon only)
umbral-eclipse-magnitude (on Earth for Moon only)

Reimplemented from StelObject.

Reimplemented in Comet.

◆ getInfoString()

virtual QString Planet::getInfoString	(	const StelCore *	core,
		const InfoStringGroup &	flags
	)		const

virtual

Planets support the following InfoStringGroup flags:

Name
Magnitude
RaDec
AltAzi
Distance
Size
PlainText
Extra: Heliocentric Ecliptical Coordinates & Observer-planetocentric Ecliptical Coordinates, Phase, illumination, phase angle & elongation from the Sun
Note
subclasses should prefer to override only the component infostrings getInfoString...(), not this method!

Parameters

core the StelCore object

flags a set of InfoStringGroup items to include in the return value.

Returns
a QString containing an HMTL encoded description of the Planet.

Implements StelObject.

◆ getJ2000EquatorialPos()

virtual Vec3d Planet::getJ2000EquatorialPos ( const StelCore * core ) const

virtual

frame (practically equal to ecliptic of J2000 for us) coordinates relative to the parent body (sun, planet). To get J2000 equatorial coordinates, we require heliocentric ecliptical positions (adding up parent positions) of observer and Planet. Then we use the matrix rotation multiplication with an existing matrix in StelCore to orient from eclipticalJ2000 to equatorialJ2000. The end result is a non-normalized 3D vector which allows retrieving distances etc. The positional computation is called by SolarSystem. If the core's aberration setting is active, the J2000 position will then include it.

Implements StelObject.

◆ getPAsun()

static float Planet::getPAsun	(	const Vec3d &	sunPos,
		const Vec3d &	objPos
	)

static

E.g. if both are equatorial for equinox of date or J2000, the angle is zero when the bright limb is towards the north of the disk. An angle of 90° indicates a bright limb on the eastern limb, like an old moon. Source: Meeus, Astr.Algorithms (2nd ed.), 48.5.

◆ getPolarRadius()

double Planet::getPolarRadius ( void ) const

inline

Returns: the polar radius of the planet in astronomical units.

◆ getRectangularCoordinates()

Vec4d Planet::getRectangularCoordinates	(	const double	longDeg,
		const double	latDeg,
		const double	altMetres = `0.`
	)		const

Meeus, Astr. Alg. 2nd ed, Ch.11.

Parameters

longDeg	longitude of location, degrees. (currently unused. Set to 0.)
latDeg	planetographic latitude, degrees.
altMetres	altitude above ellipsoid surface (metres)

Returns: [rhoCosPhiPrime*a, rhoSinPhiPrime*a, phiPrime, rho*a] where a=equatorial radius [AU] phiPrime=planetocentric latitude rho*a=planetocentric distance of point [AU]

◆ getRotEquatorialToVsop87()

Mat4d Planet::getRotEquatorialToVsop87 ( void ) const

For planets/moons with WGCCRE rotation elements, this is just a single matrix. For objects with traditional elements, this builds up the matrix from the parents.

◆ getRotObliquity()

double Planet::getRotObliquity ( double JDE ) const

For Earth, this is the angle between axis and normal to current ecliptic of date, i.e. the ecliptic obliquity of date JDE. Note: The only place where this is not used for Earth is to build up orbits for planet moons w.r.t. the parent planet orientation.

◆ getRTSTime()

virtual Vec4d Planet::getRTSTime	(	const StelCore *	core,
		const double	altitude = `0.`
	)		const

virtual

Parameters

core	the currently active StelCore object
altitude	(optional; default=0) altitude of the object, degrees. Setting this to -6. for the Sun will find begin and end for civil twilight.

Returns: Vec4d - time of rise, transit and set closest to current time; JD.

Note

The fourth element flags particular conditions:

+100. for circumpolar objects. Rise and set give lower culmination times.
-100. for objects never rising. Rise and set give transit times.
-1000. is used as "invalid" value. The result should then not be used.

This is based on Meeus, Astronomical Algorithms (2nd ed.), but deviates in details.

Limitation for efficiency: If this is a planet moon from another planet, we compute RTS for the parent planet instead!

Reimplemented from StelObject.

◆ getSiderealTime()

double Planet::getSiderealTime	(	double	JD,
		double	JDE
	)		const

On Earth, sidereal time on the other hand is the angle along the planet equator from RA0 to the meridian, i.e. hour angle of the first point of Aries. For Earth (of course) it is sidereal time at Greenwich. V0.21+ update: For planets and Moons, in this context this is the rotation angle W of the Prime meridian from the ascending node of the planet equator on the ICRF equator. The usual WGCCRE model is W=W0+d*W1. Some planets/moons have more complicated rotations though, these are also handled in here. The planet objects with old-style data are computed like in earlier versions of Stellarium. Their computational model is however questionable. For general applicability we need both time flavours:

Parameters

JD	is JD(UT) for Earth
JDE	is used for other locations

◆ getSubSolarObserverPoints()

QPair<Vec4d, Vec3d> Planet::getSubSolarObserverPoints	(	const StelCore *	core,
		bool	jupiterGraphical = `false`
	)		const

These are defined so that over time the longitude of the central meridian increases. This means longitudes are counted positive towards the west for direct rotators and positive towards the East for negative rotators (e.g. Venus). Other cartographic conventions may have to be followed elsewhere in the program, though. (e.g. planetary feature nomenclature!) Only meaningful for earth-bound observers. Source: Explanatory Supplement 2013, 10.4.1

Parameters

jupiterGraphical Jupiter requires special treatment because its LII coordinate system does not stay in sync with the texture. (GRS is moving). Set this to true to return the incorrect, graphics-only longitude. first[0] = 10.26 phi_e [rad] Planetocentric latitude of sub-earth point first[1] = 10.26 phi'_e [rad] Planetographic latitude of sub-earth point first[2] = 10.26 lambda'_e [rad] Planetographic longitude of sub-earth point (0..2pi) first[3] = 10.29 P_n [rad] Position angle of axis north pole in equatorial coordinates of date second[0] = 10.26 phi_s [rad] Planetocentric latitude of sub-solar point second[1] = 10.26 phi'_s [rad] Planetographic latitude of sub-solar point second[2] = 10.26 lambda'_s [rad] Planetographic longitude of sub-solar point (0..2pi)

Note: : For the Moon, it is more common to give Libration angles, where L=-lambda'_e, B=phi'_e.; : For Jupiter, this returns central meridian in L_II.; : For Saturn, this returns central meridian in L_III (rotation of magnetic field).

◆ getValidPositionalDataRange()

Vec2d Planet::getValidPositionalDataRange ( const PositionQuality purpose ) const

For the major planets and moons, this is always (std::numeric_limits<double>::min(), std::numeric_limits<double>::max()) For planets with Keplerian orbits, this is [epoch-orbit_good, epoch+orbit_good] or, if purpose=Position, [epoch-min(orbit_good, 365), epoch+min(orbit_good, 365)]. This should help to detect and avoid using outdated orbital elements.

◆ hasValidPositionalData()

bool Planet::hasValidPositionalData	(	const double	JDE,
		const PositionQuality	purpose
	)		const

E.g. outdated orbital elements for Kepler orbits (beyond their orbit_good .ini file entries) may lead to invalid positions which should better not be used.

Parameters

purpose signal whether result should be good enough for observation of just for plotting orbit data. For observation, date should be within the orbit_good value, or within 1 year from epoch of the orbital elements.

Note: for major planets and moons this method will always return true

◆ setHeliocentricEclipticPos()

void Planet::setHeliocentricEclipticPos ( const Vec3d & pos )

pos heliocentric rectangular ecliptical coordinate (J2000)

◆ setRotationElements()

void Planet::setRotationElements	(	const QString	name,
		const double	_period,
		const double	_offset,
		const double	_epoch,
		const double	_obliquity,
		const double	_ascendingNode,
		const double	_ra0,
		const double	_ra1,
		const double	_de0,
		const double	_de1,
		const double	_w0,
		const double	_w1
	)

Given two data models, we must support both: the traditional elements relative to the parent object: name: English name of the object. A corrective function may be attached which depends on the name. _period: duration of sidereal rotation [Julian days] _offset: [angle at _epoch. ] _epoch: [JDE] _obliquity [rad] _ascendingNode of equator on ecliptic[rad] The more modern way to specify these elements are relative to the ICRF: ra_pole=_ra0 + T*_ra1. ra_pole and de_pole must be computed more than for initialisation for J2000 de_pole=_de0 + T*_de1. ra and de values to be stored in [rad] _w0, _w1 to be given in degrees! If _ra0 is not zero, we understand WGCCRE data ra0, ra1, de0, de1, w0, w1 are used.

◆ setRotEquatorialToVsop87()

void Planet::setRotEquatorialToVsop87 ( const Mat4d & m )

For planets/moons with WGCCRE rotation elements, this just sets this matrix. For objects with traditional elements, this builds up the matrix from the parents.

◆ setSiderealPeriod()

void Planet::setSiderealPeriod ( const double siderealPeriod )

Also sets deltaOrbitJDE and may set closeOrbit for Planet objects which have KeplerOrbits. siderealPeriod [earth days] orbital duration.

◆ translateName()

virtual void Planet::translateName ( const StelTranslator & trans )

virtual

Translate planet name using the passed translator

Reimplemented in Comet, and MinorPlanet.

core	the StelCore object
flags	a set of InfoStringGroup items to include in the return value.

Data Structures

Public Types

Public Member Functions

Static Public Member Functions

Data Fields

Static Public Attributes

Protected Member Functions

Protected Attributes

Static Protected Attributes

Friends

Additional Inherited Members

Member Enumeration Documentation

◆ PositionQuality

Member Function Documentation

◆ computeDistance()

◆ computeModelMatrix()

◆ computeTransMatrix()

◆ draw3dModel()

◆ drawObjModel()

◆ ensureObjLoaded()

◆ getEquatorialRadius()

◆ getHeliocentricPos()

◆ getID()

◆ getInfoMap()

◆ getInfoString()

◆ getJ2000EquatorialPos()

◆ getPAsun()

◆ getPolarRadius()

◆ getRectangularCoordinates()

◆ getRotEquatorialToVsop87()

◆ getRotObliquity()

◆ getRTSTime()

◆ getSiderealTime()

◆ getSubSolarObserverPoints()

◆ getValidPositionalDataRange()

◆ hasValidPositionalData()

◆ setHeliocentricEclipticPos()

◆ setRotationElements()

◆ setRotEquatorialToVsop87()

◆ setSiderealPeriod()

◆ translateName()