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/***************************************************************************
ksmoon.cpp - Trinity Desktop Planetarium
-------------------
begin : Sun Aug 26 2001
copyright : (C) 2001 by Jason Harris
email : kstars@30doradus.org
***************************************************************************/
/***************************************************************************
* *
* This program is free software; you can redistribute it and/or modify *
* it under the terms of the GNU General Public License as published by *
* the Free Software Foundation; either version 2 of the License, or *
* (at your option) any later version. *
* *
***************************************************************************/
#include <stdlib.h>
#include <math.h>
#include <tqfile.h>
#include "ksnumbers.h"
#include "ksutils.h"
#include "kssun.h"
#include "ksmoon.h"
#include "kstarsdata.h"
KSMoon::KSMoon(KStarsData *kd)
: KSPlanetBase( kd, I18N_NOOP("Moon"), "", 3474.8 /*diameter in km*/ ) {
BData.setAutoDelete(true);
LRData.setAutoDelete(true);
}
KSMoon::~KSMoon() {
}
bool KSMoon::data_loaded = false;
TQPtrList<KSMoon::MoonLRData> KSMoon::LRData;
TQPtrList<KSMoon::MoonBData> KSMoon::BData;
bool KSMoon::loadData() {
if (data_loaded) return true;
TQString line;
TQFile f;
int nd, nm, nm1, nf;
double Li, Ri, Bi; //coefficients of the sums
if ( KSUtils::openDataFile( f, "moonLR.dat" ) ) {
TQTextStream stream( &f );
while ( !stream.eof() ) {
line = stream.readLine();
TQTextIStream instream( &line );
instream >> nd >> nm >> nm1 >> nf >> Li >> Ri;
LRData.append(new MoonLRData(nd, nm, nm1, nf, Li, Ri));
}
f.close();
} else
return false;
if ( KSUtils::openDataFile( f, "moonB.dat" ) ) {
TQTextStream stream( &f );
while ( !stream.eof() ) {
line = stream.readLine();
TQTextIStream instream( &line );
instream >> nd >> nm >> nm1 >> nf >> Bi;
BData.append(new MoonBData(nd, nm, nm1, nf, Bi));
}
f.close();
}
data_loaded = true;
return true;
}
bool KSMoon::findGeocentricPosition( const KSNumbers *num, const KSPlanetBase* ) {
//Algorithms in this subroutine are taken from Chapter 45 of "Astronomical Algorithms"
//by Jean Meeus (1991, Willmann-Bell, Inc. ISBN 0-943396-35-2. http://www.willbell.com/math/mc1.htm)
TQString fname, snum, line;
TQFile f;
double DegtoRad;
double T, L, D, M, M1, F, E, A1, A2, A3;
double sumL, sumR, sumB;
DegtoRad = acos( -1.0 )/180.0;
//Julian centuries since J2000
T = num->julianCenturies();
double Et = 1.0 - 0.002516*T - 0.0000074*T*T;
//Moon's mean longitude
L = 218.3164591 + 481267.88134236*T - 0.0013268*T*T + T*T*T/538841.0 - T*T*T*T/65194000.0;
while ( L > 360.0 ) L -= 360.0;
while ( L < 0.0 ) L += 360.0;
L *= DegtoRad;
//Moon's mean elongation
D = 297.8502042 + 445267.1115168*T - 0.0016300*T*T + T*T*T/545868.0 - T*T*T*T/113065000.0;
while ( D > 360.0 ) D -= 360.0;
while ( D < 0.0 ) D += 360.0;
D *= DegtoRad;
//Sun's mean anomaly
M = 357.5291092 + 35999.0502909*T - 0.0001536*T*T + T*T*T/24490000.0;
while ( M > 360.0 ) M -= 360.0;
while ( M < 0.0 ) M += 360.0;
M *= DegtoRad;
//Moon's mean anomaly
M1= 134.9634114 + 477198.8676313*T + 0.0089970*T*T + T*T*T/69699.0 - T*T*T*T/14712000.0;
while ( M1 > 360.0 ) M1 -= 360.0;
while ( M1 < 0.0 ) M1 += 360.0;
M1 *= DegtoRad;
//Moon's argument of latitude (angle from ascending node)
F = 93.2720993 + 483202.0175273*T - 0.0034029*T*T - T*T*T/3526000.0 + T*T*T*T/863310000.0;
while ( F > 360.0 ) F -= 360.0;
while ( F < 0.0 ) F += 360.0;
F *= DegtoRad;
A1 = 119.75 + 131.849*T;
A2 = 53.09 + 479264.290*T;
A3 = 313.45 + 481226.484*T;
while ( A1 > 360.0 ) A1 -= 360.0;
while ( A1 < 0.0 ) A1 += 360.0;
while ( A2 > 360.0 ) A2 -= 360.0;
while ( A2 < 0.0 ) A2 += 360.0;
while ( A3 > 360.0 ) A3 -= 360.0;
while ( A3 < 0.0 ) A3 += 360.0;
A1 *= DegtoRad;
A2 *= DegtoRad;
A3 *= DegtoRad;
//Calculate the series expansions stored in moonLR.txt and moonB.txt.
//
sumL = 0.0;
sumR = 0.0;
if (!loadData()) return false;
for (MoonLRData *mlrd = LRData.first(); mlrd != 0; mlrd = LRData.next()) {
E = 1.0;
if ( mlrd->nm ) { //if M != 0, include changing eccentricity of Earth's orbit
E = Et;
if ( abs( mlrd->nm )==2 ) E = E*E; //use E^2
}
sumL += E*mlrd->Li*sin( mlrd->nd*D + mlrd->nm*M + mlrd->nm1*M1 + mlrd->nf*F );
sumR += E*mlrd->Ri*cos( mlrd->nd*D + mlrd->nm*M + mlrd->nm1*M1 + mlrd->nf*F );
}
sumB = 0.0;
for (MoonBData *mbd = BData.first(); mbd != 0; mbd = BData.next()) {
E = 1.0;
if ( mbd->nm ) { //if M != 0, include changing eccentricity of Earth's orbit
E = Et;
if ( abs( mbd->nm )==2 ) E = E*E; //use E^2
}
sumB += E*mbd->Bi*sin( mbd->nd*D + mbd->nm*M + mbd->nm1*M1 + mbd->nf*F );
}
//Additive terms for sumL and sumB
sumL += ( 3958.0*sin( A1 ) + 1962.0*sin( L-F ) + 318.0*sin( A2 ) );
sumB += ( -2235.0*sin( L ) + 382.0*sin( A3 ) + 175.0*sin( A1-F ) + 175.0*sin( A1+F ) + 127.0*sin( L-M1 ) - 115.0*sin( L+M1 ) );
//Geocentric coordinates
setEcLong( ( L + DegtoRad*sumL/1000000.0 ) * 180./dms::PI ); //convert radians to degrees
setEcLat( ( DegtoRad*sumB/1000000.0 ) * 180./dms::PI );
Rearth = ( 385000.56 + sumR/1000.0 )/AU_KM; //distance from Earth, in AU
setAngularSize( asin(physicalSize()/Rearth/AU_KM)*60.*180./dms::PI ); //angular size in arcmin
EclipticToEquatorial( num->obliquity() );
//Determine position angle
findPA( num );
return true;
}
void KSMoon::findPhase( const KSSun *Sun ) {
Phase.setD( ecLong()->Degrees() - Sun->ecLong()->Degrees() );
Phase.setD( Phase.reduce().Degrees() );
int iPhase = int( 0.1*Phase.Degrees()+0.5 );
if (iPhase==36) iPhase = 0;
TQString sPhase;
sPhase = sPhase.sprintf( "%02d", iPhase );
TQString imName = "moon" + sPhase + ".png";
TQFile imFile;
if ( KSUtils::openDataFile( imFile, imName ) ) {
imFile.close();
image0()->load( imFile.name() );
image()->load( imFile.name() );
}
}
TQString KSMoon::phaseName() const {
double f = illum();
double p = phase().Degrees();
//First, handle the major phases
if ( f > 0.99 ) return i18n( "moon phase, 100 percent illuminated", "Full moon" );
if ( f < 0.01 ) return i18n( "moon phase, 0 percent illuminated", "New moon" );
if ( fabs( f - 0.50 ) < 0.01 ) {
if ( p < 180.0 ) return i18n( "moon phase, half-illuminated and growing", "First quarter" );
else return i18n( "moon phase, half-illuminated and shrinking", "Third quarter" );
}
//Next, handle the more general cases
if ( p < 90.0 ) return i18n( "moon phase between new moon and 1st quarter", "Waxing crescent" );
else if ( p < 180.0 ) return i18n( "moon phase between 1st quarter and full moon", "Waxing gibbous" );
else if ( p < 270.0 ) return i18n( "moon phase between full moon and 3rd quarter", "Waning gibbous" );
else if ( p < 360.0 ) return i18n( "moon phase between 3rd quarter and new moon", "Waning crescent" );
else return i18n( "unknown" );
}
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