예제 #1
0
        public static double MeanObliquityOfEcliptic(double JD)
        {
            double U        = (JD - 2451545) / 3652500;
            double Usquared = U * U;
            double Ucubed   = Usquared * U;
            double U4       = Ucubed * U;
            double U5       = U4 * U;
            double U6       = U5 * U;
            double U7       = U6 * U;
            double U8       = U7 * U;
            double U9       = U8 * U;
            double U10      = U9 * U;


            return(AASCoordinateTransformation.DMSToDegrees(23, 26, 21.448) - AASCoordinateTransformation.DMSToDegrees(0, 0, 4680.93) * U
                   - AASCoordinateTransformation.DMSToDegrees(0, 0, 1.55) * Usquared
                   + AASCoordinateTransformation.DMSToDegrees(0, 0, 1999.25) * Ucubed
                   - AASCoordinateTransformation.DMSToDegrees(0, 0, 51.38) * U4
                   - AASCoordinateTransformation.DMSToDegrees(0, 0, 249.67) * U5
                   - AASCoordinateTransformation.DMSToDegrees(0, 0, 39.05) * U6
                   + AASCoordinateTransformation.DMSToDegrees(0, 0, 7.12) * U7
                   + AASCoordinateTransformation.DMSToDegrees(0, 0, 27.87) * U8
                   + AASCoordinateTransformation.DMSToDegrees(0, 0, 5.79) * U9
                   + AASCoordinateTransformation.DMSToDegrees(0, 0, 2.45) * U10);
        }
예제 #2
0
        public static AAS2DCoordinate PrecessEquatorialFK4(double Alpha, double Delta, double JD0, double JD)
        {
            double T        = (JD0 - 2415020.3135) / 36524.2199;
            double t        = (JD - JD0) / 36524.2199;
            double tsquared = t * t;
            double tcubed   = tsquared * t;

            //Now convert to radians
            Alpha = AASCoordinateTransformation.HoursToRadians(Alpha);
            Delta = AASCoordinateTransformation.DegreesToRadians(Delta);

            double sigma = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, (2304.250 + 1.396 * T) * t + 0.302 * tsquared + 0.018 * tcubed));
            double zeta  = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, 0.791 * tsquared + 0.001 * tcubed)) + sigma;
            double phi   = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, (2004.682 - 0.853 * T) * t - 0.426 * tsquared - 0.042 * tcubed));
            double A     = Math.Cos(Delta) * Math.Sin(Alpha + sigma);
            double B     = Math.Cos(phi) * Math.Cos(Delta) * Math.Cos(Alpha + sigma) - Math.Sin(phi) * Math.Sin(Delta);
            double C     = Math.Sin(phi) * Math.Cos(Delta) * Math.Cos(Alpha + sigma) + Math.Cos(phi) * Math.Sin(Delta);

            double          DeltaAlpha = AASCoordinateTransformation.DMSToDegrees(0, 0, 0.0775 + 0.0850 * T);
            AAS2DCoordinate value      = new AAS2DCoordinate();

            value.X = AASCoordinateTransformation.MapTo0To24Range(AASCoordinateTransformation.RadiansToHours(Math.Atan2(A, B) + zeta) + DeltaAlpha);
            value.Y = AASCoordinateTransformation.RadiansToDegrees(Math.Asin(C));

            return(value);
        }
예제 #3
0
        public static AASPhysicalSunDetails Calculate(double JD)
        {
            double theta = AASCoordinateTransformation.MapTo0To360Range((JD - 2398220) * 360 / 25.38);
            double I     = 7.25;
            double K     = 73.6667 + 1.3958333 * (JD - 2396758) / 36525;

            //Calculate the apparent longitude of the sun (excluding the effect of nutation)
            double L       = AASEarth.EclipticLongitude(JD);
            double R       = AASEarth.RadiusVector(JD);
            double SunLong = L + 180 - AASCoordinateTransformation.DMSToDegrees(0, 0, 20.4898 / R);

            double epsilon = AASNutation.TrueObliquityOfEcliptic(JD);

            //Convert to radians
            epsilon = AASCoordinateTransformation.DegreesToRadians(epsilon);
            SunLong = AASCoordinateTransformation.DegreesToRadians(SunLong);
            K       = AASCoordinateTransformation.DegreesToRadians(K);
            I       = AASCoordinateTransformation.DegreesToRadians(I);
            theta   = AASCoordinateTransformation.DegreesToRadians(theta);

            double x = Math.Atan(-Math.Cos(SunLong) * Math.Tan(epsilon));
            double y = Math.Atan(-Math.Cos(SunLong - K) * Math.Tan(I));

            AASPhysicalSunDetails details = new AASPhysicalSunDetails();

            details.P  = AASCoordinateTransformation.RadiansToDegrees(x + y);
            details.B0 = AASCoordinateTransformation.RadiansToDegrees(Math.Asin(Math.Sin(SunLong - K) * Math.Sin(I)));

            double eta = Math.Atan(Math.Tan(SunLong - K) * Math.Cos(I));

            details.L0 = AASCoordinateTransformation.MapTo0To360Range(AASCoordinateTransformation.RadiansToDegrees(eta - theta));

            return(details);
        }
예제 #4
0
        public static AAS2DCoordinate PrecessEcliptic(double Lambda, double Beta, double JD0, double JD)
        {
            double T        = (JD0 - 2451545.0) / 36525;
            double Tsquared = T * T;
            double t        = (JD - JD0) / 36525;
            double tsquared = t * t;
            double tcubed   = tsquared * t;

            //Now convert to radians
            Lambda = AASCoordinateTransformation.DegreesToRadians(Lambda);
            Beta   = AASCoordinateTransformation.DegreesToRadians(Beta);

            double eta = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, (47.0029 - 0.06603 * T + 0.000598 * Tsquared) * t + (-0.03302 + 0.000598 * T) * tsquared + 0.00006 * tcubed));
            double pi  = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, 174.876384 * 3600 + 3289.4789 * T + 0.60622 * Tsquared - (869.8089 + 0.50491 * T) * t + 0.03536 * tsquared));
            double p   = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, (5029.0966 + 2.22226 * T - 0.000042 * Tsquared) * t + (1.11113 - 0.000042 * T) * tsquared - 0.000006 * tcubed));
            double A   = Math.Cos(eta) * Math.Cos(Beta) * Math.Sin(pi - Lambda) - Math.Sin(eta) * Math.Sin(Beta);
            double B   = Math.Cos(Beta) * Math.Cos(pi - Lambda);
            double C   = Math.Cos(eta) * Math.Sin(Beta) + Math.Sin(eta) * Math.Cos(Beta) * Math.Sin(pi - Lambda);

            AAS2DCoordinate value = new AAS2DCoordinate();

            value.X = AASCoordinateTransformation.MapTo0To360Range(AASCoordinateTransformation.RadiansToDegrees(p + pi - Math.Atan2(A, B)));
            value.Y = AASCoordinateTransformation.RadiansToDegrees(Math.Asin(C));

            return(value);
        }
예제 #5
0
        public static AAS2DCoordinate PrecessEquatorial(double Alpha, double Delta, double JD0, double JD)
        {
            double T        = (JD0 - 2451545.0) / 36525;
            double Tsquared = T * T;
            double t        = (JD - JD0) / 36525;
            double tsquared = t * t;
            double tcubed   = tsquared * t;

            //Now convert to radians
            Alpha = AASCoordinateTransformation.HoursToRadians(Alpha);
            Delta = AASCoordinateTransformation.DegreesToRadians(Delta);

            double sigma = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, (2306.2181 + 1.39656 * T - 0.000139 * Tsquared) * t + (0.30188 - 0.000344 * T) * tsquared + 0.017998 * tcubed));
            double zeta  = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, (2306.2181 + 1.39656 * T - 0.000139 * Tsquared) * t + (1.09468 + 0.000066 * T) * tsquared + 0.018203 * tcubed));
            double phi   = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, (2004.3109 - 0.8533 * T - 0.000217 * Tsquared) * t - (0.42665 + 0.000217 * T) * tsquared - 0.041833 * tcubed));
            double A     = Math.Cos(Delta) * Math.Sin(Alpha + sigma);
            double B     = Math.Cos(phi) * Math.Cos(Delta) * Math.Cos(Alpha + sigma) - Math.Sin(phi) * Math.Sin(Delta);
            double C     = Math.Sin(phi) * Math.Cos(Delta) * Math.Cos(Alpha + sigma) + Math.Cos(phi) * Math.Sin(Delta);

            AAS2DCoordinate value = new AAS2DCoordinate();

            value.X = AASCoordinateTransformation.MapTo0To24Range(AASCoordinateTransformation.RadiansToHours(Math.Atan2(A, B) + zeta));
            value.Y = AASCoordinateTransformation.RadiansToDegrees(Math.Asin(C));

            return(value);
        }
예제 #6
0
        public static double Calculate(double JD)
        {
            double rho        = (JD - 2451545) / 365250;
            double rhosquared = rho * rho;
            double rhocubed   = rhosquared * rho;
            double rho4       = rhocubed * rho;
            double rho5       = rho4 * rho;

            //Calculate the Suns mean longitude
            double L0 = AASCoordinateTransformation.MapTo0To360Range(280.4664567 + 360007.6982779 * rho + 0.03032028 * rhosquared +
                                                                     rhocubed / 49931 - rho4 / 15300 - rho5 / 2000000);

            //Calculate the Suns apparent right ascension
            double          SunLong    = AASSun.ApparentEclipticLongitude(JD);
            double          SunLat     = AASSun.ApparentEclipticLatitude(JD);
            double          epsilon    = AASNutation.TrueObliquityOfEcliptic(JD);
            AAS2DCoordinate Equatorial = AASCoordinateTransformation.Ecliptic2Equatorial(SunLong, SunLat, epsilon);

            epsilon = AASCoordinateTransformation.DegreesToRadians(epsilon);
            double E = L0 - 0.0057183 - Equatorial.X * 15 + AASCoordinateTransformation.DMSToDegrees(0, 0, AASNutation.NutationInLongitude(JD)) * Math.Cos(epsilon);

            if (E > 180)
            {
                E = -(360 - E);
            }
            E *= 4; //Convert to minutes of time

            return(E);
        }
예제 #7
0
        public static AASEclipticalElementDetails Calculate(double i0, double w0, double omega0, double JD0, double JD)
        {
            double T        = (JD0 - 2451545.0) / 36525;
            double Tsquared = T * T;
            double t        = (JD - JD0) / 36525;
            double tsquared = t * t;
            double tcubed   = tsquared * t;

            //Now convert to radians
            double i0rad     = AASCoordinateTransformation.DegreesToRadians(i0);
            double omega0rad = AASCoordinateTransformation.DegreesToRadians(omega0);

            double eta = (47.0029 - 0.06603 * T + 0.000598 * Tsquared) * t + (-0.03302 + 0.000598 * T) * tsquared + 0.00006 * tcubed;

            eta = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, eta));

            double pi = 174.876384 * 3600 + 3289.4789 * T + 0.60622 * Tsquared - (869.8089 + 0.50491 * T) * t + 0.03536 * tsquared;

            pi = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, pi));

            double p = (5029.0966 + 2.22226 * T - 0.000042 * Tsquared) * t + (1.11113 - 0.000042 * T) * tsquared - 0.000006 * tcubed;

            p = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, p));

            double sini0rad        = Math.Sin(i0rad);
            double cosi0rad        = Math.Cos(i0rad);
            double sinomega0rad_pi = Math.Sin(omega0rad - pi);
            double cosomega0rad_pi = Math.Cos(omega0rad - pi);
            double sineta          = Math.Sin(eta);
            double coseta          = Math.Cos(eta);
            double A    = sini0rad * sinomega0rad_pi;
            double B    = -sineta * cosi0rad + coseta * sini0rad * cosomega0rad_pi;
            double irad = Math.Asin(Math.Sqrt(A * A + B * B));

            AASEclipticalElementDetails details = new AASEclipticalElementDetails();

            details.i = AASCoordinateTransformation.RadiansToDegrees(irad);
            double cosi = cosi0rad * coseta + sini0rad * sineta * cosomega0rad_pi;

            if (cosi < 0)
            {
                details.i = 180 - details.i;
            }

            double phi = pi + p;

            details.omega = AASCoordinateTransformation.MapTo0To360Range(AASCoordinateTransformation.RadiansToDegrees(Math.Atan2(A, B) + phi));

            A = -sineta * sinomega0rad_pi;
            B = sini0rad * coseta - cosi0rad * sineta * cosomega0rad_pi;
            double deltaw = AASCoordinateTransformation.RadiansToDegrees(Math.Atan2(A, B));

            details.w = AASCoordinateTransformation.MapTo0To360Range(w0 + deltaw);

            return(details);
        }
예제 #8
0
        public static double CorrectionInLatitude(double Longitude, double JD)
        {
            double T     = (JD - 2451545) / 36525;
            double Ldash = Longitude - 1.397 * T - 0.00031 * T * T;

            //Convert to radians
            Ldash = AASCoordinateTransformation.DegreesToRadians(Ldash);

            double value = 0.03916 * (Math.Cos(Ldash) - Math.Sin(Ldash));

            return(AASCoordinateTransformation.DMSToDegrees(0, 0, value));
        }
예제 #9
0
        public static double ApparentEclipticLongitude(double JD)
        {
            double Longitude = GeometricFK5EclipticLongitude(JD);

            //Apply the correction in longitude due to nutation
            Longitude += AASCoordinateTransformation.DMSToDegrees(0, 0, AASNutation.NutationInLongitude(JD));

            //Apply the correction in longitude due to aberration
            double R = AASEarth.RadiusVector(JD);

            Longitude -= AASCoordinateTransformation.DMSToDegrees(0, 0, 20.4898 / R);

            return(Longitude);
        }
예제 #10
0
        public static AAS3DCoordinate ConvertVSOPToFK5AnyEquinox(AAS3DCoordinate value, double JDEquinox)
        {
            double t        = (JDEquinox - 2451545.0) / 36525;
            double tsquared = t * t;
            double tcubed   = tsquared * t;

            double sigma = 2306.2181 * t + 0.30188 * tsquared + 0.017988 * tcubed;

            sigma = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, sigma));

            double zeta = 2306.2181 * t + 1.09468 * tsquared + 0.018203 * tcubed;

            zeta = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, zeta));

            double phi = 2004.3109 * t - 0.42665 * tsquared - 0.041833 * tcubed;

            phi = AASCoordinateTransformation.DegreesToRadians(AASCoordinateTransformation.DMSToDegrees(0, 0, phi));

            double cossigma = Math.Cos(sigma);
            double coszeta  = Math.Cos(zeta);
            double cosphi   = Math.Cos(phi);
            double sinsigma = Math.Sin(sigma);
            double sinzeta  = Math.Sin(zeta);
            double sinphi   = Math.Sin(phi);

            double xx = cossigma * coszeta * cosphi - sinsigma * sinzeta;
            double xy = sinsigma * coszeta + cossigma * sinzeta * cosphi;
            double xz = cossigma * sinphi;
            double yx = -cossigma * sinzeta - sinsigma * coszeta * cosphi;
            double yy = cossigma * coszeta - sinsigma * sinzeta * cosphi;
            double yz = -sinsigma * sinphi;
            double zx = -coszeta * sinphi;
            double zy = -sinzeta * sinphi;
            double zz = cosphi;

            AAS3DCoordinate result = new AAS3DCoordinate()
            {
                X = xx * value.X + yx * value.Y + zx * value.Z,
                Y = xy * value.X + yy * value.Y + zy * value.Z,
                Z = xz * value.X + yz * value.Y + zz * value.Z
            };

            return(result);
        }
예제 #11
0
        public static double ApparentEclipticLongitude(double JD, bool bHighPrecision)
        {
            double Longitude = GeometricFK5EclipticLongitude(JD, bHighPrecision);

            //Apply the correction in longitude due to nutation
            Longitude += AASCoordinateTransformation.DMSToDegrees(0, 0, AASNutation.NutationInLongitude(JD));

            //Apply the correction in longitude due to aberration
            double R = AASEarth.RadiusVector(JD, bHighPrecision);

            if (bHighPrecision)
            {
                Longitude -= (0.005775518 * R * AASCoordinateTransformation.DMSToDegrees(0, 0, VariationGeometricEclipticLongitude(JD)));
            }
            else
            {
                Longitude -= AASCoordinateTransformation.DMSToDegrees(0, 0, 20.4898 / R);
            }

            return(Longitude);
        }
예제 #12
0
 public static double TrueObliquityOfEcliptic(double JD)
 {
     return(MeanObliquityOfEcliptic(JD) + AASCoordinateTransformation.DMSToDegrees(0, 0, NutationInObliquity(JD)));
 }
예제 #13
0
        public static AASEllipticalPlanetaryDetails Calculate(double JD, AASEllipticalObject ellipticalObject, bool bHighPrecision)
        {
            //What will the the return value
            AASEllipticalPlanetaryDetails details = new AASEllipticalPlanetaryDetails();

            //Calculate the position of the earth first
            double JD0 = JD;
            double L0  = AASEarth.EclipticLongitude(JD0, bHighPrecision);
            double B0  = AASEarth.EclipticLatitude(JD0, bHighPrecision);
            double R0  = AASEarth.RadiusVector(JD0, bHighPrecision);

            L0 = AASCoordinateTransformation.DegreesToRadians(L0);
            B0 = AASCoordinateTransformation.DegreesToRadians(B0);
            double cosB0 = Math.Cos(B0);

            //Iterate to find the positions adjusting for light-time correction if required
            double L = 0;
            double B = 0;
            double R = 0;

            if (ellipticalObject != AASEllipticalObject.SUN)
            {
                bool   bRecalc      = true;
                bool   bFirstRecalc = true;
                double LPrevious    = 0;
                double BPrevious    = 0;
                double RPrevious    = 0;

                while (bRecalc)
                {
                    switch (ellipticalObject)
                    {
                    case AASEllipticalObject.SUN:

                        L = AASSun.GeometricEclipticLongitude(JD0, bHighPrecision);
                        B = AASSun.GeometricEclipticLatitude(JD0, bHighPrecision);
                        R = AASEarth.RadiusVector(JD0, bHighPrecision);
                        break;

                    case AASEllipticalObject.MERCURY:

                        L = AASMercury.EclipticLongitude(JD0, bHighPrecision);
                        B = AASMercury.EclipticLatitude(JD0, bHighPrecision);
                        R = AASMercury.RadiusVector(JD0, bHighPrecision);
                        break;

                    case AASEllipticalObject.VENUS:

                        L = AASVenus.EclipticLongitude(JD0, bHighPrecision);
                        B = AASVenus.EclipticLatitude(JD0, bHighPrecision);
                        R = AASVenus.RadiusVector(JD0, bHighPrecision);
                        break;

                    case AASEllipticalObject.MARS:

                        L = AASMars.EclipticLongitude(JD0, bHighPrecision);
                        B = AASMars.EclipticLatitude(JD0, bHighPrecision);
                        R = AASMars.RadiusVector(JD0, bHighPrecision);
                        break;

                    case AASEllipticalObject.JUPITER:

                        L = AASJupiter.EclipticLongitude(JD0, bHighPrecision);
                        B = AASJupiter.EclipticLatitude(JD0, bHighPrecision);
                        R = AASJupiter.RadiusVector(JD0, bHighPrecision);
                        break;

                    case AASEllipticalObject.SATURN:

                        L = AASSaturn.EclipticLongitude(JD0, bHighPrecision);
                        B = AASSaturn.EclipticLatitude(JD0, bHighPrecision);
                        R = AASSaturn.RadiusVector(JD0, bHighPrecision);
                        break;

                    case AASEllipticalObject.URANUS:

                        L = AASUranus.EclipticLongitude(JD0, bHighPrecision);
                        B = AASUranus.EclipticLatitude(JD0, bHighPrecision);
                        R = AASUranus.RadiusVector(JD0, bHighPrecision);
                        break;

                    case AASEllipticalObject.NEPTUNE:

                        L = AASNeptune.EclipticLongitude(JD0, bHighPrecision);
                        B = AASNeptune.EclipticLatitude(JD0, bHighPrecision);
                        R = AASNeptune.RadiusVector(JD0, bHighPrecision);
                        break;

                    case AASEllipticalObject.PLUTO:

                        L = AASPluto.EclipticLongitude(JD0);
                        B = AASPluto.EclipticLatitude(JD0);
                        R = AASPluto.RadiusVector(JD0);
                        break;

                    default:
                        break;
                    }

                    if (!bFirstRecalc)
                    {
                        bRecalc   = ((Math.Abs(L - LPrevious) > 0.00001) || (Math.Abs(B - BPrevious) > 0.00001) || (Math.Abs(R - RPrevious) > 0.000001));
                        LPrevious = L;
                        BPrevious = B;
                        RPrevious = R;
                    }
                    else
                    {
                        bFirstRecalc = false;
                    }

                    //Calculate the new value
                    if (bRecalc)
                    {
                        double Lrad     = AASCoordinateTransformation.DegreesToRadians(L);
                        double Brad     = AASCoordinateTransformation.DegreesToRadians(B);
                        double cosB     = Math.Cos(Brad);
                        double cosL     = Math.Cos(Lrad);
                        double x1       = R * cosB * cosL - R0 * cosB0 * Math.Cos(L0);
                        double y1       = R * cosB * Math.Sin(Lrad) - R0 * cosB0 * Math.Sin(L0);
                        double z1       = R * Math.Sin(Brad) - R0 * Math.Sin(B0);
                        double distance = Math.Sqrt(x1 * x1 + y1 * y1 + z1 * z1);

                        //Prepare for the next loop around
                        JD0 = JD - AASElliptical.DistanceToLightTime(distance);
                    }
                }
            }

            double x = 0;
            double y = 0;
            double z = 0;

            if (ellipticalObject != AASEllipticalObject.SUN)
            {
                double Lrad = AASCoordinateTransformation.DegreesToRadians(L);
                double Brad = AASCoordinateTransformation.DegreesToRadians(B);
                double cosB = Math.Cos(Brad);
                double cosL = Math.Cos(Lrad);

                x = R * cosB * cosL - R0 * cosB0 * Math.Cos(L0);
                y = R * cosB * Math.Sin(Lrad) - R0 * cosB0 * Math.Sin(L0);
                z = R * Math.Sin(Brad) - R0 * Math.Sin(B0);
            }
            else
            {
                x = -R0 *cosB0 *Math.Cos(L0);

                y = -R0 *cosB0 *Math.Sin(L0);

                z = -R0 *Math.Sin(B0);
            }

            double x2 = x * x;
            double y2 = y * y;

            details.ApparentGeocentricLatitude  = AASCoordinateTransformation.RadiansToDegrees(Math.Atan2(z, Math.Sqrt(x2 + y2)));
            details.ApparentGeocentricDistance  = Math.Sqrt(x2 + y2 + z * z);
            details.ApparentGeocentricLongitude = AASCoordinateTransformation.MapTo0To360Range(AASCoordinateTransformation.RadiansToDegrees(Math.Atan2(y, x)));
            details.ApparentLightTime           = AASElliptical.DistanceToLightTime(details.ApparentGeocentricDistance);

            //Adjust for Aberration
            AAS2DCoordinate Aberration = AASAberration.EclipticAberration(details.ApparentGeocentricLongitude, details.ApparentGeocentricLatitude, JD, bHighPrecision);

            details.ApparentGeocentricLongitude += Aberration.X;
            details.ApparentGeocentricLatitude  += Aberration.Y;

            //convert to the FK5 system
            double DeltaLong = AASFK5.CorrectionInLongitude(details.ApparentGeocentricLongitude, details.ApparentGeocentricLatitude, JD);

            details.ApparentGeocentricLatitude  += AASFK5.CorrectionInLatitude(details.ApparentGeocentricLongitude, JD);
            details.ApparentGeocentricLongitude += DeltaLong;

            //Correct for nutation
            double NutationInLongitude = AASNutation.NutationInLongitude(JD);
            double Epsilon             = AASNutation.TrueObliquityOfEcliptic(JD);

            details.ApparentGeocentricLongitude += AASCoordinateTransformation.DMSToDegrees(0, 0, NutationInLongitude);

            //Convert to RA and Dec
            AAS2DCoordinate ApparentEqu = AASCoordinateTransformation.Ecliptic2Equatorial(details.ApparentGeocentricLongitude, details.ApparentGeocentricLatitude, Epsilon);

            details.ApparentGeocentricRA          = ApparentEqu.X;
            details.ApparentGeocentricDeclination = ApparentEqu.Y;

            return(details);
        }