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package Astro::Montenbruck::Ephemeris::Planet::Sun; |
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use strict; |
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use warnings; |
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use base qw/Astro::Montenbruck::Ephemeris::Planet/; |
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use Math::Trig qw/:pi rad2deg/; |
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use Astro::Montenbruck::MathUtils qw /frac ARCS reduce_rad/; |
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use Astro::Montenbruck::Ephemeris::Pert qw/pert/; |
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use Astro::Montenbruck::Ephemeris::Planet qw/$SU/; |
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1195
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our $VERSION = 0.01; |
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sub new { |
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my $class = shift; |
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$class->SUPER::new( id => $SU ); |
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} |
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sub position { |
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my ( $self, $t ) = @_; |
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# mean anomalies of planets and mean arguments of lunar orbit [rad] |
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my $m2 = pi2 * frac( 0.1387306 + 162.5485917 * $t ); |
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my $m3 = pi2 * frac( 0.9931266 + 99.9973604 * $t ); |
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my $m4 = pi2 * frac( 0.0543250 + 53.1666028 * $t ); |
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my $m5 = pi2 * frac( 0.0551750 + 8.4293972 * $t ); |
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my $m6 = pi2 * frac( 0.8816500 + 3.3938722 * $t ); |
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my $d = pi2 * frac( 0.8274 + 1236.8531 * $t ); |
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my $a = pi2 * frac( 0.3749 + 1325.5524 * $t ); |
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my $u = pi2 * frac( 0.2591 + 1342.2278 * $t ); |
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my ( $dl, $dr, $db ) = ( 0, 0, 0 ); # Corrections in longitude ["], |
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my $pert_cb = sub { $dl += $_[0]; $dr += $_[1]; $db += $_[2] }; |
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355
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# Keplerian terms and perturbations by Venus |
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my $term = pert( |
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T => $t, |
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M => $m3, |
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m => $m2, |
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I_min => 0, |
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I_max => 7, |
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i_min => -6, |
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i_max => 0, |
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callback => $pert_cb |
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); |
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$term->( 1, 0, 0, -0.22, 6892.76, -16707.37, -0.54, 0, 0 ); |
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$term->( 1, 0, 1, -0.06, -17.35, 42.04, -0.15, 0.00, 0.00 ); |
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$term->( 1, 0, 2, -0.01, -0.05, 0.13, -0.02, 0.00, 0.00 ); |
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$term->( 2, 0, 0, 0.00, 71.98, -139.57, 0.00, 0.00, 0.00 ); |
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$term->( 2, 0, 1, 0.00, -0.36, 0.70, 0.00, 0.00, 0.00 ); |
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$term->( 3, 0, 0, 0.00, 1.04, -1.75, 0.00, 0.00, 0.00 ); |
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$term->( 0, -1, 0, 0.03, -0.07, -0.16, -0.07, 0.02, -0.02 ); |
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$term->( 1, -1, 0, 2.35, -4.23, -4.75, -2.64, 0.00, 0.00 ); |
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$term->( 1, -2, 0, -0.10, 0.06, 0.12, 0.20, 0.02, 0.00 ); |
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$term->( 2, -1, 0, -0.06, -0.03, 0.20, -0.01, 0.01, -0.09 ); |
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$term->( 2, -2, 0, -4.70, 2.90, 8.28, 13.42, 0.01, -0.01 ); |
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$term->( 3, -2, 0, 1.80, -1.74, -1.44, -1.57, 0.04, -0.06 ); |
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$term->( 3, -3, 0, -0.67, 0.03, 0.11, 2.43, 0.01, 0.00 ); |
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$term->( 4, -2, 0, 0.03, -0.03, 0.10, 0.09, 0.01, -0.01 ); |
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$term->( 4, -3, 0, 1.51, -0.40, -0.88, -3.36, 0.18, -0.10 ); |
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$term->( 4, -4, 0, -0.19, -0.09, -0.38, 0.77, 0.00, 0.00 ); |
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$term->( 5, -3, 0, 0.76, -0.68, 0.30, 0.37, 0.01, 0.00 ); |
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$term->( 5, -4, 0, -0.14, -0.04, -0.11, 0.43, -0.03, 0.00 ); |
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$term->( 5, -5, 0, -0.05, -0.07, -0.31, 0.21, 0.00, 0.00 ); |
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$term->( 6, -4, 0, 0.15, -0.04, -0.06, -0.21, 0.01, 0.00 ); |
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$term->( 6, -5, 0, -0.03, -0.03, -0.09, 0.09, -0.01, 0.00 ); |
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$term->( 6, -6, 0, 0.00, -0.04, -0.18, 0.02, 0.00, 0.00 ); |
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$term->( 7, -5, 0, -0.12, -0.03, -0.08, 0.31, -0.02, -0.01 ); |
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# perturbations by Mars |
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$term = pert( |
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T => $t, |
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M => $m3, |
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m => $m4, |
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I_min => 1, |
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I_max => 5, |
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i_min => -8, |
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i_max => -1, |
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callback => $pert_cb |
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); |
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$term->( 1, -1, 0, -0.22, 0.17, -0.21, -0.27, 0.00, 0.00 ); |
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$term->( 1, -2, 0, -1.66, 0.62, 0.16, 0.28, 0.00, 0.00 ); |
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$term->( 2, -2, 0, 1.96, 0.57, -1.32, 4.55, 0.00, 0.01 ); |
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$term->( 2, -3, 0, 0.40, 0.15, -0.17, 0.46, 0.00, 0.00 ); |
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$term->( 2, -4, 0, 0.53, 0.26, 0.09, -0.22, 0.00, 0.00 ); |
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$term->( 3, -3, 0, 0.05, 0.12, -0.35, 0.15, 0.00, 0.00 ); |
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$term->( 3, -4, 0, -0.13, -0.48, 1.06, -0.29, 0.01, 0.00 ); |
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$term->( 3, -5, 0, -0.04, -0.20, 0.20, -0.04, 0.00, 0.00 ); |
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$term->( 4, -4, 0, 0.00, -0.03, 0.10, 0.04, 0.00, 0.00 ); |
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$term->( 4, -5, 0, 0.05, -0.07, 0.20, 0.14, 0.00, 0.00 ); |
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$term->( 4, -6, 0, -0.10, 0.11, -0.23, -0.22, 0.00, 0.00 ); |
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$term->( 5, -7, 0, -0.05, 0.00, 0.01, -0.14, 0.00, 0.00 ); |
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$term->( 5, -8, 0, 0.05, 0.01, -0.02, 0.10, 0.00, 0.00 ); |
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97
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# perturbations by Sun |
98
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13
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$term = pert( |
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T => $t, |
100
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M => $m3, |
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m => $m5, |
102
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I_min => -1, |
103
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I_max => 3, |
104
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i_min => -4, |
105
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i_max => -1, |
106
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callback => $pert_cb |
107
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); |
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$term->( -1, -1, 0, 0.01, 0.07, 0.18, -0.02, 0.00, -0.02 ); |
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$term->( 0, -1, 0, -0.31, 2.58, 0.52, 0.34, 0.02, 0.00 ); |
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$term->( 1, -1, 0, -7.21, -0.06, 0.13, -16.27, 0.00, -0.02 ); |
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$term->( 1, -2, 0, -0.54, -1.52, 3.09, -1.12, 0.01, -0.17 ); |
112
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$term->( 1, -3, 0, -0.03, -0.21, 0.38, -0.06, 0.00, -0.02 ); |
113
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15
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$term->( 2, -1, 0, -0.16, 0.05, -0.18, -0.31, 0.01, 0.00 ); |
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$term->( 2, -2, 0, 0.14, -2.73, 9.23, 0.48, 0.00, 0.00 ); |
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$term->( 2, -3, 0, 0.07, -0.55, 1.83, 0.25, 0.01, 0.00 ); |
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$term->( 2, -4, 0, 0.02, -0.08, 0.25, 0.06, 0.00, 0.00 ); |
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$term->( 3, -2, 0, 0.01, -0.07, 0.16, 0.04, 0.00, 0.00 ); |
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$term->( 3, -3, 0, -0.16, -0.03, 0.08, -0.64, 0.00, 0.00 ); |
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$term->( 3, -4, 0, -0.04, -0.01, 0.03, -0.17, 0.00, 0.00 ); |
120
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121
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# perturbations by Saturn |
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$term = pert( |
123
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T => $t, |
124
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M => $m3, |
125
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m => $m6, |
126
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I_min => -0, |
127
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I_max => 2, |
128
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i_min => -2, |
129
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i_max => -1, |
130
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callback => $pert_cb |
131
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); |
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$term->( 0, -1, 0, 0.00, 0.32, 0.01, 0.00, 0.00, 0.00 ); |
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$term->( 1, -1, 0, -0.08, -0.41, 0.97, -0.18, 0.00, -0.01 ); |
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$term->( 1, -2, 0, 0.04, 0.10, -0.23, 0.10, 0.00, 0.00 ); |
135
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14
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$term->( 2, -2, 0, 0.04, 0.10, -0.35, 0.13, 0.00, 0.00 ); |
136
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137
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# difference of Earth-Moon-barycentre and centre of the Earth |
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4
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10
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my $dpa = $d + $a; |
139
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4
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9
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my $dma = $d - $a; |
140
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4
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18
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$dl += |
141
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+6.45 * sin($d) - |
142
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0.42 * sin($dma) + |
143
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0.18 * sin($dpa) + |
144
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0.17 * sin( $d - $m3 ) - |
145
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0.06 * sin( $d + $m3 ); |
146
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147
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4
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14
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$dr += |
148
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+30.76 * cos($d) - |
149
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3.06 * cos($dma) + |
150
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0.85 * cos($dpa) - |
151
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0.58 * cos( $d + $m3 ) + |
152
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0.57 * cos( $d - $m3 ); |
153
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154
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4
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9
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$db += +0.576 * sin($u); |
155
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156
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# long-periodic perturbations |
157
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4
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19
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$dl += |
158
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+6.40 * sin( pi2 * ( 0.6983 + 0.0561 * $t ) ) + |
159
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1.87 * sin( pi2 * ( 0.5764 + 0.4174 * $t ) ) + |
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0.27 * sin( pi2 * ( 0.4189 + 0.3306 * $t ) ) + |
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0.20 * sin( pi2 * ( 0.3581 + 2.4814 * $t ) ); |
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# ecliptic coordinates ([rad],[AU]) |
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pi2 * frac( |
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0.7859453 + $m3 / pi2 + |
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( ( 6191.2 + 1.1 * $t ) * $t + $dl ) / 1296.0e3 |
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) |
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); |
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rad2deg($l), rad2deg($b), $r; |
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} |
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1; |
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__END__ |
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=pod |
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=encoding UTF-8 |
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=head1 NAME |
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Astro::Montenbruck::Ephemeris::Planet::Sun - Sun. |
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=head1 SYNOPSIS |
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use Astro::Montenbruck::Ephemeris::Planet::Sun; |
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my $planet = Astro::Montenbruck::Ephemeris::Planet::Sun->new(); |
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my @geo = $planet->position($t); # apparent geocentric ecliptical coordinates |
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=head1 DESCRIPTION |
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Child class of L<Astro::Montenbruck::Ephemeris::Planet>, responsible for calculating |
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B<Sun> position. |
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=head1 METHODS |
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=head2 Astro::Montenbruck::Ephemeris::Planet::Sun->new |
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Constructor. |
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=head2 $self->position($t) |
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Geocentric ecliptic coordinates of the Sun |
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=head3 Arguments |
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=over |
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=item B<$t> â time in Julian centuries since J2000: (JD-2451545.0)/36525.0 |
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=back |
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=head3 Returns |
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Hash of geocentric ecliptical coordinates. |
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=over |
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=item * B<x> â geocentric longitude, arc-degrees |
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=item * B<y> â geocentric latitude, arc-degrees |
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=item * B<z> â distance from Earth, AU |
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=back |
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232
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=head1 AUTHOR |
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234
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Sergey Krushinsky, C<< <krushi at cpan.org> >> |
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236
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=head1 COPYRIGHT AND LICENSE |
237
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238
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Copyright (C) 2009-2019 by Sergey Krushinsky |
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240
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This library is free software; you can redistribute it and/or modify |
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it under the same terms as Perl itself. |
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243
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=cut |