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use strict;
use Math::Trig qw/:pi/;
use Astro::Montenbruck::MathUtils qw /frac ARCS/;
our $VERSION = 0.01;
sub new {
my $class = shift;
$class->SUPER::new( id => $VE );
}
# Venus heliocentric position
sub heliocentric {
my ( $self, $t ) = @_;
# mean anomalies of planets in [rad]
my $m1 = pi2 * frac( 0.4861431 + 415.2018375 * $t );
my $m2 = pi2 * frac( 0.1400197 + 162.5494552 * $t );
my $m3 = pi2 * frac( 0.9944153 + 99.9982208 * $t );
my $m4 = pi2 * frac( 0.0556297 + 53.1674631 * $t );
my $m5 = pi2 * frac( 0.0567028 + 8.4305083 * $t );
my $m6 = pi2 * frac( 0.8830539 + 3.3947206 * $t );
my ( $dl, $dr, $db ) = ( 0, 0, 0 ); # Corrections in longitude ["]
my $pert_cb = sub { $dl += $_[0]; $dr += $_[1]; $db += $_[2] };
# Perturbations by Mercury
my $term = pert(
T => $t,
M => $m2,
m => $m1,
I_min => 1,
I_max => 5,
i_min => -2,
i_max => -1,
callback => $pert_cb
);
$term->( 1, -1, 0, 0.00, 0.00, 0.06, -0.09, 0.01, 0.00 );
$term->( 2, -1, 0, 0.25, -0.09, -0.09, -0.27, 0.00, 0.00 );
$term->( 4, -2, 0, -0.07, -0.08, -0.14, 0.14, -0.01, -0.01 );
$term->( 5, -2, 0, -0.35, 0.08, 0.02, 0.09, 0.00, 0.00 );
# Keplerian motion and perturbations by the Earth
$term = pert(
T => $t,
M => $m2,
m => $m3,
I_min => 1,
I_max => 8,
i_min => -8,
i_max => 0,
callback => $pert_cb
);
$term->( 1, 0, 0, 2.37, 2793.23, -4899.07, 0.11, 9995.27, 7027.22 );
$term->( 1, 0, 1, 0.10, -19.65, 34.40, 0.22, 64.95, -86.10 );
$term->( 1, 0, 2, 0.06, 0.04, -0.07, 0.11, -0.55, -0.07 );
$term->( 2, 0, 0, -170.42, 73.13, -16.59, 0.00, 67.71, 47.56 );
$term->( 2, 0, 1, 0.93, 2.91, 0.23, 0.00, -0.03, -0.92 );
$term->( 3, 0, 0, -2.31, 0.90, -0.08, 0.00, 0.04, 2.09 );
$term->( 1, -1, 0, -2.38, -4.27, 3.27, -1.82, 0.00, 0.00 );
$term->( 1, -2, 0, 0.09, 0.00, -0.08, 0.05, -0.02, -0.25 );
$term->( 2, -2, 0, -9.57, -5.93, 8.57, -13.83, -0.01, -0.01 );
$term->( 2, -3, 0, -2.47, -2.40, 0.83, -0.95, 0.16, 0.24 );
$term->( 3, -2, 0, -0.09, -0.05, 0.08, -0.13, -0.28, 0.12 );
$term->( 3, -3, 0, 7.12, 0.32, -0.62, 13.76, -0.07, 0.01 );
$term->( 3, -4, 0, -0.65, -0.17, 0.18, -0.73, 0.10, 0.05 );
$term->( 3, -5, 0, -1.08, -0.95, -0.17, 0.22, -0.03, -0.03 );
$term->( 4, -3, 0, 0.06, 0.00, -0.01, 0.08, 0.14, -0.18 );
$term->( 4, -4, 0, 0.93, -0.46, 1.06, 2.13, -0.01, 0.01 );
$term->( 4, -5, 0, -1.53, 0.38, -0.64, -2.54, 0.27, 0.00 );
$term->( 4, -6, 0, -0.17, -0.05, 0.03, -0.11, 0.02, 0.00 );
$term->( 5, -5, 0, 0.18, -0.28, 0.71, 0.47, -0.02, 0.04 );
$term->( 5, -6, 0, 0.15, -0.14, 0.30, 0.31, -0.04, 0.03 );
$term->( 5, -7, 0, -0.08, 0.02, -0.03, -0.11, 0.01, 0.00 );
$term->( 5, -8, 0, -0.23, 0.00, 0.01, -0.04, 0.00, 0.00 );
$term->( 6, -6, 0, 0.01, -0.14, 0.39, 0.04, 0.00, -0.01 );
$term->( 6, -7, 0, 0.02, -0.05, 0.12, 0.04, -0.01, 0.01 );
$term->( 6, -8, 0, 0.10, -0.10, 0.19, 0.19, -0.02, 0.02 );
$term->( 7, -7, 0, -0.03, -0.06, 0.18, -0.08, 0.00, 0.00 );
$term->( 8, -8, 0, -0.03, -0.02, 0.06, -0.08, 0.00, 0.00 );
# Perturbations by Mars
$term = pert(
T => $t,
M => $m2,
m => $m4,
I_min => 1,
I_max => 2,
i_min => -3,
i_max => -2,
callback => $pert_cb
);
$term->( 1, -3, 0, -0.65, 1.02, -0.04, -0.02, -0.02, 0.00 );
$term->( 2, -2, 0, -0.05, 0.04, -0.09, -0.10, 0.00, 0.00 );
$term->( 2, -3, 0, -0.50, 0.45, -0.79, -0.89, 0.01, 0.03 );
# Perturbations by Venus
$term = pert(
T => $t,
M => $m2,
m => $m5,
I_min => 0,
I_max => 3,
i_min => -3,
i_max => -1,
callback => $pert_cb
);
$term->( 0, -1, 0, -0.05, 1.56, 0.16, 0.04, -0.08, -0.04 );
$term->( 1, -1, 0, -2.62, 1.40, -2.35, -4.40, 0.02, 0.03 );
$term->( 1, -2, 0, -0.47, -0.08, 0.12, -0.76, 0.04, -0.18 );
$term->( 2, -2, 0, -0.73, -0.51, 1.27, -1.82, -0.01, 0.01 );
$term->( 2, -3, 0, -0.14, -0.10, 0.25, -0.34, 0.00, 0.00 );
$term->( 3, -3, 0, -0.01, 0.04, -0.11, -0.02, 0.00, 0.00 );
# Perturbations by Saturn
$term = pert(
T => $t,
M => $m2,
m => $m6,
I_min => 0,
I_max => 1,
i_min => -1,
i_max => -1,
callback => $pert_cb
);
$term->( 0, -1, 0, 0.00, 0.21, 0.00, 0.00, 0.00, -0.01 );
$term->( 1, -1, 0, -0.11, -0.14, 0.24, -0.20, 0.01, 0.00 );
# Ecliptic coordinates ([rad],[AU])
$dl +=
+2.74 * sin( pi2 * ( 0.0764 + 0.4174 * $t ) ) +
0.27 * sin( pi2 * ( 0.9201 + 0.3307 * $t ) );
$dl += +1.9 + 1.8 * $t;
my $l =
pi2 *
frac( 0.3654783 + $m2 / pi2 +
( ( 5071.2 + 1.1 * $t ) * $t + $dl ) / 1296.0e3 );
my $r = 0.7233482 - 0.0000002 * $t + $dr * 1.0e-6;
my $b = ( -67.70 + ( 0.04 + 0.01 * $t ) * $t + $db ) / ARCS;
$l, $b, $r;
}
# Intermediate variables for calculating geocentric positions.
sub _lbr_geo {
my ( $self, $t ) = @_;
my $m = pi2 * frac( 0.1400197 + 162.5494552 * $t );
my $dl = 280.00 + 3.79 * cos($m);
my $dr = 1.37 * sin($m);
my $db = 9.54 * cos($m) - 13.57 * sin($m);
$dl, $db, $dr;
}
1;
__END__
=pod
=encoding UTF-8
=head1 NAME
Astro::Montenbruck::Ephemeris::Planet::Venus - Venus.
=head1 SYNOPSIS
use Astro::Montenbruck::Ephemeris::Planet::Venus;
my $planet = Astro::Montenbruck::Ephemeris::Planet::Venus->new();
my @geo = $planet->position($t); # apparent geocentric ecliptical coordinates
=head1 DESCRIPTION
Child class of L<Astro::Montenbruck::Ephemeris::Planet>, responsible for calculating
B<Venus> position.
=head1 METHODS
=head2 Astro::Montenbruck::Ephemeris::Planet::Venus->new
Constructor.
=head2 $self->heliocentric($t)
See description in L<Astro::Montenbruck::Ephemeris::Planet>.
=head1 AUTHOR
Sergey Krushinsky, C<< <krushi at cpan.org> >>
=head1 COPYRIGHT AND LICENSE
Copyright (C) 2009-2019 by Sergey Krushinsky
This library is free software; you can redistribute it and/or modify
it under the same terms as Perl itself.
=cut