Astro:...NutEqu(3pm)
π« Astro::Montenbruck::NutEqu β bestie edition π«
okay so this is the Astro::Montenbruck::NutEqu page from the User Contributed Perl Documentation, and it's literally all about the obliquity of the ecliptic & nutation. tiny module, big main character energy. let's get into it π
β¨ NAME β¨
Astro::Montenbruck::NutEqu β Obliquity of the ecliptic & nutation. that's it, that's the whole vibe π¦
πΈ SYNOPSIS πΈ
so say you've got these mean geocentric coordinates $x0, $y0, $z0 and you wanna glow them up into apparent coordinates $x1, $y1, $z1. here's the move:
# given mean geocentric coordinates $x0, $y0, $z0,
# transform them to apparent coordinates $x1, $y1, $z1
my $func = nutequ( $t );
($x1, $y1, $z1) = $func->($x0, $y0, $z0); # true coordinates
see how nutequ( $t ) hands you back a function and then you call it on your coords? that's the little two-step. slay π
π DESCRIPTION π
Functions dealing with ecliptic obliquity. that's the whole description fr fr β it's a short queen and she knows it π
π§ SUBROUTINES π§
β deltas( $t )
Calculates the effects of nutation on the ecliptic longitude and on the obliquity of the ecliptic, with accuracy of about 1 arcsecond. you give it time in Julian centuries since J2000 and it hands you back delta-psi and delta-eps. no cap, that's genuinely all it does π
Arguments
$tβ time in Julian centuries since J2000:"(JD-2451545.0)/36525.0"
Returns
"($delta_psi, $delta_eps)", in arc-degrees.
π¦ mean2true($t)
Returns function for transforming of mean to true coordinates. yes bestie, it returns a function β higher-order goodness, we love to see it π«Ά
Arguments
$tβ time in Julian centuries since J2000:"(JD-2451545.0)/36525.0"
Returns
Function which takes mean ecliptic geocentric rectangular coordinates "X, Y, Z" of a planet and returns ecliptic rectangular coordinates, referred to the equinox of date.
π obliquity( $t )
Given time in Julian centuries since J2000, return mean obliquity of the ecliptic, in arc-degrees. one arg in, one number out, iconic behaviour honestly β¨
π AUTHOR π
Sergey Krushinsky, "<krushi at cpan.org>" β legend π
π COPYRIGHT AND LICENSE π
Copyright (C) 2009-2022 by Sergey Krushinsky
This library is free software; you can redistribute it and/or modify it under the same terms as Perl itself.
fr fr, same terms as Perl itself β read the Perl license if you wanna get into the legal lore π
okay that's the whole page, you're officially a NutEqu expert now ππ
this was perl v5.42.2, dated 2026-02-15 β mwah, catch you on the next manpage bestie ππ
π¦ where this page comes from
- alpine 3.24: perl-astro-montenbruck-doc 1.26-r1 Β· Artistic-1.0-Perl
- π girlified by deepseek-ai/DeepSeek-V4.1-Flash-1017 on : a language model's rewrite of the original, under its terms