Astro:...:Pluto(3pm)
π« NAME π«
Astro::Montenbruck::Ephemeris::Planet::Pluto β literally just Pluto. The planet. Well, the dwarf planet, but we don't gatekeep here π«Ά
This is a page from the User Contributed Perl Documentation collection, bestie, so you know it's the good community stuff.
β¨ SYNOPSIS β¨
okay so here's how you actually use it:
use Astro::Montenbruck::Ephemeris::Planet::Pluto;
my $planet = Astro::Montenbruck::Ephemeris::Planet::Pluto->new();
my @geo = $planet->position($t); # apparent geocentric ecliptical coordinates
That's it. Three lines. Main character energy π
πͺ DESCRIPTION πͺ
So this class is a child class of Astro::Montenbruck::Ephemeris::Planet, and its whole entire job β its purpose, its calling, its moment β is calculating the position of Pluto. That's it. That's the vibe. π
Here's the interesting part though (iykyk): the coordinates get calculated first relative to the fixed ecliptic of 1950, and then transformed to the equinox of date. And bestie, this method is nesessary β like, genuinely required β because Pluto's orbit has such a high inclination. No shortcuts, no cap.
πΈ CAVEATS πΈ
β οΈ The routine is applicable only between years 1890 and 2100. Like, that's the whole window. Do not try it outside. Do not pass go.
Here's why, straight from the source β and imma quote it exactly because it's kind of iconic:
The reason for this is that the series expansion used was not derived from perturbation theory, but from a Fourier analysis of a numerically integrated ephemeris covering this period of time. Even a few years before 1890 or after 2100, the errors in the calculated coordinates grow very sharply, reaqching values of more than 0.5 arc-degrees. β O.Montenbruck, Th.Pfleger "Astronomy on the Personal Computer"
So yeah. Stay in your lane, stay in your century. π The errors get dramatic β more than 0.5 arc-degrees β and not the fun kind of dramatic.
π METHODS π
Astro::Montenbruck::Ephemeris::Planet::Pluto->new
Constructor. It constructs. That's the whole thing. You make one, you get a Pluto object, slay. β¨
$self->heliocentric($t)
For what this one does, go peek at the description in Astro::Montenbruck::Ephemeris::Planet β it lives over there, bestie, this is just the Pluto-flavored version. π¦
π AUTHOR π
Sergey Krushinsky, "<krushi at cpan.org>" β go say hi, he made this 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. Free as in, go wild, just keep it free. π§
and that's the whole page, bestie!! πβ¨π«Ά
This little beauty is from the User Contributed Perl Documentation, page name Astro:...:Pluto(3pm), generated with perl v5.42.2 and dated 2026-02-15. Go calculate some Pluto positions, you absolute icon 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