1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
// SPDX-License-Identifier: BSD-3-Clause
// Copyright (C) 2026 Vallés Puig, Ramon
//! Pluto abbreviated series (Meeus 1998, ch. 37).
//!
//! ## Scientific scope
//!
//! Low-precision heliocentric position of Pluto from the Meeus (1998)
//! abbreviated series (Astronomical Algorithms, 2nd ed., ch. 37).
//! Accurate to ≈ 0.1 arcsec over 1885–2099.
//!
//! The [`pluto_data`] sub-module exposes:
//!
//! * [`pluto_data::PLUTO_ARGUMENTS`] — 43 Delaunay-like argument sets (j, s, p).
//! * [`pluto_data::PLUTO_LONGITUDE_TERMS`] — sine/cosine amplitudes for longitude.
//! * [`pluto_data::PLUTO_LATITUDE_TERMS`] — sine/cosine amplitudes for latitude.
//! * [`pluto_data::PLUTO_RADIUS_TERMS`] — sine/cosine amplitudes for radius.
//!
//! ## References
//!
//! * Meeus, J. (1998). Astronomical Algorithms (2nd ed.). Willmann-Bell. Ch. 37.
/// Argument multipliers for Jupiter (j), Saturn (s), and Pluto (p) mean
/// longitudes in the Meeus (1998) abbreviated Pluto series.
/// Sine (`a`) and cosine (`b`) amplitude pair for a single Pluto series term.
///
/// Longitude and latitude amplitudes are in units of 0.1 µas; radius
/// amplitudes are in units of 1e-7 AU.
/// Provenance for the Pluto abbreviated series.