SatKit¶
Satellite astrodynamics in Rust, with full Python bindings.
SatKit is a high-performance orbital mechanics library written in Rust with complete Python bindings via PyO3. It handles coordinate transforms, orbit propagation, time systems, gravity models, atmospheric density, and JPL ephemerides -- everything needed for satellite astrodynamics work.
Pre-built wheels are available for Linux, macOS, and Windows on Python 3.10--3.14.
Quick Start¶
The satkit_data package is installed automatically as a dependency and includes gravity models, JPL ephemerides, and Earth orientation parameters -- no extra download step needed. To update space weather and Earth orientation parameters to the latest values, run:
Quick Examples¶
SGP4 propagation¶
import satkit as sk
tle = sk.TLE.from_lines([
"ISS (ZARYA)",
"1 25544U 98067A 24001.50000000 .00016717 00000-0 10270-3 0 9003",
"2 25544 51.6432 351.4697 0007417 130.5364 329.6482 15.48915330299357"
])
pos, vel = sk.sgp4(tle, sk.time(2024, 1, 2))
High-precision propagation¶
import satkit as sk
import numpy as np
r0 = 6378e3 + 500e3 # 500 km altitude
v0 = np.sqrt(sk.consts.mu_earth / r0)
settings = sk.propsettings(
gravity_model=sk.gravmodel.jgm3,
gravity_degree=8,
)
result = sk.propagate(
np.array([r0, 0, 0, 0, v0, 0]),
sk.time(2024, 1, 1),
end=sk.time(2024, 1, 1) + sk.duration.from_days(1),
propsettings=settings,
)
state = result.interp(sk.time(2024, 1, 1) + sk.duration.from_hours(6))
Coordinate transforms¶
import satkit as sk
time = sk.time(2024, 1, 1, 12, 0, 0)
coord = sk.itrfcoord(latitude_deg=42.0, longitude_deg=-71.0, altitude=100.0)
q = sk.frametransform.qitrf2gcrf(time)
gcrf_pos = q * coord.vector
Features¶
Coordinate Frames¶
Full IAU-2006/2000 reduction with Earth orientation parameters:
| Frame | Description |
|---|---|
| ITRF | International Terrestrial Reference Frame (Earth-fixed) |
| GCRF | Geocentric Celestial Reference Frame (inertial) |
| TEME | True Equator Mean Equinox (SGP4 output frame) |
| CIRS | Celestial Intermediate Reference System |
| TIRS | Terrestrial Intermediate Reference System |
| Geodetic | Latitude / longitude / altitude (WGS-84) |
Plus ENU, NED, and geodesic distance (Vincenty) utilities.
Orbit Propagation¶
- Numerical -- Adaptive Runge-Kutta integrators (9(8), 8(7), 6(5), 5(4)) with dense output, state transition matrix, and configurable force models
- SGP4 -- Standard TLE/OMM propagator with TLE fitting from precision states
- Keplerian -- Analytical two-body propagation
- Lambert -- Multi-revolution Lambert targeting for orbit transfer design
Force Models¶
- Earth gravity: JGM2, JGM3, EGM96, ITU GRACE16 (spherical harmonics up to degree/order 360)
- Third-body gravity: Sun and Moon via JPL DE440/441 ephemerides
- Atmospheric drag: NRLMSISE-00 (pure Rust) with automatic space weather data
- Solar radiation pressure: Cannonball model with shadow function
Time Systems¶
Seamless conversion between UTC, TAI, TT, TDB, UT1, and GPS time scales with full leap-second handling.
Solar System¶
- JPL DE440/DE441 ephemerides for all planets, Sun, Moon, and barycenters
- Fast analytical Sun/Moon models for lower-precision work
- Sunrise/sunset and Moon phase calculations
Quick Links¶
| Installation | Install from PyPI or build from source |
| Data Files | Required data files for calculations |
| Learn | Tutorials and theory — from basics to advanced topics |
| API Reference | Full Python API documentation |
| Rust API (docs.rs) | Rust API reference |
| GitHub | Source code and issue tracker |
Author¶
Steven Michael (ssmichael@gmail.com)
Please reach out if you find errors in code or calculations, are interested in contributing to this repository, or have suggestions for improvements to the API.