Typed astronomy & satellite mechanics in safe Rust.
Siderust provides ephemerides, coordinate transforms, time-scale handling, and orbit-analysis building blocks for scientific applications. The primary Rust implementation avoids unsafe; allocation behavior depends on the enabled subsystems and is documented at the module level. External reference fixtures are being expanded, so scientific claims should be read against the validation tests that ship with the crate.
- Supported Feature Flags
- Features
- Installation
- Coordinate Systems
- Units & Physical Quantities
- Quick Start
- Examples
- Crate Layout
- Roadmap
- Contributing
- License
- Acknowledgments
| Feature | Default | What it enables |
|---|---|---|
serde |
✔ | Serialize / Deserialize on public types (default) |
| (base) | VSOP87 + ELP2000-82B analytical ephemerides, full coordinate/altitude API | |
de440 |
JPL DE440 Chebyshev ephemeris backend (1550–2650 CE) | |
de441 |
JPL DE441 Chebyshev ephemeris backend (extended coverage) | |
atmosphere |
Atmospheric tables and radiative transfer helpers | |
photometry |
Photometric passbands and throughput unit (Johnson–Cousins UBVRI) | |
spice |
High-level SPICE kernel context (SpiceContext, KernelSet) |
|
pod |
Precise Orbit Determination toolkit (WLS, EKF, force models, I/O) | |
pod-parquet |
Parquet residuals writer (implies pod) |
|
pod-doris |
DORIS RINEX observation parser (implies pod) |
|
runtime-data |
Runtime dataset-loading helpers via siderust-archive |
Note:
no_stdandf128quad‑precision are not supported today. The crate depends onstd‑only libraries such aschrono. Sub‑cratesqttyandqtty-coredo offerno_stdsupport independently. C ABI bindings live in the separatesiderust-fficrate rather than asiderustfeature flag.
| Category | What you get |
|---|---|
| Coordinate Systems | Position and spherical Direction types parameterised by ReferenceCenter, ReferenceFrame, and Unit. Compile‑time guarantees prevent mixing frames by accident. |
| Target Tracking | Target<T> couples any coordinate with an observation epoch and optional ProperMotion, enabling extrapolation & filtering. |
| Physical Units | Strongly typed Mass, Length, Angle, Velocity, Duration & more via the qtty crate, dimensional correctness at compile time. |
| Celestial Mechanics | VSOP87 & ELP2000 theories, Pluto (Meeus/Williams), light‑time & aberration, nutation & precession, apparent Sun & Moon, culmination searches, SGP4/TLE propagation. |
| Ephemeris Backends | Pluggable Ephemeris trait with three backends, Vsop87Ephemeris (always available), De440Ephemeris, and De441Ephemeris (feature-gated JPL DE4xx). |
| Altitude API | Unified AltitudePeriodsProvider trait for Sun, Moon, stars, and arbitrary ICRS directions, find crossings, culminations, altitude ranges, and above/below‑threshold periods. |
| Catalogs & Bodies | Built‑in Sun→Neptune, asteroids (Ceres, Bennu, Apophis), comets (Halley, Encke, Hale-Bopp), a starter star catalog, + helpers for custom datasets. |
| Observatories | Predefined sites (Roque de los Muchachos, El Paranal, Mauna Kea, La Silla) with ObserverSite for topocentric transforms. |
Coordinate algebra and reusable conic geometry are provided by affn; Kepler-equation solving and domain-neutral conic propagation live in keplerian; siderust adds astronomy-specific time, frame transforms, ephemeris backends, and body/observer orchestration on top.
Siderust is built on two cross-cutting principles documented in
doc/conventions.md:
-
Typed quantities everywhere. Every scalar that has physical meaning — pressures, scale heights, optical depths, airmasses, albedos, illumination fractions, CIP coordinates — is a
qttynewtype. Passing a rawf64where aHectopascalsorKilometersis expected is a compile-time error. -
Phantom-typed model selection. Algorithm variants (e.g. nutation models) are selected at the call site via zero-sized phantom type parameters such as
to_frame_as::<EquatorialFrame, Iau2006A>(jd). There are no runtime enums to match on. Dispatch is fully monomorphised.
- Stellar aberration uses the full special-relativistic (Lorentz) formula per IERS Conventions (2020, §7.2); annual uses VSOP87E barycentric Earth velocity and topocentric adds a diurnal
ω×rterm. - The Earth-orientation chain now exposes public frame transforms for
GCRS ↔ CIRS ↔ TIRS ↔ ITRF/ECEF, plus the usual inertial and operational frames (ICRS,ICRF,EME2000,TEME,Galactic, planetary body-fixed). - Local orbital frames (
RTN,LVLH,VNC) and covariance transport in those frames are first-class via [astro::dynamics::frames::LocalOrbitalFrame] and [astro::dynamics::covariance::StateCovariance], built from a typed [OrbitState].
Large scientific datasets — VSOP87, IAU 2000A nutation, ELP2000-82B,
Sun-Earth Lagrange Chebyshev kernels, SPICE time/frame/constants kernels,
and dataset generators/validators — live in the separate
Siderust/archive repository, attached
here as the archive/ git submodule.
After cloning Siderust, initialise the submodule:
git submodule update --init --recursiveAll archive metadata uses TOML (MANIFEST.toml, per-family
manifest.toml). Binary payloads use their authoritative formats (SPICE
.bsp, Siderust Chebyshev Kernel .sck, raw .dat). The archive layout,
manifest schema, and regeneration recipes are documented in
archive/README.md and
archive/schema/archive-manifest-v1.md.
The default siderust build does not require a separate archive checkout.
Large scientific datasets (VSOP87, ELP2000, nutation, gravity, atmosphere, Pluto)
are embedded via the siderust-archive
crate which is a regular Cargo dependency. JPL DE4xx kernels are resolved at
runtime from the local filesystem or downloaded on demand via runtime-data.
Add to your Cargo.toml:
[dependencies]
siderust = "0.8"VSOP87/ELP2000 coefficients, nutation tables, and EOP data are provided by
siderust-archive (scientific
datasets, manifests, checksums, provenance) and
tempoch (UTC/TAI/TT/UT1/TDB time scales,
ΔT, and EOP freshness). Optional JPL kernels are downloaded on demand when the
corresponding feature is enabled; see doc/datasets.md.
Siderust always includes Vsop87Ephemeris (VSOP87 + ELP2000-82B).
Optional features add JPL backends:
de440→De440Ephemeris(1550–2650 CE)de441→De441Ephemeris(extended coverage from NAIFde441_part-2.bsp)
DefaultEphemeris selects the best available:
De441Ephemeriswhende441is enabled- otherwise
De440Ephemeriswhende440is enabled - otherwise
Vsop87Ephemeris
- VSOP87-only (explicit)
[dependencies]
siderust = { version = "0.8", default-features = false }- Enable DE440
[dependencies]
siderust = { version = "0.8", features = ["de440"] }- Enable DE441
[dependencies]
siderust = { version = "0.8", features = ["de441"] }- Combine backends in one binary
use siderust::ephemeris::{Ephemeris, Vsop87Ephemeris};
use siderust::time::JulianDate;
let jd = JulianDate::J2000;
// Analytical series (always available)
let earth_vsop = Vsop87Ephemeris::earth_heliocentric(jd);// With `de441` feature enabled:
use siderust::ephemeris::De441Ephemeris;
let earth_jpl = De441Ephemeris::earth_heliocentric(jd);You can combine ephemeris features with others (for example serde):
[dependencies]
siderust = { version = "0.8", features = ["de441", "serde"] }When JPL features are enabled, build scripts may download:
de440.bsp(~120 MB)de441_part-2.bsp(~1.65 GB)
Default checked-in behavior is real JPL builds (no global stubbing).
By default, downloaded JPL kernels are cached under Cargo's build output directory (OUT_DIR),
so cargo clean (or switching targets) can force a re-download.
To download once and reuse across builds, set SIDERUST_DATASETS_DIR to a persistent location
and prefetch the kernel you need:
export SIDERUST_DATASETS_DIR="$HOME/.cache/siderust"
../archive/scripts/prefetch_datasets.sh --de440 # downloads $SIDERUST_DATASETS_DIR/de440_dataset/de440.bspNotes:
cargo test --all-featuresenablesde440, so it will try to acquirede440.bspif missing.- If the file is already present in the datasets directory, the build script reuses it.
Real JPL mode (recommended for representative DE440/DE441 behavior):
unset SIDERUST_JPL_STUB
cargo test --features de440
cargo test --features de441Offline/stub mode (explicit opt-in for fast local loops):
SIDERUST_JPL_STUB=all cargo check --all-featuresSupported stub values:
de441: stubs DE441 only (De441Ephemerisis mocked toVsop87Ephemeris).de440: stubs DE440 only.de440,de441orall(also1,true,yes,on): stubs both.
Optional local override file (keep untracked):
# .cargo/config.local.toml
[env]
SIDERUST_JPL_STUB = "all"Use it explicitly:
cargo --config .cargo/config.local.toml check --all-featuresCaveat:
- Stubbed DE datasets compile successfully, but low-level DE calls are unavailable at runtime.
de441has a high-level mock backend (De441Ephemeris -> Vsop87Ephemeris).de440is compile-only when stubbed; direct runtime calls toDe440Ephemeriswill panic.
Coverage:
- Fallible JPL APIs such as
try_position,try_velocity, andtry_position_velocityreturn an error outside the Chebyshev segment coverage. - The legacy infallible JPL APIs are retained for compatibility and panic with an explicit out-of-range message instead of silently extrapolating.
- Earth-orientation lookups are keyed by UTC/MJD. The default IERS provider uses
tempoch's bundled EOP data and reports missing coverage rather than fabricating zero EOP values. UseNullEoponly when a documented zero-EOP approximation is intended.
Siderust encodes both the origin and the orientation of every coordinate at the type level:
use siderust::coordinates::{cartesian, centers::*, frames::*};
use qtty::Au;
// Position of Mars in the Heliocentric Ecliptic frame
let mars_helio = cartesian::Position::<Heliocentric, EclipticMeanJ2000, Au>::new(1.5, 0.0, 0.0);Impossible states (e.g. adding heliocentric and geocentric positions) simply do not compile.
The public frame set includes:
- inertial / catalogue frames:
ICRS,ICRF,EquatorialMeanJ2000,EME2000,EquatorialMeanOfDate,EquatorialTrueOfDate,FK4B1950,Galactic - Earth-rotation chain frames:
GCRS,CIRS,TIRS,ITRF,ECEF - operational / mission frames:
TEME,Horizontal, and the planetary body-fixed frames
For most centers (Barycentric, Heliocentric, Geocentric) all invariants are
enforced at compile time with zero runtime cost (Params = ()).
Parameterized centers (Topocentric, Bodycentric) carry runtime data
(e.g., ObserverSite). The center type is still checked at compile time, but
parameter equality (e.g., "are these two positions at the same site?") is
checked at runtime:
| API | Behaviour on mismatch |
|---|---|
pos_a - pos_b / distance_to |
assert! (panics in all builds) |
checked_sub / try_distance_to |
Returns Err(CenterParamsMismatchError) |
ObserverSite::try_new |
Validates lat/lon ranges, returns Result |
Siderust uses the qtty crate for dimensionally
typed quantities. The compiler prevents mixing incompatible units:
use qtty::*;
let distance = AstronomicalUnits::new(1.523); // Mars semi-major axis
let period = Days::new(686.97);
// distance + period → compile error (length + time)Common unit types: AstronomicalUnit (Au), Kilometer (Km), Meter,
Degree, Radian, Day, Second, AuPerDay, and many more.
use siderust::{
bodies::Mars,
time::JulianDate,
};
use chrono::prelude::*;
// 1. Select an epoch (UTC now → JD)
let jd = JulianDate::from_utc(Utc::now());
// 2. Compute barycentric ecliptic coordinates via VSOP87
let mars = Mars::vsop87e(jd);
// 3. Print Mars's barycentric ecliptic position
println!("{}", mars.position);The examples/ directory is a curated tour of the crate’s major building blocks
(coordinates, transforms, altitude periods, ephemeris backends, serialization).
- Browse:
examples/README.md - Run one:
cargo run --example 01_basic_coordinates
Feature-gated examples:
# JPL DE4xx (may download large BSP datasets unless you explicitly stub)
cargo run --example 12_runtime_ephemeris --features de440
cargo run --example 12_runtime_ephemeris --features de441
# Fast/offline loop: compile JPL features but skip runtime DE calls
SIDERUST_JPL_STUB=all cargo run --example 12_runtime_ephemeris --features de440,de441
# Serde
cargo run --example 11_serde_serialization --features serde├─ astro/ # Aberration, nutation, precession, sidereal time
├─ bodies/ # Planet, Star, Satellite, Asteroid, Comet + built-in catalogs
├─ calculus/
│ ├─ altitude/ # Unified altitude API (AltitudePeriodsProvider trait)
│ ├─ ephemeris/ # Ephemeris trait + VSOP87/DE440/DE441 backends
│ ├─ jpl/ # Shared JPL DE4xx infrastructure (Chebyshev evaluation)
│ ├─ math_core/ # Root-finding (Brent/bisection), extrema, interval assembly
│ ├─ solar/ # Sun altitude, night/day/twilight periods
│ ├─ lunar/ # Moon altitude with topocentric parallax
│ ├─ stellar/ # Analytical star altitude engine
│ ├─ vsop87/ # VSOP87 planetary theory
│ ├─ elp2000/ # ELP2000-82B lunar theory
│ ├─ conic_equations.rs # Siderust wrappers over keplerian solvers
│ └─ pluto # Meeus/Williams Pluto ephemeris
├─ coordinates/ # Cartesian/Spherical types, frames, centers, transforms
├─ mission/ # Mission-analysis building blocks
│ ├─ geometry/ # AzElRange, Fov, TerrainMask, eclipse, orbit-relative geometry
│ ├─ context.rs # MissionContext — runtime aggregation of instruments and sites
│ └─ site.rs # Location — ground-station / observing-site metadata
├─ observatories/ # Predefined observatory locations (Roque, Paranal, Mauna Kea, La Silla)
├─ targets/ # Target<T> with time & ProperMotion
└─ time # Re-export of tempoch: JulianDate, MJD, Period<S>, time scales
- Custom dynamic reference centers (topocentric, bodycentric)
- DE440/DE441 JPL ephemerides
- Unified altitude API (
AltitudePeriodsProvidertrait) - Serde serialization support
- Gaia DR3 star ingestion & cone search
- Relativistic light‑time & gravitational deflection
- Batch orbit determination helpers (LSQ & EKF)
- GPU acceleration via
wgpu(experiment)
Contributions of algorithms, bug fixes or docs are welcome! Please:
- Fork & clone (
git clone) - Create a feature branch
- Run all tests & clippy (
cargo test && cargo clippy -- -D warnings) - Open a PR with a clear description
By participating you agree to follow the Rust Code of Conduct.
Copyright (C) 2026 Vallés Puig, Ramon
This project is licensed under the GNU Affero General Public License v3.0 (AGPL-3.0). The AGPL-3.0 ensures that:
- Any modifications and redistributions of the code (including as a network service) remain free and open.
- End users have access to the full source code, including any improvements or extensions made.
Note for commercial or proprietary use: If you wish to incorporate this code into a closed-source or otherwise differently licensed project, a dual-licensing arrangement can be negotiated. Please contact the authors to discuss terms and conditions for a commercial or proprietary license that suits your needs.
Big thanks to Màrius Montón (@mariusmm) for inviting me to his three-week Rust intro course at the Universitat Autònoma de Barcelona (UAB) in 2024 that nudge set this project in motion.