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Orbis

Full-featured satellite toolkit for Elixir.

SGP4 propagation and high-accuracy coordinate transforms are handled by a Rust NIF. Everything else — pass prediction, orbit determination, conjunction assessment, constellation management, real-time tracking, batch analysis — is pure Elixir (and Nx for GPU workloads).

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Features

Category What it does
Propagation SGP4/SDP4 via the sgp4 Rust crate (Rust NIF)
Coordinate transforms TEME, GCRS, ITRS, geodetic, topocentric — 0 ULP Skyfield parity (Rust NIF)
Ground station Pass prediction, look angles, Doppler shift, RF link budget
Orbit determination Gibbs, Herrick-Gibbs, Gauss angles-only, Lambert/Battin (Rust NIF)
Conjunction assessment Closest approach finder validated against the Iridium 33 / Cosmos 2251 collision
Eclipse prediction Sunlit / penumbra / umbra with shadow fraction
Atmospheric density NRLMSISE-00 model, surface to ~1000 km (Rust NIF)
JPL ephemeris SPK/BSP reader for Sun, Moon, planets (Rust NIF)
Live data CelesTrak TLE/OMM fetching, constellation loading, name search
Real-time tracking GenServer with PubSub-compatible broadcasts
RF primitives FSPL, EIRP, C/N₀, link margin, dish gain
Batch analysis Nx-powered tensorized geometry, visibility, and RF (GPU-ready via EXLA/Torchx)
FormatsOrbis.Elements with TLE and OMM parsers/encoders

Installation

def deps do
  [{:orbis, "~> 0.5.0"}]
end

Requires Rust for compiling the NIF.

Quick Start

# Fetch the ISS TLE from CelesTrak
{:ok, [iss]} = Orbis.CelesTrak.fetch_tle(25544)

# Propagate to now
{:ok, teme} = Orbis.propagate(iss, DateTime.utc_now())
teme.position   # {x, y, z} km
teme.velocity   # {vx, vy, vz} km/s

# Where is it over the Earth?
{:ok, geo} = Orbis.geodetic(iss, DateTime.utc_now())
# %{latitude: 23.4, longitude: -45.6, altitude_km: 420.1}

Usage

Parse from TLE or OMM

# Two-Line Element format
{:ok, elements} = Orbis.Format.TLE.parse(line1, line2)

# OMM JSON (CelesTrak / Space-Track)
{:ok, elements} = Orbis.Format.OMM.parse(omm_json_map)

# Encode back to either format
{line1, line2} = Orbis.Format.TLE.encode(elements)
omm_map = Orbis.Format.OMM.encode(elements)

The Orbis.Elements struct is format-agnostic — parse from any source, serialize to any format.

Coordinate Transforms

gcrs = Orbis.teme_to_gcrs(teme, datetime)

station = %{latitude: 40.7128, longitude: -74.006, altitude_m: 10.0}
{:ok, geo} = Orbis.geodetic(elements, datetime)
{:ok, look} = Orbis.look_angle(elements, datetime, station)
# %{azimuth: 359.6, elevation: -41.9, range_km: 9130.5}

The GCRS transform includes IAU2000A nutation (1365 terms), IAU2006 precession, frame bias, and time scale conversions (UTC→TAI→TT→TDB→UT1).

Constellation Management

{:ok, constellation} = Orbis.Constellation.load("globalstar")
constellation.count  #=> 85

# Propagate all satellites in parallel
positions = Orbis.Constellation.propagate_all(constellation, DateTime.utc_now())

# Find visible satellites from a ground station
visible = Orbis.Constellation.visible_from(constellation, station, datetime)

Real-Time Tracking

{:ok, tracker} = Orbis.Tracker.start_link(elements, interval_ms: 1000)
Orbis.Tracker.subscribe(tracker)

receive do
  {:orbis_tracker, _pid, state} ->
    IO.puts("#{state.geodetic.latitude}, #{state.geodetic.longitude}")
end

Pass Prediction

passes = Orbis.Passes.predict(elements, station,
  ~U[2024-01-01 00:00:00Z], ~U[2024-01-02 00:00:00Z])

for pass <- passes do
  IO.puts("Rise: #{pass.rise} | Max el: #{pass.max_elevation}° | Set: #{pass.set}")
end

Conjunction Assessment

approaches = Orbis.Conjunction.find(elements1, elements2,
  end_min: 2880.0, step_min: 1.0, threshold_km: 50.0)

for {tca_min, distance_km} <- approaches do
  IO.puts("TCA: +#{Float.round(tca_min / 60, 1)}h, miss: #{Float.round(distance_km, 2)} km")
end

RF Link Budget

# Path loss from slant range
fspl = Orbis.RF.fspl(look.range_km, 1616.0)  # MHz

# Full link margin
margin = Orbis.RF.link_margin(%{
  eirp_dbw: Orbis.RF.eirp(27.0, 3.0),
  fspl_db: fspl,
  receiver_gt_dbk: -12.0,
  other_losses_db: 3.0,
  required_cn0_dbhz: 35.0
})

Orbit Determination

# Gibbs: 3 position vectors → velocity
{v2, theta12, theta23, copa} = Orbis.IOD.gibbs(r1, r2, r3)

# Gauss: 3 angular observations → full orbit
{r2, v2} = Orbis.IOD.gauss(
  decl1, decl2, decl3, rtasc1, rtasc2, rtasc3,
  jd1, jdf1, jd2, jdf2, jd3, jdf3,
  site1, site2, site3)

# Lambert: transfer orbit between two positions
{v1t, v2t} = Orbis.Lambert.solve(r1, r2, v1, dm, de, nrev, dtsec)

Eclipse & Ephemeris

eph = Orbis.Ephemeris.load("/path/to/de421.bsp")

{:ok, status} = Orbis.Eclipse.check(elements, datetime, eph)
# :sunlit | :penumbra | :umbra

mars = Orbis.Ephemeris.position(eph, :mars, :earth, datetime)

Coordinate Frames

Frame Description
TEME True Equator Mean Equinox — SGP4 output frame
GCRS Geocentric Celestial Reference System — inertial
ITRS International Terrestrial Reference System — Earth-fixed
Geodetic WGS84 latitude, longitude, altitude
Topocentric Azimuth, elevation, range from a ground station

Accuracy

Component Reference Accuracy
TEME→GCRS→ITRS Skyfield 0 ULP (bit-identical)
SGP4 propagation Skyfield < 1 mm (via sgp4 crate)
Gibbs / Herrick-Gibbs Vallado Python 0 ULP
Gauss IOD Vallado Python 1e-12 relative
Lambert (Battin) Vallado Python 1e-12 relative
Conjunction Iridium/Cosmos 2251 < 2 km miss, < 1 min timing
RF (FSPL) Analytical (inverse square law) Exact

License

MIT