UnitfulAstrodynamics.jl

Astrodynamics with units! Provides common astrodynamics calculations, plotting, and iterative Halo, Kepler, and Lambert solvers.
Author JuliaAstro
Popularity
21 Stars
Updated Last
2 Months Ago
Started In
September 2020

Tests Docs

GeneralAstrodynamics.jl

Common astrodynamics calculations, with units!

Warning

The functionality in this package has being split into constituent packages, including AstrodynamicalModels.jl AstrodynamicalCalculations.jl, AstrodynamicalSolvers.jl, and more. GeneralAstrodynamics.jl is currently being refactored into a super-package, which re-exports the functionality in its constituent packages. Look out for v1.0!

JuliaCon Talk

Check out GeneralAstrodynamics in action at JuliaCon 2021! The talk Going to Jupiter with Julia walks through a simple Jupiter mission design while gently introducing astrodynamics, Julia, and GeneralAstrodynamics.

Features

Restricted Two-body Problem (R2BP)

  • Structures for Cartesian and Keplerian states, and R2BP systems
  • Functions which implement common R2BP equations
  • Kepler and Lambert solvers
  • Orbit propagation and plotting

Circular Restricted Three-body Problem (CR3BP)

  • Structures for dimensioned and normalized Cartesian states, and dimensioned and normalized CR3BP systems
  • Functions which implement common CR3BP equations
  • Analytical and iterative (numerical) Halo orbit solvers
  • Unstable and stable Halo orbit manifold computation
  • Orbit propagation and plotting
  • Zero-velocity curve computation and plotting

N-body Problem (NBP)

  • This was implemented in a previous package version, and is currently being refactored

Envisioned Usage

using GeneralAstrodynamics

orbit = rand(R2BPOrbit)
trajectory = propagate(orbit, orbital_period(orbit))

furnsh(
    de440s(),                   # position and velocity data for nearby planets
    latest_leapseconds_lsk(),   # timekeeping, parsing epochs
    gm_de440(),                 # mass parameters for major solar system bodies
    pck00011(),                 # physical properties of major solar system bodies
)

μ = reduced_mass(
  gm("earth"),
  gm("moon"),
)

orbit, T = let
  u, T = halo(μ, 2; amplitude=1e-2)

  CR3BPOrbit(CartesianState(u), CR3BParameters(μ)), T
end

trajectory = propagate(orbit, T)