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/*! # nyx-space [Nyx](https://en.wikipedia.org/wiki/Nyx) is a high fidelity, fast, reliable and validated astrodynamical toolkit library written in Rust. The ultimate goal of this library is to provide a high-speed and scalable replacement for [General Mission Analysis Tool (GMAT)](http://gmat.sourceforge.net/doc/R2018a/help.html). # Tutorial The [tutorial](tutorial/index.html) is a great place to start learning how to use nyx. The target audience is astrodynamics & aerospace engineers. If you are new to Rust, learn the basics on the ["Rust By Example" interactive tutorial](https://doc.rust-lang.org/stable/rust-by-example/). Using nyx isn't hard, despite the code of the library being quite complicated. # Features Unless specified otherwise in the documentation of specific functions, all vectors and matrices are [statically allocated](https://discourse.nphysics.org/t/statically-typed-matrices-whose-size-is-a-multiple-or-another-one/460/4). ## Propagation - Propagation with different Runge Kutta methods (validated in GMAT) - Convenient and explicit definition of the dynamics for a simulation - Propagation to different stopping conditions ## Dynamical models - Multibody dynamics using XB files - Finite burns with fuel depletion (including low thrust / ion propulsion) - Sub-Optimal Control of continuous thrust (e.g. Ruggerio, Petropoulos/Q-law) - Solar radiation pressure modeling - Basic drag models (cannonball) ## Orbit determination - Statistical Orbit Determination: Classical and Extended Kalman Filter - Orbit Determination with multibody dynamics - Smoothing and iterations of CKFs - Square Root Information Filer (SRIF) - An easy-to-use OD user interface - State noise compensation (SNC) ## Celestial computations - Orbital state manipulation (from GMAT source code and validated in GMAT) - Planetary and Solar eclipse and visibility computation - Light-time corrections and abberations # Usage Put this in your `Cargo.toml`: ```toml [dependencies] nyx-space = "0.0.20" ``` And add the following to your crate root: ```rust extern crate nyx_space as nyx; ``` */ /// Provides all the propagators / integrators available in `nyx`. pub mod propagators; /// Provides several dynamics used for orbital mechanics and attitude dynamics, which can be elegantly combined. /// /// # Simple two body propagation /// ``` /// extern crate nalgebra as na; /// extern crate hifitime; /// extern crate nyx_space as nyx; /// use hifitime::{Epoch, SECONDS_PER_DAY}; /// use nyx::celestia::{bodies, Cosm, State}; /// use nyx::dynamics::celestial::CelestialDynamics; /// use nyx::dynamics::Dynamics; /// use nyx::propagators::error_ctrl::RSSStepPV; /// use nyx::propagators::{PropOpts, Propagator}; /// /// let cosm = Cosm::from_xb("./de438s"); /// let eme2k = cosm.frame("EME2000"); /// /// let dt = Epoch::from_mjd_tai(21_545.0); /// let initial_state = State::cartesian(-2436.45, -2436.45, 6891.037, 5.088611, -5.088611, 0.0, dt, eme2k); /// /// println!("Initial state:\n{0}\n{0:o}\n", initial_state); /// /// let prop_time = 24.0 * 3_600.0; /// let accuracy = 1e-12; /// let min_step = 0.1; /// let max_step = 60.0; /// /// let rslt = State::cartesian( /// -5_971.194_376_797_643, /// 3_945.517_912_574_178_4, /// 2_864.620_957_744_429_2, /// 0.049_083_101_605_507_95, /// -4.185_084_125_817_658, /// 5.848_947_462_472_877, /// Epoch::from_mjd_tai(21_546.0), /// eme2k, /// ); /// /// let mut dynamics = CelestialDynamics::two_body(initial_state); /// let mut prop = Propagator::default( /// &mut dynamics, /// &PropOpts::with_adaptive_step(min_step, max_step, accuracy, RSSStepPV {}), /// ); /// prop.until_time_elapsed(prop_time); /// /// assert_eq!(prop.dynamics.state, rslt, "two body prop failed"); /// /// println!("Final state:\n{0}\n{0:o}", prop.dynamics.state); /// ``` /// /// # Multibody propagation of a Halo orbit /// Multibody propagation is **an order of magnitude faster** in nyx than in GMAT. /// In nyx, the following function is executed in 0.14 seconds in release mode. /// ``` /// extern crate nalgebra as na; /// extern crate hifitime; /// extern crate nyx_space as nyx; /// use hifitime::Epoch; /// use na::Vector6; /// use nyx::celestia::{bodies, Cosm, State}; /// use nyx::dynamics::celestial::CelestialDynamics; /// use nyx::propagators::*; /// use nyx::utils::rss_state_errors; /// /// let prop_time = 24.0 * 3_600.0; /// /// let cosm = Cosm::from_xb("./de438s"); /// let eme2k = cosm.frame("EME2000"); /// /// let start_time = Epoch::from_gregorian_tai_at_midnight(2020, 1, 1); /// /// let halo_rcvr = State::cartesian( /// 333_321.004_516, /// -76_134.198_887, /// -20_873.831_939, /// 0.257_153_712, /// 0.930_284_066, /// 0.346_177, /// start_time, /// eme2k, /// ); /// /// // GMAT data /// let rslt = Vector6::new( /// 345_350.664_030_479, /// 5_930.672_047_088, /// 7_333.283_779_286, /// 2.129_819_943e-2, /// 9.566_789_568e-1, /// 3.028_175_811e-1, /// ); /// /// let bodies = vec![bodies::EARTH_MOON, bodies::SUN, bodies::JUPITER_BARYCENTER]; /// let mut dynamics = CelestialDynamics::new(halo_rcvr, bodies, &cosm); /// /// let mut prop = Propagator::default(&mut dynamics, &PropOpts::default()); /// prop.until_time_elapsed(prop_time); /// let (err_r, err_v) = rss_state_errors(&prop.state_vector(), &rslt); /// /// println!( /// "RSS errors:\tpos = {:.5e} km\tvel = {:.5e} km/s\ninit\t{}\nfinal\t{}", /// err_r, err_v, halo_rcvr, prop.dynamics.state /// ); /// assert!(err_r < 1e-3, format!("multi body failed in position: {:.5e}", err_r)); /// assert!(err_v < 1e-6, format!("multi body failed in velocity: {:.5e}", err_v)); /// ``` pub mod dynamics; /// Provides the solar system planets, and state and (later) ephemeride management. /// /// # State creation and management /// ``` /// extern crate hifitime; /// extern crate nyx_space as nyx; /// /// use hifitime::Epoch; /// use nyx::celestia::{Cosm, State}; /// let mut cosm = Cosm::from_xb("./de438s"); /// // We're actually going to use the GMAT value for Earth GM (de438s has a slightly different value). /// cosm.mut_gm_for_frame("EME2000", 398_600.441_5); /// // In this case, we're creating these states around a Geoid which is Earth. /// let eme2k = cosm.frame("EME2000"); /// let dt = Epoch::from_mjd_tai(21545.0); /// let cart = State::cartesian( /// 5_946.673_548_288_958, /// 1_656.154_606_023_661, /// 2_259.012_129_598_249, /// -3.098_683_050_943_824, /// 4.579_534_132_135_011, /// 6.246_541_551_539_432, /// dt, /// eme2k, /// ); /// /// let kep = State::keplerian( /// 7_712.186_117_895_041, /// 0.158_999_999_999_999_95, /// 53.75369, /// 1.998_632_864_211_17e-5, /// 359.787_880_000_004, /// 25.434_003_407_751_188, /// dt, /// eme2k /// ); /// // We can check whether two states are equal. /// if cart != kep { /// dbg!("{:?}", cart-kep); /// panic!("This won't happen"); /// } /// // Of more interest, we can fetch specific orbital elements. /// println!("sma = {} km inc = {} degrees", cart.sma(), cart.inc()); /// // Note that the state data is stored as X, Y, Z, VX, VY, VZ. /// // Hence, the following print statement may display some rounded values despite /// // being created with fixed values. GMAT has the same "issue" /// // (but `nyx` won't change your script). /// println!("ecc = {} km RAAN = {} degrees", kep.ecc(), cart.raan()); /// ``` pub mod celestia; /// Include utility functions shared by different modules, and which may be useful to engineers. pub mod utils; /// Provides all the input/output needs for this library, including loading of SPICE kernels, and gravity potential files. pub mod io; /// Provides all the orbital determination tools. pub mod od; pub mod tutorial; #[macro_use] extern crate log; #[macro_use] extern crate prost_derive; extern crate hifitime; extern crate nalgebra as na; /// Re-export of hifitime pub mod time { pub use hifitime::*; } /// Re-export nalgebra pub mod dimensions { pub use na::base::*; }