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259 lines
7.7 KiB
259 lines
7.7 KiB
#include "orbital_mechanics.h" |
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#include <cmath> |
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#include <cassert> |
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#include <cstdio> |
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void orbital_elements_to_cartesian(OrbitalElements elements, double parent_mass, |
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Vec3* out_position, Vec3* out_velocity) { |
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double a = elements.semi_major_axis; |
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double e = elements.eccentricity; |
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double nu = elements.true_anomaly; |
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double mu = G * parent_mass; |
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double sin_nu = sin(nu); |
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double cos_nu = cos(nu); |
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double p; |
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if (fabs(e - 1.0) < PARABOLIC_TOLERANCE) { |
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p = elements.semi_latus_rectum; |
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} else { |
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p = a * (1.0 - e * e); |
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} |
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double r = p / (1.0 + e * cos_nu); |
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double x_orbital = r * cos_nu; |
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double y_orbital = r * sin_nu; |
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Vec3 position = {x_orbital, y_orbital, 0.0}; |
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double vx_orbital = -sqrt(mu / p) * sin_nu; |
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double vy_orbital = sqrt(mu / p) * (e + cos_nu); |
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Vec3 velocity = {vx_orbital, vy_orbital, 0.0}; |
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double omega = elements.argument_of_periapsis; |
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double i = elements.inclination; |
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double Omega = elements.longitude_of_ascending_node; |
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Mat3 rotation = mat3_rotation_orbital(omega, i, Omega); |
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*out_position = mat3_multiply_vec3(rotation, position); |
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*out_velocity = mat3_multiply_vec3(rotation, velocity); |
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} |
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// Shared solver constants |
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static const double KEPLER_TOLERANCE = 1.0e-10; |
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static const int KEPLER_MAX_ITERATIONS = 50; |
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double get_initial_trial_value(double mean_anomaly, double eccentricity) { |
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return mean_anomaly + eccentricity * sin(mean_anomaly) |
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+ ((pow(eccentricity, 2) / 2.0) * sin(2.0 * mean_anomaly)); |
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} |
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double solve_kepler_elliptical(double mean_anomaly, double eccentricity) { |
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double E = get_initial_trial_value(mean_anomaly, eccentricity); |
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double E_prev = E + 2.0 * KEPLER_TOLERANCE; |
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int iterations = 0; |
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while (fabs(E - E_prev) > KEPLER_TOLERANCE && iterations < KEPLER_MAX_ITERATIONS) { |
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E_prev = E; |
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double sin_E = sin(E); |
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E = E - (E - eccentricity * sin_E - mean_anomaly) / (1.0 - eccentricity * cos(E)); |
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iterations++; |
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} |
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return E; |
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} |
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double solve_kepler_hyperbolic(double mean_anomaly, double eccentricity) { |
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// Initial guess for hyperbolic anomaly |
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double H = mean_anomaly; |
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if (eccentricity * sinh(mean_anomaly) > mean_anomaly) { |
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H = log(2.0 * mean_anomaly / eccentricity); |
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} |
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double H_prev = H + 2.0 * KEPLER_TOLERANCE; |
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int iterations = 0; |
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while (fabs(H - H_prev) > KEPLER_TOLERANCE && iterations < KEPLER_MAX_ITERATIONS) { |
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H_prev = H; |
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double sinh_H = sinh(H); |
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double cosh_H = cosh(H); |
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H = H - (H - eccentricity * sinh_H - mean_anomaly) / (1.0 - eccentricity * cosh_H); |
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iterations++; |
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} |
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return H; |
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} |
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double eccentric_to_true_anomaly(double eccentric_anomaly, double eccentricity) { |
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if (fabs(1.0 - eccentricity) < 0.01) { |
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double E = eccentric_anomaly; |
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double e = eccentricity; |
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double cos_E = cos(E); |
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double sin_E = sin(E); |
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double denominator = 1.0 - e * cos_E; |
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double cos_nu = (cos_E - e) / denominator; |
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double sin_nu = sin_E * sqrt(1.0 - e * e) / denominator; |
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cos_nu = fmax(-1.0, fmin(1.0, cos_nu)); |
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sin_nu = fmax(-1.0, fmin(1.0, sin_nu)); |
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return atan2(sin_nu, cos_nu); |
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} |
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double tan_half_E = tan(eccentric_anomaly / 2.0); |
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double tan_half_nu = sqrt((1.0 + eccentricity) / (1.0 - eccentricity)) * tan_half_E; |
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return 2.0 * atan(tan_half_nu); |
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} |
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double hyperbolic_to_true_anomaly(double hyperbolic_anomaly, double eccentricity) { |
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// Hyperbolic E to true anomaly: tanh(ν/2) = √((e-1)/(e+1)) · tanh(H/2) |
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double tanh_half_H = tanh(hyperbolic_anomaly / 2.0); |
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double tanh_half_nu = sqrt((eccentricity - 1.0) / (eccentricity + 1.0)) * tanh_half_H; |
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return 2.0 * atanh(tanh_half_nu); |
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} |
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double mean_anomaly_to_true_anomaly(double mean_anomaly, double eccentricity) { |
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if (eccentricity < 1.0) { |
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double E = solve_kepler_elliptical(mean_anomaly, eccentricity); |
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return eccentric_to_true_anomaly(E, eccentricity); |
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} else { |
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double H = solve_kepler_hyperbolic(mean_anomaly, eccentricity); |
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return hyperbolic_to_true_anomaly(H, eccentricity); |
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} |
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} |
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// TODO: refactor for readability |
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OrbitalElements cartesian_to_orbital_elements(Vec3 position, Vec3 velocity, double parent_mass) { |
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double mu = G * parent_mass; |
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Vec3 h_vec = vec3_cross(position, velocity); |
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Vec3 r_vec = position; |
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Vec3 v_vec = velocity; |
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double r = vec3_magnitude(r_vec); |
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double v = vec3_magnitude(v_vec); |
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double v_squared = v * v; |
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double specific_energy = -mu / r + v_squared / 2.0; |
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double h = vec3_magnitude(h_vec); |
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double e_vec_x = ((v_squared - mu / r) * r_vec.x - (vec3_dot(r_vec, v_vec)) * v_vec.x) / mu; |
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double e_vec_y = ((v_squared - mu / r) * r_vec.y - (vec3_dot(r_vec, v_vec)) * v_vec.y) / mu; |
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double e_vec_z = ((v_squared - mu / r) * r_vec.z - (vec3_dot(r_vec, v_vec)) * v_vec.z) / mu; |
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Vec3 e_vec = {e_vec_x, e_vec_y, e_vec_z}; |
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double e = vec3_magnitude(e_vec); |
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double a; |
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if (fabs(specific_energy) < 1e-10) { |
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a = 1e10; |
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} else { |
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a = -mu / (2.0 * specific_energy); |
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} |
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double r_mag = vec3_magnitude(r_vec); |
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double r_dot_e = vec3_dot(r_vec, e_vec); |
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double true_anomaly; |
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if (e < 1e-10) { |
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true_anomaly = 0.0; |
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} else { |
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double cos_nu = r_dot_e / (r_mag * e * mu); |
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cos_nu = fmax(-1.0, fmin(1.0, cos_nu)); |
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true_anomaly = acos(cos_nu); |
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if (vec3_dot(r_vec, v_vec) < 0.0) { |
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true_anomaly = 2.0 * M_PI - true_anomaly; |
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} |
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// Normalize to (-π, π] range |
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if (true_anomaly > M_PI) { |
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true_anomaly -= 2.0 * M_PI; |
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} |
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} |
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double i; |
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double h_z = h_vec.z; |
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if (h > 1e-10) { |
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i = acos(h_z / h); |
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} else { |
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i = 0.0; |
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} |
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Vec3 n_vec = {0.0, 0.0, 1.0}; |
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Vec3 n = vec3_cross(n_vec, h_vec); |
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double n_mag = vec3_magnitude(n); |
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double Omega; |
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if (n_mag > 1e-10) { |
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Omega = acos(n.x / n_mag); |
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if (n.y < 0.0) { |
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Omega = 2.0 * M_PI - Omega; |
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} |
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} else { |
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Omega = 0.0; |
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} |
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double e_dot_n = vec3_dot(e_vec, n) / (mu * n_mag); |
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double omega; |
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if (e > 1e-10 && n_mag > 1e-10) { |
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omega = acos(e_dot_n / e); |
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if (e_vec.z < 0.0) { |
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omega = 2.0 * M_PI - omega; |
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} |
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} else { |
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omega = 0.0; |
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} |
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OrbitalElements elements; |
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if (fabs(e - 1.0) < 1e-3) { |
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elements.semi_latus_rectum = (h * h) / mu; |
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} else { |
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elements.semi_major_axis = a; |
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} |
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elements.eccentricity = e; |
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elements.true_anomaly = true_anomaly; |
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elements.inclination = i; |
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elements.longitude_of_ascending_node = Omega; |
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elements.argument_of_periapsis = omega; |
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return elements; |
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} |
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OrbitalElements propagate_orbital_elements(const OrbitalElements& elements, double dt, double parent_mass) { |
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double a = elements.semi_major_axis; |
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double e = elements.eccentricity; |
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double nu = elements.true_anomaly; |
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double mu = G * parent_mass; |
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double n = sqrt(mu / pow(fabs(a), 3.0)); |
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double E = 2.0 * atan(sqrt((1.0 - e) / (1.0 + e)) * tan(nu / 2.0)); |
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double M = E - e * sin(E); |
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M = M + n * dt; |
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double E_new = get_initial_trial_value(M, e); |
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const double CONVERGENCE_TOLERANCE = 1.0e-10; |
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const int MAX_ITERATIONS = 50; |
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int iterations = 0; |
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double E_prev = E_new + 2.0 * CONVERGENCE_TOLERANCE; |
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while (fabs(E_new - E_prev) > CONVERGENCE_TOLERANCE && iterations < MAX_ITERATIONS) { |
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E_prev = E_new; |
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double sin_E = sin(E_new); |
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E_new = E_new - (E_new - e * sin_E - M) / (1.0 - e * cos(E_new)); |
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iterations++; |
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} |
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OrbitalElements result = elements; |
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result.true_anomaly = 2.0 * atan(sqrt((1.0 + e) / (1.0 - e)) * tan(E_new / 2.0)); |
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return result; |
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}
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