Browse Source

Add functions for solving Kepler's equation, add solar system class

master
C. J. Howard 4 years ago
parent
commit
e777f5c63c
8 changed files with 294 additions and 18 deletions
  1. +1
    -0
      CMakeLists.txt
  2. +69
    -1
      src/game/astronomy/celestial-mechanics.cpp
  3. +9
    -13
      src/game/astronomy/celestial-mechanics.hpp
  4. +51
    -0
      src/game/components/orbit-component.hpp
  5. +1
    -1
      src/game/states/play-state.cpp
  6. +101
    -0
      src/game/systems/solar-system.cpp
  7. +54
    -0
      src/game/systems/solar-system.hpp
  8. +8
    -3
      src/game/systems/weather-system.cpp

+ 1
- 0
CMakeLists.txt View File

@ -4,6 +4,7 @@ option(VERSION_STRING "Project version string" "0.0.0")
project(antkeeper VERSION ${VERSION_STRING} LANGUAGES CXX)
# Find dependency packages
find_package(dr_wav REQUIRED CONFIG)
find_package(stb REQUIRED CONFIG)

+ 69
- 1
src/game/astronomy/celestial-mechanics.cpp View File

@ -70,7 +70,7 @@ double3 approx_moon_ecliptic(double jd)
+ 0.0007 * std::sin(m1 - m)
- 0.0006 * std::sin(d)
- 0.0005 * std::sin(m + m1);
const double latitude = 0.0895 * sin(f)
+ 0.0049 * std::sin(m1 + f)
+ 0.0048 * std::sin(m1 - f)
@ -129,4 +129,72 @@ double3x3 approx_moon_ecliptic_rotation(double jd)
return rz0 * rx * rz1;
}
double3 solve_kepler(const kepler_orbit& orbit, double t)
{
// Orbital period (Kepler's third law)
double pr = std::sqrt(orbit.a * orbit.a * orbit.a);
// Mean anomaly
double epoch = 0.0;
double ma = (math::two_pi<double> * (t - epoch)) / pr;
// Semi-minor axis
const double b = std::sqrt(1.0 - orbit.ec * orbit.ec);
// Trig of orbital elements (can be precalculated?)
const double cos_ma = std::cos(ma);
const double sin_ma = std::sin(ma);
const double cos_om = std::cos(orbit.om);
const double sin_om = std::sin(orbit.om);
const double cos_i = std::cos(orbit.i);
const double sin_i = std::sin(orbit.i);
// Eccentric anomaly
double ea = ma + orbit.ec * sin_ma * (1.0 + orbit.ec * cos_ma);
// Find radial distance (r) and true anomaly (v)
double x = orbit.a * (std::cos(ea) - orbit.ec);
double y = b * std::sin(ea);
double r = std::sqrt(x * x + y * y);
double v = std::atan2(y, x);
// Convert (r, v) to ecliptic rectangular coordinates
double cos_wv = std::cos(orbit.w + v);
double sin_wv = std::sin(orbit.w + v);
return double3
{
r * (cos_om * cos_wv - sin_om * sin_wv * cos_i),
r * (sin_om * cos_wv + cos_om * sin_wv * cos_i),
r * sin_wv * sin_i
};
}
double3 solve_kepler(double a, double ec, double w, double ma, double i, double om)
{
// Semi-minor axis
double b = std::sqrt(1.0 - ec * ec);
// Eccentric anomaly
double ea = ma + ec * std::sin(ma) * (1.0 + ec * std::cos(ma));
// Find radial distance (r) and true anomaly (v)
double x = a * (std::cos(ea) - ec);
double y = b * std::sin(ea);
double r = std::sqrt(x * x + y * y);
double v = std::atan2(y, x);
// Convert (r, v) to ecliptic rectangular coordinates
double cos_om = std::cos(om);
double sin_om = std::sin(om);
double cos_i = std::cos(i);
double cos_wv = std::cos(w + v);
double sin_wv = std::sin(w + v);
return double3
{
r * (cos_om * cos_wv - sin_om * sin_wv * cos_i),
r * (sin_om * cos_wv + cos_om * sin_wv * cos_i),
r * sin_wv * std::sin(i)
};
}
} // namespace ast

+ 9
- 13
src/game/astronomy/celestial-mechanics.hpp View File

@ -57,23 +57,19 @@ double3 approx_moon_ecliptic(double jd);
*/
double3x3 approx_moon_ecliptic_rotation(double jd);
struct orbital_elements
struct kepler_orbit
{
double a; ///< Semi-major axis (km)
double e; ///< Eccentricity
double w; ///< Argument of periapsis (radians)
double m; ///< Mean anomaly (radians)
double i; ///< Inclination to the ecliptic (radians)
double n; ///< Longitude of the ascending node (radians)
double a; ///< Semi-major axis, a
double ec; ///< Eccentricity, e
double w; ///< Argument of periapsis, w (radians)
double ma; ///< Mean anomaly, M (radians)
double i; ///< Inclination, i (radians)
double om; ///< Longitude of the ascending node, OMEGA (radians)
};
//constexpr orbital_elements j2k_orbit_moon = {384400.0, 0.0554, 318.15, 135.275.16, 125.08};
double3 solve_kepler(const kepler_orbit& orbit, double t);
struct orbital_state
{
double3 r; ///< Cartesian position
double3 v; ///< Cartesian velocity
};
double3 solve_kepler(double a, double ec, double w, double ma, double i, double om);
} // namespace ast

+ 51
- 0
src/game/components/orbit-component.hpp View File

@ -0,0 +1,51 @@
/*
* Copyright (C) 2020 Christopher J. Howard
*
* This file is part of Antkeeper source code.
*
* Antkeeper source code is free software: you can redistribute it and/or modify
* it under the terms of the GNU General Public License as published by
* the Free Software Foundation, either version 3 of the License, or
* (at your option) any later version.
*
* Antkeeper source code is distributed in the hope that it will be useful,
* but WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
* GNU General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with Antkeeper source code. If not, see <http://www.gnu.org/licenses/>.
*/
#ifndef ANTKEEPER_ECS_ORBIT_COMPONENT_HPP
#define ANTKEEPER_ECS_ORBIT_COMPONENT_HPP
#include "game/astronomy/celestial-mechanics.hpp"
namespace ecs {
struct orbit_component
{
double a; ///< Semi-major axis, a
double d_a;
double ec; ///< Eccentricity, e
double d_ec;
double w; ///< Argument of periapsis, w (radians)
double d_w;
double ma; ///< Mean anomaly, M (radians)
double d_ma;
double i; ///< Inclination, i (radians)
double d_i;
double om; ///< Longitude of the ascending node, OMEGA (radians)
double d_om;
};
} // namespace ecs
#endif // ANTKEEPER_ECS_ORBIT_COMPONENT_HPP

+ 1
- 1
src/game/states/play-state.cpp View File

@ -81,7 +81,7 @@ void play_state_enter(game_context* ctx)
sky_pass->set_moon_model(ctx->resource_manager->load<model>("moon.mdl"));
ctx->weather_system->set_location(ctx->biome->location[0], ctx->biome->location[1], ctx->biome->location[2]);
ctx->weather_system->set_time(2017, 8, 21, 5, 0, 0.0, -7.0);
ctx->weather_system->set_time(2017, 6, 1, 5, 0, 0.0, -7.0);
ctx->weather_system->set_sky_palette(ctx->biome->sky_palette);
ctx->weather_system->set_sun_palette(ctx->biome->sun_palette);
ctx->weather_system->set_ambient_palette(ctx->biome->ambient_palette);

+ 101
- 0
src/game/systems/solar-system.cpp View File

@ -0,0 +1,101 @@
/*
* Copyright (C) 2020 Christopher J. Howard
*
* This file is part of Antkeeper source code.
*
* Antkeeper source code is free software: you can redistribute it and/or modify
* it under the terms of the GNU General Public License as published by
* the Free Software Foundation, either version 3 of the License, or
* (at your option) any later version.
*
* Antkeeper source code is distributed in the hope that it will be useful,
* but WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
* GNU General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with Antkeeper source code. If not, see <http://www.gnu.org/licenses/>.
*/
#include "game/systems/solar-system.hpp"
#include "game/astronomy/celestial-coordinates.hpp"
#include "game/astronomy/celestial-mechanics.hpp"
#include "game/astronomy/celestial-time.hpp"
#include "game/components/orbit-component.hpp"
#include "game/components/transform-component.hpp"
using namespace ecs;
static constexpr double seconds_per_day = 24.0 * 60.0 * 60.0;
solar_system::solar_system(entt::registry& registry):
entity_system(registry),
julian_date(0.0),
time_scale(1.0),
latitude(0.0),
longitude(0.0),
altitude(0.0)
{}
void solar_system::update(double t, double dt)
{
// Add scaled timestep to Julian date
set_julian_date(julian_date + (dt * time_scale) / seconds_per_day);
// Update horizontal (topocentric) positions of orbiting bodies
registry.view<orbit_component, transform_component>().each(
[&](auto entity, auto& orbit, auto& transform)
{
double a = orbit.a;
double ec = orbit.ec;
double w = orbit.w;
double ma = orbit.ma;
double i = orbit.i;
double om = orbit.om;
double3 ecliptic = ast::solve_kepler(a, ec, w, ma, i, om);
double3 horizontal = ecliptic_to_horizontal * ecliptic;
// Subtract Earth's radius (in AU), for positon of observer
horizontal.z -= 4.25875e-5;
// Transform into local right-handed coordinates
double3 translation = ast::horizontal_to_right_handed * horizontal;
double3x3 rotation = ast::horizontal_to_right_handed * ecliptic_to_horizontal;
transform.local.translation = math::type_cast<float>(translation);
transform.local.rotation = math::type_cast<float>(math::quaternion_cast(rotation));
});
}
void solar_system::set_julian_date(double jd)
{
julian_date = jd;
// Recalculate obliquity of the ecliptic
ecl = ast::approx_ecliptic_obliquity(julian_date);
// Recalculate LMST
lmst = ast::jd_to_lmst(julian_date, longitude);
// Recalculate ecliptic to horizontal transformation matrix
ecliptic_to_horizontal = ast::ecliptic_to_horizontal(ecl, latitude, lmst);
}
void solar_system::set_time_scale(double scale)
{
time_scale = scale;
}
void solar_system::set_observer_location(double latitude, double longitude, double altitude)
{
this->latitude = latitude;
this->longitude = longitude;
this->altitude = altitude;
// Recalculate LMST
lmst = ast::jd_to_lmst(julian_date, longitude);
// Recalculate ecliptic to horizontal transformation matrix
ecliptic_to_horizontal = ast::ecliptic_to_horizontal(ecl, latitude, lmst);
}

+ 54
- 0
src/game/systems/solar-system.hpp View File

@ -0,0 +1,54 @@
/*
* Copyright (C) 2020 Christopher J. Howard
*
* This file is part of Antkeeper source code.
*
* Antkeeper source code is free software: you can redistribute it and/or modify
* it under the terms of the GNU General Public License as published by
* the Free Software Foundation, either version 3 of the License, or
* (at your option) any later version.
*
* Antkeeper source code is distributed in the hope that it will be useful,
* but WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
* GNU General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with Antkeeper source code. If not, see <http://www.gnu.org/licenses/>.
*/
#ifndef ANTKEEPER_SOLAR_SYSTEM_HPP
#define ANTKEEPER_SOLAR_SYSTEM_HPP
#include "entity-system.hpp"
#include "utility/fundamental-types.hpp"
class solar_system:
public entity_system
{
public:
solar_system(entt::registry& registry);
virtual void update(double t, double dt);
void set_julian_date(double jd);
void set_time_scale(double scale);
void set_observer_location(double latitude, double longitude, double altitude);
private:
double julian_date;
double time_scale;
double latitude;
double longitude;
double altitude;
double lmst;
double ecl;
double3x3 ecliptic_to_horizontal;
double3 sun_position;
};
#endif // ANTKEEPER_SOLAR_SYSTEM_HPP

+ 8
- 3
src/game/systems/weather-system.cpp View File

@ -83,11 +83,16 @@ void weather_system::update(double t, double dt)
double3 moon_ecliptic = ast::approx_moon_ecliptic(jd);
double3 moon_horizontal = ecliptic_to_horizontal * moon_ecliptic;
moon_horizontal.z -= 1.0; // Subtract one earth radius, for position of observer
double3 moon_spherical = ast::rectangular_to_spherical(moon_horizontal);
double3 moon_positiond = ast::horizontal_to_right_handed * moon_horizontal;
float2 moon_az_el = {static_cast<float>(moon_spherical.z) - math::pi<float>, static_cast<float>(moon_spherical.y)};
float3 moon_position = math::normalize(float3{static_cast<float>(moon_positiond.x), static_cast<float>(moon_positiond.y), static_cast<float>(moon_positiond.z)});
float2 moon_az_el = {static_cast<float>(moon_spherical.z) - math::pi<float>, static_cast<float>(moon_spherical.y)};
float3 moon_position = math::normalize(math::type_cast<float>(moon_positiond));
//double3 moon_sphericald = ast::rectangular_to_spherical(moon_positiond);
//std::cout << "old azel: " << math::degrees(moon_az_el.x) << ", " << math::degrees(moon_az_el.y) << std::endl;
//std::cout << "new azel: " << math::degrees(moon_sphericald.z) << ", " << math::degrees(moon_sphericald.y) << std::endl;
double3x3 moon_rotation_matrix = ast::horizontal_to_right_handed * ecliptic_to_horizontal;
math::quaternion<double> moon_rotationd = math::normalize(math::quaternion_cast(moon_rotation_matrix) * math::angle_axis(math::half_pi<double>, double3{0, 1, 0}) * math::angle_axis(-math::half_pi<double>, double3{0, 0, -1}));
math::quaternion<float> moon_rotation =

Loading…
Cancel
Save