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348 lines
12 KiB
Python
348 lines
12 KiB
Python
"""
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In physics and astronomy, a gravitational N-body simulation is a simulation of a
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dynamical system of particles under the influence of gravity. The system
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consists of a number of bodies, each of which exerts a gravitational force on all
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other bodies. These forces are calculated using Newton's law of universal
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gravitation. The Euler method is used at each time-step to calculate the change in
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velocity and position brought about by these forces. Softening is used to prevent
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numerical divergences when a particle comes too close to another (and the force
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goes to infinity).
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(Description adapted from https://en.wikipedia.org/wiki/N-body_simulation )
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(See also http://www.shodor.org/refdesk/Resources/Algorithms/EulersMethod/ )
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"""
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from __future__ import annotations
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import random
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from matplotlib import animation
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from matplotlib import pyplot as plt
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# Frame rate of the animation
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INTERVAL = 20
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# Time between time steps in seconds
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DELTA_TIME = INTERVAL / 1000
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class Body:
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def __init__(
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self,
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position_x: float,
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position_y: float,
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velocity_x: float,
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velocity_y: float,
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mass: float = 1.0,
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size: float = 1.0,
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color: str = "blue",
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) -> None:
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"""
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The parameters "size" & "color" are not relevant for the simulation itself,
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they are only used for plotting.
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"""
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self.position_x = position_x
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self.position_y = position_y
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self.velocity_x = velocity_x
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self.velocity_y = velocity_y
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self.mass = mass
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self.size = size
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self.color = color
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@property
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def position(self) -> tuple[float, float]:
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return self.position_x, self.position_y
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@property
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def velocity(self) -> tuple[float, float]:
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return self.velocity_x, self.velocity_y
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def update_velocity(
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self, force_x: float, force_y: float, delta_time: float
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) -> None:
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"""
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Euler algorithm for velocity
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>>> body_1 = Body(0.,0.,0.,0.)
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>>> body_1.update_velocity(1.,0.,1.)
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>>> body_1.velocity
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(1.0, 0.0)
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>>> body_1.update_velocity(1.,0.,1.)
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>>> body_1.velocity
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(2.0, 0.0)
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>>> body_2 = Body(0.,0.,5.,0.)
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>>> body_2.update_velocity(0.,-10.,10.)
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>>> body_2.velocity
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(5.0, -100.0)
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>>> body_2.update_velocity(0.,-10.,10.)
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>>> body_2.velocity
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(5.0, -200.0)
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"""
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self.velocity_x += force_x * delta_time
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self.velocity_y += force_y * delta_time
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def update_position(self, delta_time: float) -> None:
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"""
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Euler algorithm for position
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>>> body_1 = Body(0.,0.,1.,0.)
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>>> body_1.update_position(1.)
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>>> body_1.position
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(1.0, 0.0)
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>>> body_1.update_position(1.)
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>>> body_1.position
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(2.0, 0.0)
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>>> body_2 = Body(10.,10.,0.,-2.)
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>>> body_2.update_position(1.)
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>>> body_2.position
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(10.0, 8.0)
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>>> body_2.update_position(1.)
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>>> body_2.position
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(10.0, 6.0)
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"""
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self.position_x += self.velocity_x * delta_time
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self.position_y += self.velocity_y * delta_time
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class BodySystem:
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"""
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This class is used to hold the bodies, the gravitation constant, the time
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factor and the softening factor. The time factor is used to control the speed
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of the simulation. The softening factor is used for softening, a numerical
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trick for N-body simulations to prevent numerical divergences when two bodies
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get too close to each other.
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"""
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def __init__(
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self,
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bodies: list[Body],
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gravitation_constant: float = 1.0,
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time_factor: float = 1.0,
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softening_factor: float = 0.0,
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) -> None:
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self.bodies = bodies
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self.gravitation_constant = gravitation_constant
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self.time_factor = time_factor
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self.softening_factor = softening_factor
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def __len__(self) -> int:
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return len(self.bodies)
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def update_system(self, delta_time: float) -> None:
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"""
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For each body, loop through all other bodies to calculate the total
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force they exert on it. Use that force to update the body's velocity.
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>>> body_system_1 = BodySystem([Body(0,0,0,0), Body(10,0,0,0)])
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>>> len(body_system_1)
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2
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>>> body_system_1.update_system(1)
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>>> body_system_1.bodies[0].position
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(0.01, 0.0)
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>>> body_system_1.bodies[0].velocity
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(0.01, 0.0)
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>>> body_system_2 = BodySystem([Body(-10,0,0,0), Body(10,0,0,0, mass=4)], 1, 10)
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>>> body_system_2.update_system(1)
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>>> body_system_2.bodies[0].position
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(-9.0, 0.0)
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>>> body_system_2.bodies[0].velocity
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(0.1, 0.0)
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"""
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for body1 in self.bodies:
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force_x = 0.0
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force_y = 0.0
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for body2 in self.bodies:
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if body1 != body2:
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dif_x = body2.position_x - body1.position_x
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dif_y = body2.position_y - body1.position_y
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# Calculation of the distance using Pythagoras's theorem
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# Extra factor due to the softening technique
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distance = (dif_x**2 + dif_y**2 + self.softening_factor) ** (1 / 2)
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# Newton's law of universal gravitation.
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force_x += (
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self.gravitation_constant * body2.mass * dif_x / distance**3
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)
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force_y += (
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self.gravitation_constant * body2.mass * dif_y / distance**3
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)
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# Update the body's velocity once all the force components have been added
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body1.update_velocity(force_x, force_y, delta_time * self.time_factor)
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# Update the positions only after all the velocities have been updated
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for body in self.bodies:
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body.update_position(delta_time * self.time_factor)
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def update_step(
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body_system: BodySystem, delta_time: float, patches: list[plt.Circle]
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) -> None:
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"""
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Updates the body-system and applies the change to the patch-list used for plotting
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>>> body_system_1 = BodySystem([Body(0,0,0,0), Body(10,0,0,0)])
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>>> patches_1 = [plt.Circle((body.position_x, body.position_y), body.size,
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... fc=body.color)for body in body_system_1.bodies] #doctest: +ELLIPSIS
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>>> update_step(body_system_1, 1, patches_1)
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>>> patches_1[0].center
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(0.01, 0.0)
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>>> body_system_2 = BodySystem([Body(-10,0,0,0), Body(10,0,0,0, mass=4)], 1, 10)
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>>> patches_2 = [plt.Circle((body.position_x, body.position_y), body.size,
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... fc=body.color)for body in body_system_2.bodies] #doctest: +ELLIPSIS
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>>> update_step(body_system_2, 1, patches_2)
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>>> patches_2[0].center
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(-9.0, 0.0)
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"""
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# Update the positions of the bodies
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body_system.update_system(delta_time)
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# Update the positions of the patches
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for patch, body in zip(patches, body_system.bodies):
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patch.center = (body.position_x, body.position_y)
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def plot(
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title: str,
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body_system: BodySystem,
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x_start: float = -1,
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x_end: float = 1,
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y_start: float = -1,
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y_end: float = 1,
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) -> None:
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"""
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Utility function to plot how the given body-system evolves over time.
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No doctest provided since this function does not have a return value.
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"""
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fig = plt.figure()
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fig.canvas.manager.set_window_title(title)
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ax = plt.axes(
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xlim=(x_start, x_end), ylim=(y_start, y_end)
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) # Set section to be plotted
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plt.gca().set_aspect("equal") # Fix aspect ratio
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# Each body is drawn as a patch by the plt-function
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patches = [
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plt.Circle((body.position_x, body.position_y), body.size, fc=body.color)
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for body in body_system.bodies
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]
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for patch in patches:
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ax.add_patch(patch)
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# Function called at each step of the animation
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def update(frame: int) -> list[plt.Circle]: # noqa: ARG001
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update_step(body_system, DELTA_TIME, patches)
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return patches
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anim = animation.FuncAnimation( # noqa: F841
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fig, update, interval=INTERVAL, blit=True
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)
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plt.show()
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def example_1() -> BodySystem:
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"""
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Example 1: figure-8 solution to the 3-body-problem
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This example can be seen as a test of the implementation: given the right
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initial conditions, the bodies should move in a figure-8.
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(initial conditions taken from http://www.artcompsci.org/vol_1/v1_web/node56.html)
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>>> body_system = example_1()
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>>> len(body_system)
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3
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"""
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position_x = 0.9700436
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position_y = -0.24308753
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velocity_x = 0.466203685
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velocity_y = 0.43236573
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bodies1 = [
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Body(position_x, position_y, velocity_x, velocity_y, size=0.2, color="red"),
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Body(-position_x, -position_y, velocity_x, velocity_y, size=0.2, color="green"),
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Body(0, 0, -2 * velocity_x, -2 * velocity_y, size=0.2, color="blue"),
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]
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return BodySystem(bodies1, time_factor=3)
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def example_2() -> BodySystem:
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"""
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Example 2: Moon's orbit around the earth
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This example can be seen as a test of the implementation: given the right
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initial conditions, the moon should orbit around the earth as it actually does.
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(mass, velocity and distance taken from https://en.wikipedia.org/wiki/Earth
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and https://en.wikipedia.org/wiki/Moon)
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No doctest provided since this function does not have a return value.
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"""
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moon_mass = 7.3476e22
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earth_mass = 5.972e24
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velocity_dif = 1022
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earth_moon_distance = 384399000
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gravitation_constant = 6.674e-11
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# Calculation of the respective velocities so that total impulse is zero,
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# i.e. the two bodies together don't move
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moon_velocity = earth_mass * velocity_dif / (earth_mass + moon_mass)
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earth_velocity = moon_velocity - velocity_dif
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moon = Body(-earth_moon_distance, 0, 0, moon_velocity, moon_mass, 10000000, "grey")
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earth = Body(0, 0, 0, earth_velocity, earth_mass, 50000000, "blue")
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return BodySystem([earth, moon], gravitation_constant, time_factor=1000000)
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def example_3() -> BodySystem:
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"""
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Example 3: Random system with many bodies.
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No doctest provided since this function does not have a return value.
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"""
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bodies = []
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for _ in range(10):
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velocity_x = random.uniform(-0.5, 0.5)
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velocity_y = random.uniform(-0.5, 0.5)
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# Bodies are created pairwise with opposite velocities so that the
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# total impulse remains zero
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bodies.append(
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Body(
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random.uniform(-0.5, 0.5),
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random.uniform(-0.5, 0.5),
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velocity_x,
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velocity_y,
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size=0.05,
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)
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)
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bodies.append(
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Body(
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random.uniform(-0.5, 0.5),
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random.uniform(-0.5, 0.5),
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-velocity_x,
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-velocity_y,
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size=0.05,
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)
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)
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return BodySystem(bodies, 0.01, 10, 0.1)
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if __name__ == "__main__":
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plot("Figure-8 solution to the 3-body-problem", example_1(), -2, 2, -2, 2)
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plot(
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"Moon's orbit around the earth",
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example_2(),
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-430000000,
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430000000,
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-430000000,
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430000000,
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)
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plot("Random system with many bodies", example_3(), -1.5, 1.5, -1.5, 1.5)
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