API documentation (Python)¶
An Nbody integrator package for python.

class
rebound.
SimulationArchive
(filename, setup=None, setup_args=(), rebxfilename=None)[source]¶ SimulationArchive Class.
The SimulationArchive is a binary file format which includes all settings, constants as well as particle positions and velocities. This makes it possible to reproduce a simulation exactly (down to the last bit). The SimulationArchive allows you to add an arbitrary number of snapshots. Simulations can be reconstructed from these snapshots. Since version 2 of the SimulationArchive (Spring 2018), you can change anything inbetween snapshots, icluding settings like the integrator, the timestep, the number of particles. The file format is efficient in that only data that changed is stored in the SimulationArchive file. This is all done automatically. All the user has to do is call the function to create a snapshot. The SimulationArchive thus allows for fast access to any long running simulations. For a full discussion of the functionality see the paper by Rein & Tamayo 2017.
Examples
Here is a simple example:
>>> sa = rebound.SimulationArchive("archive.bin") >>> sim = sa.getSimulation(t=1e6) >>> print(sim.particles[1]) >>> for sim in sa: >>> print(sim.t, sim.particles[1].e)
Methods

getSimulation
(t, mode='snapshot', keep_unsynchronized=1)[source]¶ This function returns a simulation object at (or close to) the requested time t. Everytime this function is called a new simulation object is created.
Returns: A rebound.Simulation object. Everytime the function gets called
a new object gets created.
Examples
Here is a simple example on how to load a simulation from a Simulation Archive file with the getSimulation method. As the mode argument is set to close, the simulation will be integrated from the nearest snapshot to the request time.
>>> sa = rebound.SimulationArchive("archive.bin") >>> sim = sa.getSimulation(t=1e6, mode="close") >>> print(sim.particles[1]) >>> for sim in sa: >>> print(sim.t, sim.particles[1].e)


class
rebound.
Simulation
[source]¶ REBOUND Simulation Object.
This object encapsulated an entire REBOUND simulation. It is an abstraction of the C struct reb_simulation. You can create mutiple REBOUND simulations (the c library is thread safe).
Examples
Most simulation parameters can be directly changed with the property syntax:
>>> sim = rebound.Simulation() >>> sim.G = 1. # Sets the graviational constant (default 1) >>> sim.softening = 1. # Sets the graviational softening parameter (default 0) >>> sim.testparticle_type = 1 # Allows massive particles to feel influence from testparticles (default 0) >>> sim.dt = 0.1 # Sets the timestep (will change for adaptive integrators such as IAS15). >>> sim.t = 0. # Sets the current simulation time (default 0) >>> print(sim.N) # Gets the current number of particles >>> print(sim.N_active) # Gets the current number of active particles
Attributes
Methods

N_real
¶ Get the current number of real (i.e. no variational/shadow) particles in the simulation.

add
(particle=None, **kwargs)[source]¶ Adds a particle to REBOUND. Accepts one of the following:
 A single Particle structure.
 The particle’s mass and a set of cartesian coordinates: m,x,y,z,vx,vy,vz.
 The primary as a Particle structure, the particle’s mass and a set of orbital elements: primary,m,a,anom,e,omega,inv,Omega,MEAN (see
Orbit
for the definition of orbital elements).  A name of an object (uses NASA Horizons to look up coordinates)
 A list of particles or names.

add_particles_ascii
(s)[source]¶ Adds particles from an ASCII string.
Parameters: s : string
One particle per line. Each line should include particle’s mass, radius, position and velocity.

add_variation
(order=1, first_order=None, first_order_2=None, testparticle=1)[source]¶ This function adds a set of variational particles to the simulation.
If there are N real particles in the simulation, this functions adds N additional variational particles. To see how many particles (real and variational) are in a simulation, use
'sim.N'
. To see how many variational particles are in a simulation use'sim.N_var'
.Currently Leapfrog, WHFast and IAS15 support first order variational equations. IAS15 also supports second order variational equations.
Parameters: order : integer, optional
By default the function adds a set of first order variational particles to the simulation. Set this flag to 2 for second order.
first_order : Variation, optional
Second order variational equations depend on their corresponding first order variational equations. This parameter expects the Variation object corresponding to the first order variational equations.
first_order_2 : Variation, optional
Same as first_order. But allows to set two different indicies to calculate offdiagonal elements. If omitted, then first_order will be used for both first order equations.
testparticle : int, optional
If set to a value >= 0, then only one variational particle will be added and be treated as a test particle.
Returns: Returns Variation object (a copy–you can only modify it through its particles property or vary method).

additional_forces
¶ Get or set a function pointer for calculating additional forces in the simulation.
The argument can be a python function or something that can be cast to a C function of type CFUNCTYPE(None,POINTER(Simulaton)). If the forces are velocity dependent, the flag force_is_velocity_dependent needs to be set to 1. Otherwise the particle structures might contain incorrect velocity values.

automateSimulationArchive
(filename, interval=None, walltime=None, deletefile=False)[source]¶ This function automates taking snapshots during a simulationusing the Simulation Archive. Instead of using this function, one can also call simulationarchive_snapshot() manually to create snapshots.
Examples
The following example creates a simulation, then initializes the Simulation Archive and integrates it forward in time.
>>> sim = rebound.Simulation() >>> sim.add(m=1.) >>> sim.add(m=1.e3,x=1.,vy=1.) >>> sim.automateSimulationArchive("sa.bin",interval=1000.) >>> sim.integrate(1e8)
The SimulationArchive can later be read in using the following syntax:
>>> sa = rebound.SimulationArchive("sa.bin") >>> sim = sa[0] # get the first snapshot in the SA file (initial conditions) >>> sim = sa[1] # get the last snapshot in the SA file

boundary
¶ Get or set the boundary module.
Available boundary modules are:
'none'
(default)'open'
'periodic'
'shear'
Check the online documentation for a full description of each of the modules.

calculate_angular_momentum
()[source]¶ Returns a list of the three (x,y,z) components of the total angular momentum of all particles in the simulation.

calculate_com
(first=0, last=None)[source]¶ Returns the center of momentum for all particles in the simulation.
Parameters: first: int, optional
If
first
is specified, only calculate the center of momentum starting from index=``first``.last : int or None, optional
If
last
is specified only calculate the center of momentum up to (but excluding) index=``last``. Same behavior as Python’s range function.Examples
>>> sim = rebound.Simulation() >>> sim.add(m=1, x=20) >>> sim.add(m=1, x=10) >>> sim.add(m=1, x=0) >>> sim.add(m=1, x=10) >>> sim.add(m=1, x=20) >>> com = sim.calculate_com() >>> com.x 0.0 >>> com = sim.calculate_com(first=2,last=4) # Considers indices 2,3 >>> com.x 5.0

calculate_energy
()[source]¶ Returns the sum of potential and kinetic energy of all particles in the simulation.

calculate_lyapunov
()[source]¶ Return the current Lyapunov Characteristic Number (LCN). Note that you need to call init_megno() before the start of the simulation. To get a timescale (the Lyapunov timescale), take the inverse of this quantity.

calculate_megno
()[source]¶ Return the current MEGNO value. Note that you need to call init_megno() before the start of the simulation.

calculate_orbits
(primary=None, jacobi_masses=False, heliocentric=None, barycentric=None)[source]¶ Calculate orbital parameters for all partices in the simulation. By default this functions returns the orbits in Jacobi coordinates.
If MEGNO is enabled, variational particles will be ignored.
Parameters: primary : rebound.Particle, optional
Set the primary against which to reference the osculating orbit. Default(use Jacobi center of mass)
jacobi_masses: bool
Whether to use jacobi primary mass in orbit calculation. (Default: False)
heliocentric: bool, DEPRECATED
To calculate heliocentric elements, pass primary=sim.particles[0]
barycentric : bool, DEPRECATED
To calculate barycentric elements, pass primary=sim.calculate_com()
Returns: Returns an array of Orbits of length N1.

coefficient_of_restitution
¶ Get or set a function pointer that defined the coefficient of restitution.

collision
¶ Get or set the collision module.
Available collision modules are:
'none'
(default)'direct'
'tree'
'mercurius'
'direct'
Check the online documentation for a full description of each of the modules.

collision_resolve
¶ Get or set a function pointer for collision resolving routine.
 Possible options for setting:
 Function pointer
 “merge”: two colliding particles will merge)
 “hardsphere”: two colliding particles will bounce of using a set coefficient of restitution

configure_box
(boxsize, root_nx=1, root_ny=1, root_nz=1)[source]¶ Initialize the simulation box.
This function only needs to be called it boundary conditions other than “none” are used. In such a case the boxsize must be known and is set with this function.
Parameters: boxsize : float, optional
The size of one root box.
root_nx, root_ny, root_nz : int, optional
The number of root boxes in each direction. The total size of the simulation box will be
root_nx * boxsize
,root_ny * boxsize
androot_nz * boxsize
. By default there will be exactly one root box in each direction.

configure_ghostboxes
(nghostx=0, nghosty=0, nghostz=0)[source]¶ Initialize the ghost boxes.
This function only needs to be called it boundary conditions other than “none” or “open” are used. In such a case the number of ghostboxes must be known and is set with this function.
Parameters: nghostx, nghosty, nghostz : int
The number of ghost boxes in each direction. All values default to 0 (no ghost boxes).

convert_particle_units
(*args)[source]¶ Will convert the units for the simulation (i.e. convert G) as well as the particles’ cartesian elements. Must have set sim.units ahead of calling this function so REBOUND knows what units to convert from.
Parameters: 3 strings corresponding to units of time, length and mass. Can be in any order and aren’t case sensitive. You can add new units to rebound/rebound/units.py

free_particle_ap
¶ Get or set a function pointer for freeing the ap pointer whenever sim.remove is called.

classmethod
from_archive
(filename, snapshot=1)[source]¶ Loads a REBOUND simulation from a SimulationArchive binary file. It uses the last snapshot in that file unless otherwise specified. This function is only really useful for restarting a simulation. For full access to the Simulation Archive, use the SimulationArchive class.
After loading the REBOUND simulation from file, you need to reset any function pointers manually. Please read all documentation before using this function as it has several requirements to work correctly.
Returns: A rebound.Simulation object.

classmethod
from_file
(filename)[source]¶ Loads a REBOUND simulation from a file.
After loading the REBOUND simulation from file, you need to reset any function pointers manually.
Returns: A rebound.Simulation object. Examples
The following example creates a simulation, saves it to a file and then creates a copy of the simulation store in the binary file.
>>> sim = rebound.Simulation() >>> sim.add(m=1.) >>> sim.add(m=1.e3,x=1.,vy=1.) >>> sim.save("simulation.bin") >>> sim_copy = rebound.Simulation.from_file("simulation.bin")

getWidget
(**kwargs)[source]¶ Wrapper function that returns a new widget attached to this simulation.
Widgets provide realtime 3D visualizations from within an Jupyter notebook. See the Widget class for more details on the possible arguments.
Returns: A rebound.Widget object. Examples
>>> sim = rebound.Simulation() >>> sim.add(m=1.) >>> sim.add(m=1.e3,x=1.,vy=1.) >>> sim.getWidget()

gravity
¶ Get or set the gravity module.
Available gravity modules are:
'none'
'basic'
(default)'compensated'
'tree'
Check the online documentation for a full description of each of the modules.

heartbeat
¶ Set a function pointer for a heartbeat function. The heartbeat function is called every timestep and can be used to monitor long simulations, check for stalled simulations and output debugging information.
The argument can be a python function or something that can be cast to a C function or a python function.
The function called will receive a pointer to the simulation object as its argument.
Examples
>>> import rebound >>> sim = rebound.Simulation() >>> sim.add(m=1.) >>> sim.add(m=1e3, a=1) >>> def heartbeat(sim): >>> # sim is a pointer to the simulation object, >>> # thus use contents to access object data. >>> # See ctypes documentation for details. >>> print(sim.contents.t) >>> sim.heartbeat = heartbeat >>> sim.integrate(1.)

init_megno
()[source]¶ This function initialises the chaos indicator MEGNO particles and enables their integration.
MEGNO is short for Mean Exponential Growth of Nearby orbits. It can be used to test if a system is chaotic or not. In the backend, the integrator is integrating an additional set of particles using the variational equation. Note that variational equations are better suited for this than shadow particles. MEGNO is currently only supported in the IAS15 and WHFast integrators.
This function also needs to be called if you are interested in the Lyapunov exponent as it is calculate with the help of MEGNO. See Rein and Tamayo 2015 for details on the implementation.
For more information on MENGO see e.g. http://dx.doi.org/10.1051/00046361:20011189

integrate
(tmax, exact_finish_time=1)[source]¶ Main integration function. Call this function when you have setup your simulation and want to integrate it forward (or backward) in time. The function might be called many times to integrate the simulation in steps and create outputs inbetween steps.
Parameters: tmax : float
The final time of your simulation. If the current time is 100, and tmax=200, then after the calling the integrate routine, the time has advanced to t=200. If tmax is larger than or equal to the current time, no integration will be performed.
exact_finish_time: int, optional
This argument determines whether REBOUND should try to finish at the exact time (tmax) you give it or if it is allowed to overshoot. Overshooting could happen if one starts at t=0, has a timestep of dt=10 and wants to integrate to tmax=25. With
exact_finish_time=1
, the integrator will choose the last timestep such that t is exactly 25 after the integration, otherwise t=30. Note that changing the timestep does affect the accuracy of symplectic integrators negatively.Examples
The typical usage is as follows. Note the use of
np.linspace
to create equally spaced outputs. Usingnp.logspace
can be used to easily produce logarithmically spaced outputs.>>> import numpy as np >>> for time in np.linspace(0,100.,10): >>> sim.integrate(time) >>> perform_output(sim)

integrator
¶ Get or set the intergrator module.
Available integrators are:
'ias15'
(default)'whfast'
'sei'
'leapfrog'
'hermes'
'janus'
'mercurius'
'bs'
'none'
Check the online documentation for a full description of each of the integrators.

integrator_synchronize
()[source]¶ Call this function if safemode is disabled and you need synchronize particle positions and velocities between timesteps.

move_to_com
()[source]¶ This function moves all particles in the simulation to a center of momentum frame. In that frame, the center of mass is at the origin and does not move. It makes sense to call this function at the beginning of the integration, especially for the high accuray integrators IAS15 and WHFast.

particles
¶ Returns a Particles object that allows users to access particles like a dictionary using indices, hashes, or strings.
The Particles object uses pointers and thus the contents update as the simulation progresses. Note that the pointers could change, for example when a particle is added or removed from the simulation.

particles_ascii
(prec=8)[source]¶ Returns an ASCII string with all particles’ masses, radii, positions and velocities.
Parameters: prec : int, optional
Number of digits after decimal point. Default 8.

post_timestep_modifications
¶ Get or set a function pointer for posttimestep modifications.
The argument can be a python function or something that can be cast to a C function or a python function.

pre_timestep_modifications
¶ Get or set a function pointer for pretimestep modifications.
The argument can be a python function or something that can be cast to a C function or a python function.

refreshWidgets
()[source]¶ This function manually refreshed all widgets attached to this simulation.
You want to call this function if any particle data has been manually changed.

remove
(index=None, hash=None, keepSorted=True)[source]¶ Removes a particle from the simulation.
Parameters: index : int, optional
Specify particle to remove by index.
hash : c_uint32 or string, optional
Specifiy particle to remove by hash (if a string is passed, the corresponding hash is calculated).
keepSorted : bool, optional
By default, remove preserves the order of particles in the particles array. Might set it to zero in cases with many particles and many removals to speed things up.

serialize_particle_data
(**kwargs)[source]¶ Fast way to access serialized particle data via numpy arrays.
This function can directly set the values of numpy arrays to current particle data. This is significantly faster than accessing particle data via sim.particles as all the copying is done on the C side. No memory is allocated by this function. It expects correctly sized numpy arrays as arguments. The argument name indicates what kind of particle data is written to the array.
Possible argument names are “hash”, “m”, “r”, “xyz”, “vxvyvz”. The datatype for the “hash” array needs to be uint32. The other arrays expect a datatype of float64. The lengths of “hash”, “m”, “r” arrays need to be at least sim.N. The lengths of xyz and vxvyvz need to be at least 3*sim.N. Exceptions are raised otherwise.
Note that this routine is only intended for special use cases where speed is an issue. For normal use, it is recommended to access particle data via the sim.particles array. Be aware of potential issues that arrise by directly accesing the memory of numpy arrays (see numpy documentation for more details).
Examples
This sets an array to the xyz positions of all particles:
>>> import numpy as np >>> a = np.zeros((sim.N,3),dtype="float64") >>> sim.serialize_particle_data(xyz=a) >>> print(a)
To get all current radii of particles:
>>> a = np.zeros(sim.N,dtype="float64") >>> sim.serialize_particle_data(r=a) >>> print(a)
To get all current radii and hashes of particles:
>>> a = np.zeros(sim.N,dtype="float64") >>> b = np.zeros(sim.N,dtype="uint32") >>> sim.serialize_particle_data(r=a,hash=b) >>> print(a,b)

simulationarchive_filename
¶ Returns the current SimulationArchive filename in use. Do not set manually. Use sim.automateSimulationArchive() instead

simulationarchive_snapshot
(filename)[source]¶ Take a snapshot and save it to a SimulationArchive file. If the file does not exist yet, a new one will be created. If the file does exist, a snapshot will be appended.

step
()[source]¶ Perform exactly one integration step with REBOUND. This function is rarely needed. Instead, use integrate().

tree_update
()[source]¶ Call this function to update the tree structure manually after removing particles.

units
¶ Tuple of the units for length, time and mass. Can be set in any order, and strings are not casesensitive. See ipython_examples/Units.ipynb for more information. You can check the units’ exact values and add Additional units in rebound/rebound/units.py. Units should be set before adding particles to the simulation (will give error otherwise).
Examples
>>> sim = rebound.Simulation() >>> sim.units = ('yr', 'AU', 'Msun')


class
rebound.
Orbit
[source]¶ A class containing orbital parameters for a particle. This is an abstraction of the reb_orbit data structure in C.
When using the various REBOUND functions using Orbits, all angles are in radians. The following image illustrated the most important angles used. In REBOUND the reference direction is the positive x direction, the reference plane is the xy plane.
Image from wikipedia. CCBYSA3.
Attributes
d (float) radial distance from reference v (float) velocity relative to central object’s velocity h (float) specific angular momentum P (float) orbital period (negative if hyperbolic) n (float) mean motion (negative if hyperbolic) a (float) semimajor axis e (float) eccentricity inc (float) inclination Omega (float) longitude of ascending node omega (float) argument of pericenter pomega (float) longitude of pericenter f (float) true anomaly M (float) mean anomaly l (float) mean longitude = Omega + omega + M theta (float) true longitude = Omega + omega + f T (float) time of pericenter passage

rebound.
OrbitPlot
(sim, figsize=None, lim=None, limz=None, Narc=100, unitlabel=None, color=False, periastron=False, trails=True, show_orbit=True, lw=1.0, slices=False, plotparticles=[], primary=None)[source]¶ Convenience function for plotting instantaneous orbits.
Parameters: slices : bool, optional
Plot all three slices if set to True. Default is False and plots orbits only in the xy plane.
figsize : tuple of float, optional
Tuple defining the figure size (default: (5,5))
lim : float, optional
Limit for axes (default: None = automatically determined)
limz : float, optional
Limit for z axis, only used if slices=True (default: None = automatically determined)
unitlabel : str, optional
String describing the units, shown on axis labels (default: None)
color : bool, str or list, optional
By default plots in black. If set to True, plots using REBOUND color cycle. If a string or list of strings, e.g. [‘red’, ‘cyan’], will cycle between passed colors.
periastron : bool, optional
Draw a marker at periastron (default: False)
trails : bool, optional
Draw trails instead of solid lines (default: False)
show_orbit : bool, optional
Draw orbit trails/lines (default: True)
lw : float, optional
Linewidth (default: 1.)
plotparticles : list, optional
List of particles to plot. Can be a list of any valid keys for accessing sim.particles, i.e., integer indices or hashes (default: plot all particles)
primary : rebound.Particle, optional
Pimrary to use for the osculating orbit (default: Jacobi center of mass)
Returns: fig
A matplotlib figure
Examples
The following example illustrates a typical use case.
>>> sim = rebound.Simulation() >>> sim.add(m=1) >>> sim.add(a=1) >>> fig = rebound.OrbitPlot(sim) >>> fig.savefig("image.png") # save figure to file >>> fig.show() # show figure on screen

class
rebound.
Particle
(simulation=None, particle=None, m=None, x=None, y=None, z=None, vx=None, vy=None, vz=None, primary=None, a=None, P=None, e=None, inc=None, Omega=None, omega=None, pomega=None, f=None, M=None, l=None, theta=None, T=None, r=None, date=None, variation=None, variation2=None, h=None, k=None, ix=None, iy=None, hash=0, jacobi_masses=False)[source]¶ The main REBOUND particle data structure. This is an abstraction of the reb_particle structure in C. The Particle fields are set at the end of simulation.py to avoid circular references.
Attributes
x, y, z (float) Particle positions vx, vy, vz (float) Particle velocities ax, ay, az (float) Particle accelerations m (float) Particle mass r (float) Particle radius lastcollision (float) Last time the particle had a physical collision (if checking for collisions) c (c_void_p (C void pointer)) Pointer to the cell the particle is currently in (if using tree code) ap (c_void_p (C void pointer)) Pointer to additional parameters one might want to add to particles _sim (POINTER(rebound.Simulation)) Internal pointer to the parent simulation (used in C version of REBOUND) a, e, inc, Omega, omega, f (float) (Kepler Elements) Semimajor axis, eccentricity, inclination, longitude of the ascending node, argument of periapsis, and true anomaly respectively. The Keplerian Elements are in Jacobi coordinates (with mu = G*Minc, where Minc is the total mass from index 0 to the particle’s index, inclusive). Methods

__init__
(simulation=None, particle=None, m=None, x=None, y=None, z=None, vx=None, vy=None, vz=None, primary=None, a=None, P=None, e=None, inc=None, Omega=None, omega=None, pomega=None, f=None, M=None, l=None, theta=None, T=None, r=None, date=None, variation=None, variation2=None, h=None, k=None, ix=None, iy=None, hash=0, jacobi_masses=False)[source]¶ Initializes a Particle structure. Rather than explicitly creating a Particle structure, users may use the
add()
member function of a Simulation instance, which will both create a Particle and then add it to the simulation with one function call.This function accepts either cartesian positions and velocities, classical orbital elements together with the reference Particle (the primary), as well as orbital parameters defined by Pal (2009).
For convenience, optional keywords that are not passed default to zero (mass, cartesian and orbital elements).
Whenever initializing a particle from orbital elements, one must specify either the semimajor axis or the period of the orbit.
For classical orbital paramerers, one can specify the longitude of the ascending node by passing Omega, to specify the pericenter one can pass either omega or pomega (not both), and for the longitude/anomaly one can pass one of f, M, l or theta. See ipython_examples/OrbitalElements.ipynb for examples. See also Murray & Dermott Solar System Dynamics for formal definitions of angles in orbital mechanics.
All angles should be specified in radians.
Parameters: simulation : Simulation
Simulation instance associated with this particle (Required if passing orbital elements or setting up a variation).
particle : Particle, optional
If a particle is passed, a copy of that particle is returned. If a variational particle is initialized, then
particle
is original particle that will be varied.m : float
Mass (Default: 0)
x, y, z : float
Positions in Cartesian coordinates (Default: 0)
vx, vy, vz : float
Velocities in Cartesian coordinates (Default: 0)
primary : Particle
Primary body for converting orbital elements to cartesian (Default: center of mass of the particles in the passed simulation, i.e., this will yield Jacobi coordinates as one progressively adds particles)
a : float
Semimajor axis (a or P required if passing orbital elements)
P : float
Orbital period (a or P required if passing orbital elements)
e : float
Eccentricity (Default: 0)
inc : float
Inclination (Default: 0)
Omega : float
Longitude of ascending node (Default: 0)
omega : float
Argument of pericenter (Default: 0)
pomega : float
Longitude of pericenter (Default: 0)
f : float
True anomaly (Default: 0)
M : float
Mean anomaly (Default: 0)
l : float
Mean longitude (Default: 0)
theta : float
True longitude (Default: 0)
T : float
Time of pericenter passage
h : float
h variable, see Pal (2009) for a definition (Default: 0)
k : float
k variable, see Pal (2009) for a definition (Default: 0)
ix : float
ix variable, see Pal (2009) for a definition (Default: 0)
iy : float
iy variable, see Pal (2009) for a definition (Default: 0)
r : float
Particle radius (only used for collisional simulations)
date : string
For consistency with adding particles through horizons. Not used here.
variation : string (Default: None)
Set this string to the name of an orbital parameter to initialize the particle as a variational particle. Can be one of the following: m, a, e, inc, omega, Omega, f, k, h, lambda, ix, iy.
variation2 : string (Default: None)
Set this string to the name of a second orbital parameter to initialize the particle as a second order variational particle. Only used for second order variational equations. Can be one of the following: m, a, e, inc, omega, Omega, f, k, h, lambda, ix, iy.
hash : c_uint32
Unsigned integer identifier for particle. Can pass an integer directly, or a string that will be converted to a hash. User is responsible for assigning unique hashes.
jacobi_masses: bool
Whether to use jacobi primary mass in orbit initialization. Particle mass will still be set to physical value (Default: False)
Examples
——–
>>> sim = rebound.Simulation()
>>> sim.add(m=1.)
>>> p1 = rebound.Particle(simulation=sim, m=0.001, a=0.5, e=0.01)
>>> p2 = rebound.Particle(simulation=sim, m=0.0, x=1., vy=1.)
>>> p3 = rebound.Particle(simulation=sim, m=0.001, a=1.5, h=0.1, k=0.2, l=0.1)
>>> p4 = rebound.Particle(simulation=sim, m=0.001, a=1.5, omega=”uniform”) # omega will be a random number between 0 and 2pi

calculate_orbit
(primary=None, G=None)[source]¶ Returns a rebound.Orbit object with the keplerian orbital elements corresponding to the particle around the passed primary (rebound.Particle) If no primary is passed, defaults to Jacobi coordinates (with mu = G*Minc, where Minc is the total mass from index 0 to the particle’s index, inclusive).
Parameters: primary : rebound.Particle
Central body (Optional. Default uses Jacobi coordinates)
G : float
Gravitational constant (Optional. Default takes G from simulation in which particle is in)
Returns: A rebound.Orbit object
Examples
>>> sim = rebound.Simulation() >>> sim.add(m=1.) >>> sim.add(x=1.,vy=1.) >>> orbit = sim.particles[1].calculate_orbit(sim.particles[0]) >>> print(orbit.e) # gives the eccentricity

copy
()[source]¶ Returns a deep copy of the particle. The particle is not added to any simulation by default.

hash
¶ Get or set the particle’s hash. If set to a string, the corresponding integer hash is calculated.

sample_orbit
(Npts=100, primary=None, trailing=True, timespan=None, useTrueAnomaly=True)[source]¶ Returns a nested list of xyz positions along the osculating orbit of the particle. If primary is not passed, returns xyz positions along the Jacobi osculating orbit (with mu = G*Minc, where Minc is the total mass from index 0 to the particle’s index, inclusive).
Parameters: Npts : int, optional
Number of points along the orbit to return (default: 100)
primary : rebound.Particle, optional
Primary to use for the osculating orbit (default: Jacobi center of mass)
trailing: bool, optional
Whether to return points stepping backwards in time (True) or forwards (False). (default: True)
timespan: float, optional
Return points (for the osculating orbit) from the current position to timespan (forwards or backwards in time depending on trailing keyword). Defaults to the orbital period for bound orbits, and to the rough time it takes the orbit to move by the current distance from the primary for a hyperbolic orbit. Implementation currently only supports this option if useTrueAnomaly=False.
useTrueAnomaly: bool, optional
Will sample equally spaced points in true anomaly if True, otherwise in mean anomaly. Latter might be better for hyperbolic orbits, where true anomaly can stay near the limiting value for a long time, and then switch abruptly at pericenter. (Default: True)

vxyz
¶ Get or set the xyz velocity coordinates of the particle.

xyz
¶ Get or set the xyz position coordinates of the particle.


exception
rebound.
Encounter
[source]¶ The simulation exited because a close encounter has been detected. You may want to search for the pair of bodies which have the smallest distance.

exception
rebound.
Collision
[source]¶ The simulation exited because a collision has been detected. You may want to search for which particles have a lastcollision time equal to the simulation time.

exception
rebound.
Escape
[source]¶ The simulation exited because a particle has been se encounter has been detected. You may want to search for the particle with the largest distance from the origin and remove it from the simulation.

exception
rebound.
NoParticles
[source]¶ The simulation exited because no particles are left in the simulation.

class
rebound.
InterruptiblePool
(processes=None, initializer=None, initargs=(), **kwargs)[source]¶ A modified version of
multiprocessing.pool.Pool
that has better behavior with regard toKeyboardInterrupts
in themap()
method.Parameters:  processes – (optional) The number of worker processes to use; defaults to the number of CPUs.
 initializer – (optional)
Either
None
, or a callable that will be invoked by each worker process when it starts.  initargs – (optional)
Arguments for initializer; it will be called as
initializer(*initargs)
.  kwargs – (optional)
Extra arguments. Python 2.7 supports a
maxtasksperchild
parameter.
Methods

class
rebound.
Variation
[source]¶ REBOUND Variational Configuration Object.
This object encapsulated the configuration of one set of variational equations in a REBOUND simulation. It is an abstraction of the C struct reb_variational_configuration.
None of the fields in this struct should be changed after it has been initialized.
One rebound simulation can include any number of first and second order variational equations.
Note that variations are only encoded as particles for convenience. A variational particle’s position and velocity should be interpreted as a derivative, i.e. how much that position orvelocity varies with respect to the first or secondorder variation. See ipython_examples/VariationalEquations.ipynb and Rein and Tamayo (2016) for details.
Examples
>>> sim = rebound.Simulation() # Create a simulation >>> sim.add(m=1.) # Add a star >>> sim.add(m=1.e3, a=1.) # a planet >>> var_config = sim.add_variation() # Add a set of variational equations. >>> var_config.particles[1].x = 1. # Initialize the variational particle corresponding to the planet >>> sim.integrate(100.) # Integrate the simulation >>> print(var_config.particles[0].vx) # Print the velocity of the variational particle corresponding to the star
Attributes
Methods

particles
¶ Access the variational particles corresponding to this set of variational equations.
The function returns a list of particles which are sorted in the same way as those in sim.particles
The particles are pointers and thus can be modified.
If there are N real particles, this function will also return a list of N particles (all of which are variational particles).

vary
(particle_index, variation, variation2=None, primary=None)[source]¶ This function can be used to initialize the variational particles that are part of a Variation.
Note that rather than using this convenience function, one can also directly manipulate the particles’ coordinate using the following syntax:
>>> var = sim.add_variation() >>> var.particles[0].x = 1.
The
vary()
function is useful for initializing variations corresponding to changes in one of the orbital parameters for a particle on a bound Keplerian orbit.The function supports both first and second order variations in the following classical orbital parameters:
a, e, inc, omega, Omega, f as well as the Pal (2009) coordinates:
 a, h, k, ix, iy, lambda
and in both cases the mass m of the particle. The advantage of the Pal coordinate system is that all derivatives are well behaved (infinitely differentiable). Classical orbital parameters on the other hand exhibit coordinate singularities, for example when e=0.
The following example initializes the variational particles corresponding to a change in the semimajor axis of the particle with index 1:
>>> var = sim.add_variation() >>> var.vary(1,"a")
Parameters: particle_index : int
The index of the particle that should be varied. The index starts at 0 and runs through N1. The first particle added to a simulation receives the index 0, the second 1, and the on.
variation : string
This parameter determines which orbital parameter is varied.
variation2: string, optional
This is only used for second order variations which can depend on two varying parameters. If omitted, then it is assumed that the parameter variation is variation2.
primary: Particle, optional
By default variational particles are created in the Heliocentric frame. Set this parameter to use any other particles as a primary (e.g. the center of mass).


class
rebound.
reb_simulation_integrator_whfast
[source]¶ This class is an abstraction of the Cstruct reb_simulation_integrator_whfast. It controls the behaviour of the symplectic WHFast integrator described in Rein and Tamayo (2015).
This struct should be accessed via the simulation class only. Here is an example:
>>> sim = rebound.Simulation() >>> sim.ri_whfast.corrector = 11
Variables:  corrector (int) – The order of the symplectic corrector in the WHFast integrator. By default the symplectic correctors are turned off (=0). For high accuracy simulation set this value to 11. For more details read Rein and Tamayo (2015).
 recalculate_coordinates_this_timestep (int) – Sets a flag that tells WHFast that the particles have changed. Setting this flag to 1 (default 0) triggers the WHFast integrator to recalculate Jacobi/heliocenctric coordinates. This is needed if the user changes the particle position, velocity or mass inbetween timesteps. After every timestep the flag is set back to 0, so if you continuously update the particles manually, you need to set this flag to 1 after every timestep.
 coordinates (string) – Sets the internal coordinate system that WHFast is using. By default
it uses
'jacobi'
(=0) coordinates. Other options are'democraticheliocentric'
(=1) and'whds'
(=2). See Hernandez and Dehnen (2017) for more information.  safe_mode (int) – If safe_mode is 1 (default) particles can be modified between timesteps and particle velocities and positions are always synchronised. If you set safe_mode to 0, the speed and accuracy of WHFast improve. However, make sure you are aware of the consequences. Read the iPython tutorial on advanced WHFast usage to learn more.
Attributes

coordinates
¶ Get or set the internal coordinate system.
Available coordinate systems are:
'jacobi'
(default)'democraticheliocentric'
'whds'

class
rebound.
reb_simulation_integrator_sei
[source]¶ This class is an abstraction of the Cstruct reb_simulation_integrator_sei. It controls the behaviour of the symplectic SEI integrator for shearing sheet calculations. It is described in Rein and Tremaine (2011).
This struct should be accessed via the simulation class only. Here is an example:
>>> sim = rebound.Simulation() >>> sim.ri_sei.OMEGA = 1.58
Variables:  OMEGA (float) – The epicyclic frequency OMEGA. For simulations making use of shearing sheet boundary conditions, REBOUND needs to know the epicyclic frequency. By default OMEGA is 1. For more details read Rein and Tremaine 2011.
 OMEGAZ (float) – The z component of the epicyclic frequency OMEGA. By default it is assuming OMEGAZ is the same as OMEGA.