Source code for scenarioCustomGravBody

#
#  ISC License
#
#  Copyright (c) 2021, Autonomous Vehicle Systems Lab, University of Colorado at Boulder
#
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r"""

.. raw:: html

    <iframe width="560" height="315" src="https://www.youtube.com/embed/uUomHSGQW3c" frameborder="0" allow="accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture" allowfullscreen></iframe>

Overview
--------

Demonstrates how to setup a custom gravity object in Basilisk that is not directly supported by
the ``simIncludeGravBody.py`` file.  In this simulation the sun is created using standard values, the Earth
is created using custom values, and the asteroid Itokawa is created with custom values.

.. image:: /_images/static/scenarioCustomGravObject.jpg
   :align: center

Further, the Vizard binary file is setup to load up a custom CAD model for the asteroid. The spacecraft
orbit is defined relative to the asteroid.  Note, this feature requires :ref:`Vizard <vizard>` version 1.8 or higher.

The script is found in the folder ``basilisk/examples`` and executed by using::

      python3 scenarioCustomGravBody.py

The simulation layout is shown in the following illustration.  A single simulation process is created
which contains both modules.

.. image:: /_images/static/test_scenarioCustomGravBody.svg
   :align: center

:ref:`planetEphemeris` is used to create the planet ephemeris states. The sun is assumed to be stationary,
while Earth is on a circular orbit and Itokawa is on its elliptical heliocentric orbit.

The method ``createCustomGravObject()`` is used to create the BSK grav bodies for both earth and Itokawa.
The earth body is already supported in :ref:`simIncludeGravBody`, but in this script we show how this could
be customized.  The gravity body ephemeris states are connected to the :ref:`planetEphemeris` planet
state output messages.

Finally, the recorded states will all be relative to the inertial origin at the sun.  :ref:`planetEphemeris` does not
have the ``zeroBase`` capability as :ref:`spiceInterface` has.  This script also records the asteroid
states so that the plot is done of the spacecraft motion relative to the asteroid.

The simulation executes and shows a plot of the spacecraft motion relative to the asteroid.

Illustration of Simulation Results
----------------------------------

::

    show_plots = True

.. image:: /_images/Scenarios/scenarioCustomGravBody1.svg
   :align: center

"""

#
# Basilisk Scenario Script and Integrated Test
#
# Purpose:  Basic simulation showing how to setup a custom gravity object
# Author:   Hanspeter Schaub
# Creation Date:  Feb. 23, 2021
#

import os

import matplotlib.pyplot as plt
from Basilisk.simulation import planetEphemeris
from Basilisk.simulation import spacecraft
from Basilisk.utilities import (SimulationBaseClass, macros, simIncludeGravBody, vizSupport)
from Basilisk.utilities import orbitalMotion
from Basilisk.utilities import unitTestSupport


# The path to the location of Basilisk
# Used to get the location of supporting data.
fileName = os.path.basename(os.path.splitext(__file__)[0])



[docs] def run(show_plots): """ The scenarios can be run with the followings setups parameters: Args: show_plots (bool): Determines if the script should display plots """ path = os.path.dirname(os.path.abspath(__file__)) # Create simulation variable names simTaskName = "simTask" simProcessName = "simProcess" # Create a sim module as an empty container scSim = SimulationBaseClass.SimBaseClass() # # create the simulation process # dynProcess = scSim.CreateNewProcess(simProcessName) # create the dynamics task and specify the simulation time step information simulationTimeStep = macros.sec2nano(10.0) simulationTime = macros.min2nano(1120.0) dynProcess.addTask(scSim.CreateNewTask(simTaskName, simulationTimeStep)) # setup celestial object ephemeris module gravBodyEphem = planetEphemeris.PlanetEphemeris() gravBodyEphem.ModelTag = 'planetEphemeris' scSim.AddModelToTask(simTaskName, gravBodyEphem) gravBodyEphem.setPlanetNames(planetEphemeris.StringVector(["Itokawa", "earth"])) # specify orbits of gravitational bodies oeAsteroid = planetEphemeris.ClassicElementsMsgPayload() oeAsteroid.a = 1.3241 * orbitalMotion.AU * 1000 # meters oeAsteroid.e = 0.2801 oeAsteroid.i = 1.6214*macros.D2R oeAsteroid.Omega = 69.081*macros.D2R oeAsteroid.omega = 162.82*macros.D2R oeAsteroid.f = 90.0*macros.D2R oeEarth = planetEphemeris.ClassicElementsMsgPayload() oeEarth.a = orbitalMotion.AU * 1000 # meters oeEarth.e = 0.0167086 oeEarth.i = 7.155 * macros.D2R oeEarth.Omega = 174.9 * macros.D2R oeEarth.omega = 288.1 * macros.D2R oeEarth.f = 270.0 * macros.D2R # specify celestial object orbit gravBodyEphem.planetElements = planetEphemeris.classicElementVector([oeAsteroid, oeEarth]) # specify celestial object orientation gravBodyEphem.rightAscension = planetEphemeris.DoubleVector([0.0 * macros.D2R, 0.0 * macros.D2R]) gravBodyEphem.declination = planetEphemeris.DoubleVector([0.0 * macros.D2R, 0.0 * macros.D2R]) gravBodyEphem.lst0 = planetEphemeris.DoubleVector([0.0 * macros.D2R, 0.0 * macros.D2R]) gravBodyEphem.rotRate = planetEphemeris.DoubleVector( [360 * macros.D2R / (12.132 * 3600.), 360 * macros.D2R / (24. * 3600.)]) # setup Sun gravity body gravFactory = simIncludeGravBody.gravBodyFactory() gravFactory.createSun() # setup asteroid gravity body mu = 2.34268 # meters^3/s^2 asteroid = gravFactory.createCustomGravObject("Itokawa", mu, radEquator=200) asteroid.isCentralBody = True # ensure this is the central gravitational body asteroid.planetBodyInMsg.subscribeTo(gravBodyEphem.planetOutMsgs[0]) # setup Earth gravity Body earth = gravFactory.createCustomGravObject("earth", 0.3986004415E+15, radEquator=6378136.6) earth.planetBodyInMsg.subscribeTo(gravBodyEphem.planetOutMsgs[1]) # create SC object scObject = spacecraft.Spacecraft() scObject.ModelTag = "bskSat" gravFactory.addBodiesTo(scObject) scSim.AddModelToTask(simTaskName, scObject) # setup orbit initial conditions about the asteroid oe = orbitalMotion.ClassicElements() oe.a = 500.0 # meters oe.e = 0.0001 oe.i = 33.3 * macros.D2R oe.Omega = 48.2 * macros.D2R oe.omega = 347.8 * macros.D2R oe.f = 85.3 * macros.D2R rN, vN = orbitalMotion.elem2rv(mu, oe) # To set the spacecraft initial conditions, the following initial position and velocity variables are set: scObject.hub.r_CN_NInit = rN # m - r_BN_N scObject.hub.v_CN_NInit = vN # m/s - v_BN_N # # Setup data logging before the simulation is initialized # numDataPoints = 100 samplingTime = unitTestSupport.samplingTime(simulationTime, simulationTimeStep, numDataPoints) scRec = scObject.scStateOutMsg.recorder(samplingTime) astRec = gravBodyEphem.planetOutMsgs[0].recorder(samplingTime) scSim.AddModelToTask(simTaskName, scRec) scSim.AddModelToTask(simTaskName, astRec) # if this scenario is to interface with the BSK Viz, uncomment the following lines # to save the BSK data to a file, uncomment the saveFile line below # Note that the gravitational body information is pulled automatically from the spacecraft object(s) # Even if custom gravitational bodies are added, this information is pulled by the method below if vizSupport.vizFound: viz = vizSupport.enableUnityVisualization(scSim, simTaskName, scObject # , saveFile=fileName ) viz.settings.showSpacecraftLabels = 1 # load CAD for custom gravity model vizSupport.createCustomModel(viz, modelPath=os.path.join(path, "dataForExamples", "Itokawa", "ItokawaHayabusa.obj"), shader=1, simBodiesToModify=['Itokawa'], scale=[962, 962, 962]) # initialize Simulation scSim.InitializeSimulation() # configure a simulation stop time and execute the simulation run scSim.ConfigureStopTime(simulationTime) scSim.ExecuteSimulation() # retrieve logged spacecraft position relative to asteroid posData = scRec.r_BN_N - astRec.PositionVector # # plot the results # timeAxis = scRec.times() * macros.NANO2HOUR plt.close("all") # clears out plots from earlier test runs plt.figure(1) fig = plt.gcf() ax = fig.gca() ax.ticklabel_format(useOffset=False, style='plain') for idx in range(3): plt.plot(timeAxis, posData[:, idx] , color=unitTestSupport.getLineColor(idx, 3), label='$r_{BI,' + str(idx) + '}$') plt.legend(loc='lower right') plt.xlabel('Time [h]') plt.ylabel('Itokawa Relative Position [m]') figureList = {} pltName = fileName + "1" figureList[pltName] = plt.figure(1) if show_plots: plt.show() # close the plots being saved off to avoid over-writing old and new figures plt.close("all") return figureList
# # This statement below ensures that the unit test scrip can be run as a # stand-along python script # if __name__ == "__main__": run( True # show_plots )