Going to Mars with Python using poliastro¶
This is an example on how to use poliastro, a little library I’ve been working on to use in my Astrodynamics lessons. It features conversion between classical orbital elements and position vectors, propagation of Keplerian orbits, initial orbit determination using the solution of the Lambert’s problem and orbit plotting.
In this example we’re going to draw the trajectory of the mission Mars Science Laboratory (MSL), which carried the rover Curiosity to the surface of Mars in a period of something less than 9 months.
Note: This is a very simplistic analysis which doesn’t take into account many important factors of the mission, but can serve as an starting point for more serious computations (and as a side effect produces a beautiful plot at the end).
First of all, we import the necessary modules. Apart from poliastro we will make use of astropy to deal with physical units and time definitions and jplephem to compute the positions and velocities of the planets:
from astropy import units as u from astropy import time import numpy as np from poliastro import iod from poliastro.bodies import Earth, Mars, Sun from poliastro.ephem import Ephem from poliastro.maneuver import Maneuver from poliastro.twobody import Orbit from poliastro.util import time_range
# More info: https://plotly.com/python/renderers/ import plotly.io as pio pio.renderers.default = "plotly_mimetype+notebook_connected"
We need a binary file from NASA called SPICE kernel to compute the position and velocities of the planets. Astropy downloads it for us:
from astropy.coordinates import solar_system_ephemeris solar_system_ephemeris.set("jpl")
<ScienceState solar_system_ephemeris: 'jpl'>
The initial data was gathered from Wikipedia: the date of the launch was on November 26, 2011 at 15:02 UTC and landing was on August 6, 2012 at 05:17 UTC. We compute then the time of flight, which is exactly what it sounds:
# Initial data date_launch = time.Time("2011-11-26 15:02", scale="utc").tdb date_arrival = time.Time("2012-08-06 05:17", scale="utc").tdb
To compute the transfer orbit, we have the useful function
lambert : according to a theorem with the same name, the transfer orbit between two points in space only depends on those two points and the time it takes to go from one to the other. We could make use of the raw algorithms available in
poliastro.iod for solving this but working with the
poliastro.maneuvers is even easier!
We just need to create the orbits for each one of the planets at the specific departure and arrival dates:
earth = Ephem.from_body(Earth, time_range(date_launch, end=date_arrival)) mars = Ephem.from_body(Mars, time_range(date_launch, end=date_arrival))
# Solve for departure and target orbits ss_earth = Orbit.from_ephem(Sun, earth, date_launch) ss_mars = Orbit.from_ephem(Sun, mars, date_arrival)
We can now solve for the maneuver that will take us from Earth to Mars. After solving it, we just need to apply it to the departure orbit to solve for the transfer one:
# Solve for the transfer maneuver man_lambert = Maneuver.lambert(ss_earth, ss_mars) # Get the transfer and final orbits ss_trans, ss_target = ss_earth.apply_maneuver(man_lambert, intermediate=True)
Let’s plot this transfer orbit in 3D!
from poliastro.plotting import OrbitPlotter3D
plotter = OrbitPlotter3D() plotter.set_attractor(Sun) plotter.plot_ephem(earth, date_launch, label="Earth at launch position") plotter.plot_ephem(mars, date_arrival, label="Mars at arrival position") plotter.plot_trajectory( ss_trans.sample(max_anomaly=180 * u.deg), color="black", label="Transfer orbit", ) plotter.set_view(30 * u.deg, 260 * u.deg, distance=3 * u.km)
/tmp/ipykernel_2105/2813620182.py:7: DeprecationWarning: Specifying min_anomaly and max_anomaly in method `sample` is deprecated and will be removed in a future release, use `Orbit.to_ephem(strategy=TrueAnomalyBounds(min_nu=..., max_nu=...))` instead
Not bad! Let’s celebrate with some music!
from IPython.display import YouTubeVideo YouTubeVideo("zSgiXGELjbc")