#!/usr/bin/env python # coding: utf-8 # In[1]: get_ipython().run_line_magic('matplotlib', 'inline') import numpy as np import matplotlib.pyplot as plt from mpl_toolkits.axes_grid1.inset_locator import zoomed_inset_axes from mpl_toolkits.axes_grid1.inset_locator import mark_inset from astropy import units as u from poliastro.bodies import Earth from poliastro.twobody import State from poliastro.maneuver import Maneuver # In[2]: ZOOM = True R = np.linspace(2, 75, num=100) Rstar = [15.58, 40, 60, 100, 200, np.inf] hohmann_data = np.zeros_like(R) bielliptic_data = np.zeros((len(R), len(Rstar))) ss_i = State.circular(Earth, 1.8 * u.km) r_i = ss_i.a v_i = np.sqrt(ss_i.v.dot(ss_i.v)) for ii, r in enumerate(R): r_f = r * r_i man = Maneuver.hohmann(ss_i, r_f) hohmann_data[ii] = (man.get_total_cost() / v_i).decompose().value for jj, rstar in enumerate(Rstar): r_b = rstar * r_i man = Maneuver.bielliptic(ss_i, r_b, r_f) bielliptic_data[ii, jj] = (man.get_total_cost() / v_i).decompose().value idx_max = np.argmax(hohmann_data) ylims = (0.35, 0.6) # In[3]: plt.style.use('pybonacci') fig, ax = plt.subplots(figsize=(8, 6)) l, = ax.plot(R, hohmann_data, lw=2) for jj in range(len(Rstar)): ax.plot(R, bielliptic_data[:, jj], color=l.get_color()) ax.vlines([11.94, R[idx_max]], *ylims, color='0.6') if ZOOM: ax_zoom = zoomed_inset_axes(ax, 4, loc=4, axes_kwargs={'axisbg': '0.97'}) ax_zoom.plot(R, hohmann_data, lw=2) for jj in range(len(Rstar)): ax_zoom.plot(R, bielliptic_data[:, jj], color=l.get_color()) ax_zoom.vlines([11.94, R[idx_max]], *ylims, color='0.6') ax_zoom.set_xlim(11.0, 16.0) ax_zoom.set_ylim(0.52, 0.545) ax_zoom.set_xticks([]) ax_zoom.set_yticks([]) ax_zoom.grid(False) ax_zoom.set_title("4x zoom") mark_inset(ax, ax_zoom, loc1=1, loc2=3, fc="none", ec='0.3') ax.set_xlabel("R") ax.set_ylabel("Relative change in velocity") ax.set_ylim(*ylims) ax.set_xlim(2, 75) ax.set_title("Hohmann vs bielliptic transfers") # In[ ]: