Masses

Corps

kg

M sol

Soleil

Jupiter

Terre

Rayons

km

R sol

Corps

Soleil

Jupiter

Terre

demi-grand

km

u.a.

Corps

M jup

R jup

R sol

M terre

axes

Jupiter

Terre

B3 = 1.99E30
C3 = 1
B4 = 1.9E27
C4 = 9.55E-4
B5 = 5.97E24
C5 = 3.0E-6
B9 = 696342
C9 = 1
B10 = 71492
C10 = 0.10267
B11 = 6378
C11 = 0.00915
D3 = 1047.7
D4 = 1
D5 = 0.00315
D9 = 9.74
E9 = 109
D10 = 1
E10 = 11.2
D11 = 0.0892
E11 = 1
E3 = 333000
E4 = 317.8
E5 = 1
a = 5.2
M_E = 1
M_P = 1 (slider from -5 to 5, step 1)
R_E = 1
p: sqrt(a^(3) / (M_E + M_P / D3))
a_P: a * M_E / (M_E + M_P / D3)
a_E: a * M_P / D3 / (M_E + M_P / D3)
p_J: p * 365.25
G = (0, 0)
c_E = Circle(G, a_E)
c_P = Circle(G, a_P)
θ = 0.5969026041820608 rad (slider from 0*° to 6.283185307179586, step 0.1*°)
E: (a_E; θ)
P: (a_P; θ + π)
laps = Segment(E, P)
B15 = 7.78412027E8
C15 = 5.2
B16 = 1.49597888E8
C16 = 1
v_P: 2 * π * a_P * B16 / (p_J * 24 * 3600)
v_E: 2 * π * a_E * B16 / (p_J * 24 * 3600)
cr_E = Circle(E, R_E * B9 / B16)
α_E: 2 * atan(R_E * B9 / B16 / a) * 180 / π