Table 1: Position and Jacobi constant for the collinear equilibrium points L_i, i=1,2,3, and values of $\mu$ indicated. See the text for details.
$\mu =10^{-4}$ x_i $C_{{\rm J}_i}$

L₁ -1.0324251917 3.008955890917

L₂ -0.9680652061 3.009089235145

L₃ 1.0000416667 3.000199989791

$\mu=0.304018792\times10^{-5}$ x_i $C_{{\rm J}_i}$

L₁ -1.010074939199 3.000896881934

L₂ -0.989986240081 3.000900935559

L₃ 1.000001266745 3.000006080366

**Table 1:** Position and Jacobi constant for the collinear equilibrium points L_i, i=1,2,3, and values of $\mu$ indicated. See the text for details.
$\mu =10^{-4}$	x_i	$C_{{\rm J}_i}$
L₁	-1.0324251917	3.008955890917
L₂	-0.9680652061	3.009089235145
L₃	1.0000416667	3.000199989791
$\mu=0.304018792\times10^{-5}$	x_i	$C_{{\rm J}_i}$
L₁	-1.010074939199	3.000896881934
L₂	-0.989986240081	3.000900935559
L₃	1.000001266745	3.000006080366

Source LaTeX | All tables | In the text

	1 Introduction
	2 Basic aspects
	3 Planar horseshoe orbits
	4 Bifurcating 3D families
	5 Conclusions
	References