A Study about the Integration of the Elliptical Orbital Motion Based on a Special One-Parametric Family of Anomalies

Figure 2

Points distribution for 𝑒=0.7, 𝛼=0.0,0.5,0.75,1.0.

(a) 𝛼=0.0

(b) 𝛼=0.5

(c) 𝛼=0.75

(d) 𝛼=1.0