“…The standard maneuver can be identified by the following three parameters: r ap , the minimum distance between the fragment and the Earth during the closest approach; v − inf and v + inf , the velocities of the particle with respect to the Earth, before and after the passage, respectively; v 2 , the Earth velocity around the Sun; δ, half of the angle of the curvature due to the close approach; and , the angle of approach, that is, the angle between the line connecting the primaries and the periapsis of the close approach trajectory. The velocity and orbital elements of m 2 are changed by the close approach with the Earth (Formiga and Prado 2015;dos Santos et al 2013). The orbital elements of each fragment with respect to the Sun before the maneuver are semi-major axis (a), eccentricity (e), energy (E) and angular momentum (C).…”