“…Taking into account the oblateness of the Earth, in model ( 4), (5), under the condition h Kf = h Kg , by virtue of integral (10), the initial velocity is determined from the relation ( 16) where Let us provide numerical estimates for the case z 0 = 0. When flying from the Earth to a planet in a geocentric orbit with V ∞ = 3-4 km/s, taking into account the Earth's oblateness in (17), increases initial velocity V 0 in comparison with Keplerian case (16) from ~11.410-11.713 to ~11.413-11.716 km/s, i.e., by ~3 m/s.…”