“…To get another standard trajectory, we can variate the h value by a virtual choice of Venus' initial position, while leaving conditions (1) intact. With the help of this scheme, we managed to build an empiric GA sensitivity function S(h) [7,8] which gave the values of the probe's FP deflection under a relatively small IP change dh. The results were surprising: for h = (16 − 10) • 10 4 km, S(h) ∼ = 10 4 − 10 5 ; this means that, e.g., for h = 10, 000 km (4000 km over Venus' surface) an IP change dh = 1 km entails the FP shift of ~82,000 km, which can be detected from Earth (for simplicity, the Earth's gravity is not taken into consideration).…”