Take the mean distances of the Moon and the Sun from Earth to be 0.4×106 km and 150×106 km, respectively. Their masses are 8×1022 kg and 2×1030 kg, respectively. Let δF1 be the difference in the forces exerted by the Moon at the nearest and farthest points on Earth, and let δF2 be the corresponding difference due to the Sun. The number closest to δF2δF1 is:
(1) 2
(2) 6
(3) 10−2
(4) 0.6