During a solar eclipse, the Moon is positioned directly between Earth and the Sun. The masses of the Sun, Earth, and the Moon are 1.99 x 1030 kg, 5.98 x 1024 kg, and 7.36 x 1022 kg, respectively. The Moon's Macmillan Learning mean distance from Earth is 3.84 x 108 m, and Earth's mean distance from the Sun is 1.50 x 10" m. The gravitational constant is G = 6.67 x 10-11 N.m2/kg2. Find the magnitude F of the net gravitational force acting on the Moon during the solar eclipse due to both Earth and the Sun. F = N What is the direction of this force? O toward the Sun O toward Earth O elsewhere O toward Venus