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. 99×1030 kg, 5. 98×1024 kg, and 7. 36×1022 kg, respectively. The moon's mean distance from earth is 3. 84×108 m, and earth's mean distance from the sun is 1. 50×1011 m. The gravitational constant is =6. 67×10−11 n·m2/kg2. Find the magnitude of the net gravitational force acting on the moon during the solar eclipse due to both earth and the sun.