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 x 1024 kg, and 7.36 x 1022 kg, respectively. The Moon's mean distance from Earth is 3.84 × 10° m, and Earth's mean distance from the Sun is 1.50 × 10'1 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

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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 × 1024 kg, and 7.36 × 1022 kg, respectively. The Moon's
mean distance from Earth is 3.84 × 10% 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
Transcribed Image Text: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 × 1024 kg, and 7.36 × 1022 kg, respectively. The Moon's mean distance from Earth is 3.84 × 10% 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
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