The moon is 3.9 × 105 km from Earth's center and 1.5 × 108 km from the Sun's center. The masses of earth and the sun are 6.0 × 1024 kg and 2.0 × 1030 kg, respectively. Find the ratio of the gravitational fields due to Earth and the Sun at the center of the Moon.
The gravitational force due to moon by Earth is
"F=\\frac{G(M_{Earth}M_{Moon})}{d^2}"
"F=\\frac{6.67\u00d710^{-11}(6\u00d710^{24}\u00d77.3\u00d710^{22})}{(3.9\u00d710^5)^2}=1.92\u00d710^{26} N"
The gravitational force due to Moon by Sun is
"F=\\frac{G(M_{Sun}M_{Moon})}{d^2}"
"F=\\frac{6.67\u00d710^{-11}(2\u00d710^{30}\u00d77.3\u00d710^{22})}{(1.5\u00d710^8)^2}=3.24\u00d710^{34}N"
The ratio of gravitation force due to earth and sun on the centre of moon is
"\\frac{3.24\u00d710^{34}}{1.92\u00d710^{26}}=1.69\u00d710^4"
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