I. (09). m = 2 kg b = 3 meters g= 10 m/s Mass of Sun...

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I. (09). m = 2 kg b = 3 meters g= 10 m/s² Mass of Sun 2 x 1030 kg Earth - Sun Distance ≈ 1.5 x 10¹¹ m G≈ 6.67 x 10-¹1 Nm²/kg² i. In Newtons, determine an approximate numerical value for the amount of Gravitational Force exerted by the mass onto the center of Planet Earth. Assume: ii. In Newtons, determine an approximate numerical value for the amount of Gravitational Force exerted by the sun onto the center of Planet Earth. I. (09). m = 2 kg b = 3 meters g= 10 m/s² Mass of Sun 2 x 1030 kg Earth - Sun Distance ≈ 1.5 x 10¹¹ m G≈ 6.67 x 10-¹1 Nm²/kg² i. In Newtons, determine an approximate numerical value for the amount of Gravitational Force exerted by the mass onto the center of Planet Earth. Assume: ii. In Newtons, determine an approximate numerical value for the amount of Gravitational Force exerted by the sun onto the center of Planet Earth.

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i The gravitational force exerted by the mass onto the center of Planet Earth can be calculated usin... View the full answer