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ilc said:The attachment shows my approach to this problem, however, the answer is incorrect.
can anyone explain to me how i should be thinking of this problem?
To calculate the force, you will need to use the equation F = GmM/r^2, where G is the gravitational constant, m is the mass of the object, M is the mass of the planet or star, and r is the distance between the two objects.
The gravitational constant (G) is a fundamental constant that appears in the equation for gravitational force. It has a value of 6.67 x 10^-11 Nm^2/kg^2.
Yes, the equation F = GmM/r^2 can be used for any mass and radius, as long as the units are consistent (e.g. mass in kilograms and radius in meters).
The mass and radius directly affect the force according to the equation F = GmM/r^2. As the mass or radius increases, the force between two objects also increases. This is because the larger the mass or radius, the stronger the gravitational pull between the two objects.
The units of force when using the equation F = GmM/r^2 are newtons (N). This is the standard unit of force in the International System of Units (SI).