Mark O. answered 04/29/19
Learn Physics, Math, and Comp Sci from Professional Scientist
We can look at the interaction of a planet in a gravitational interaction with another body, like a star like the Sun, a couple of different ways.
First, you can directly use Newton's Law of Universal Gravitation and calculate the force between the Earth and Sun. Let Me = 5.98 X 1024 kg be the mass of the earth and Ms = 1.99 X 1030 kg be the mass of the Sun. The center-to-center distance between the Earth and Sun is R = 1.5 X 1011m. Newton's Law of Universal Gravitation is
F = GMeMs / R2, where G = 6.67 X 10-11 Nm2 / kg2 is Newton's Universal Gravitational constant,
F = (6.67 X 10-11 Nm2 / kg2)(5.98 X 1024 kg)(1.99 X 1030 kg)/(1.5 X 1011m)2 = 3.5 X 1022 N
This is how the number that you were given was calculated.
Another way to look at this problem is to see the Earth as a test mass in the Sun's gravitational field. Let the gravitational field of the Sun be given by a function A(R) = GMs / R2, and any planet of mass M at a given distance R acts as a test mass in the Sun's gravitational field. For a given test mass M at a radial distance R from the Sun, the force would then be
F = M*A(R)
So, to get the value of the gravitational field at the location of the Earth, you would take the force value that you were given and divide it by the mass of the Earth:
A(R) = F/Me = 3.6 X 1022 N / 5.98 X 1024 kg = 6.02 X 10-3 N/kg