What best describes Newton law of universal gravitation

Newton's law of universal gravitation states that every particle in the universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

To calculate the gravitational force between two objects using this law, you need the following information:

1. The masses of the two objects (m1 and m2): These are typically given in kilograms.

2. The distance between the centers of the two objects (r): This is measured in meters.

Once you have this information, you can calculate the gravitational force (F) using the following formula:

F = G * (m1 * m2) / r^2

where G is the gravitational constant, which is approximately equal to 6.67430 × 10^-11 N(m/kg)^2.

To find the best description of Newton's law of universal gravitation, you could say that it explains how every particle with mass attracts every other particle with mass, and the strength of this attraction is determined by their masses and the distance between them.

F=G*M1*M2/r^2