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  1. t. e. Newton's law of universal gravitation says that every particle attracts every other particle in the universe with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between their centers. Separated objects attract and are attracted as if all their mass were concentrated at ...

  2. But Newton’s formulation introduces the additional factor of the masses of the Sun ( M1) and the planet ( M2 ), both expressed in units of the Sun’s mass. Newton’s universal law of gravitation can be used to show mathematically that this relationship is actually. a 3 = ( M 1 + M 2) × P 2. where a is the semimajor axis and P is the ...

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    • Figure \\(\\PageIndex{1}\\): According to early accounts, Newton was inspired to make the connection between falling bodies and astronomical motions when he saw an apple fall from a tree and realized that if the gravitational force could extend above the ground to a tree, it might also reach the Sun.
    • Figure \\(\\PageIndex{2}\\): Gravitational attraction is along a line joining the centers of mass of these two bodies. The magnitude of the force is the same on each, consistent with Newton’s third law.
    • Figure \\(\\PageIndex{3}\\): The distance between the centers of mass of Earth and an object on its surface is very nearly the same as the radius of Earth, because Earth is so much larger than the object.
    • Figure \\(\\PageIndex{4}\\): The Moon causes ocean tides by attracting the water on the near side more than Earth, and by attracting Earth more than the water on the far side.
  4. The equation for Newton’s law of gravitation is: F g = G m 1 m 2 r 2. where: F g is the gravitational force between m 1 and m 2 , G is the gravitational constant equal to 6.67 × 10 − 11 m 3 kg ⋅ s 2 , and. m 1 and m 2 are masses. The force is directly proportional to the product of the masses. It is also inversely proportional to the ...

  5. Aug 11, 2021 · The equal but opposite force F 21 F → 21 is the force on object 2 exerted by object 1. Figure 13.2.1 13.2. 1: Gravitational force acts along a line joining the centers of mass of two objects. These equal but opposite forces reflect Newton’s third law, which we discussed earlier.

  6. 9.2: Newton’s Universal Theory of Gravity. Newton supposedly gained insight into the gravitational force by observing an apple falling from a tree and concluding that if it is the same force that makes apples fall at sea level and at the top of a mountain, perhaps that force can be exerted all the way up to the moon.

  7. 4.2 Newton’s First Law of Motion: Inertia; 4.3 Newton’s Second Law of Motion: Concept of a System; 4.4 Newton’s Third Law of Motion: Symmetry in Forces; 4.5 Normal, Tension, and Other Examples of Forces; 4.6 Problem-Solving Strategies; 4.7 Further Applications of Newton’s Laws of Motion; 4.8 Extended Topic: The Four Basic Forces—An ...

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