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  1. 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 their masses and inversely proportional to the square of the distance between their centers of mass. This is called an inverse-square law.

  2. Coulomb's inverse-square law, or simply Coulomb's law, is an experimental law [1] of physics that calculates the amount of force between two electrically charged particles at rest. This electric force is conventionally called the electrostatic force or Coulomb force. [2] Although the law was known earlier, it was first published in 1785 by ...

  3. Both forces act along the imaginary line joining the objects. Both forces are inversely proportional to the square of the distance between the objects, this is known as the inverse-square law. Also, both forces have proportionality constants. F g uses G and F E uses k , where k = 9.0 × 10 9 N ⋅ m 2 C 2 .

  4. A Coulomb is a charge which repels an equal charge of the same sign with a force of 9×10 9 N when the charges are one metre apart in a vacuum. Coulomb force is the conservative mutual and internal force. The value of εo is 8.86 × 10-12 C2/Nm2 (or) 8.86 × 10-12 Fm–1. Note: Coulomb force is true only for static charges.

  5. Apr 25, 2024 · The formula for the force of attraction is expressed as follows: Fg = Gm1m2 d2 F g = G m 1 m 2 d 2. Here: F represents the force of attraction. G is the gravitational constant (6.67 × 10 -11 Nm 2 /kg 2 ), m 1 is the mass of the first object, m 2 is the mass of the second object, and. d is the distance between the two objects.

  6. en.wikipedia.org › wiki › GravityGravity - Wikipedia

    The force of gravity on Earth is the resultant (vector sum) of two forces: (a) The gravitational attraction in accordance with Newton's universal law of gravitation, and (b) the centrifugal force, which results from the choice of an earthbound, rotating frame of reference.

  7. Apr 10, 2022 · Gravity, the attractive force between all masses, is what keeps the planets in orbit. Newton’s universal law of gravitation relates the gravitational force to mass and distance: Fgravity = GM1M2 R2 F g r a v i t y = G M 1 M 2 R 2. The force of gravity is what gives us our sense of weight.

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