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  1. The gravity of Earth, denoted by g, is the net acceleration that is imparted to objects due to the combined effect of gravitation (from mass distribution within Earth) and the centrifugal force (from the Earth's rotation ). [2] [3] It is a vector quantity, whose direction coincides with a plumb bob and strength or magnitude is given by the norm .

  2. At a fixed point on the surface, the magnitude of Earth's gravity results from combined effect of gravitation and the centrifugal force from Earth's rotation. At different points on Earth's surface, the free fall acceleration ranges from 9.764 to 9.834 m/s 2 (32.03 to 32.26 ft/s 2), depending on altitude, latitude, and longitude.

  3. Learn about gravity, the universal force of attraction acting between all matter, and its effects on Earth and the cosmos. Find out the acceleration of gravity on Earth and how it differs from other planets and the Moon.

  4. Free Falling objects are falling under the sole influence of gravity. This force causes all free-falling objects on Earth to have a unique acceleration value of approximately 9.8 m/s/s, directed downward. We refer to this special acceleration as the acceleration caused by gravity or simply the acceleration of gravity.

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  6. Calculate Earth’s mass given that the acceleration due to gravity at the North Pole is 9.830 m/s 2 and the radius of the Earth is 6371 km from pole to center. 5.94 × 10 17 kg 5.94 × 10 24 kg

  7. Gravity - Acceleration, Earth, Moon: The value of the attraction of gravity or of the potential is determined by the distribution of matter within Earth or some other celestial body. In turn, as seen above, the distribution of matter determines the shape of the surface on which the potential is constant. Measurements of gravity and the potential are thus essential both to geodesy, which is the ...

  8. A simpler expression, equation (5), gives the surface acceleration on Earth. Setting a mass equal to Earth’s mass M E and the distance equal to Earth’s radius r E, the downward acceleration of a body at the surface g is equal to the product of the universal gravitational constant and the mass of Earth divided by the square of the radius:

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