Gravity Physics Example 1

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Example 1

easy
Calculate the gravitational force between Earth (M=5.97×1024 kgM = 5.97 \times 10^{24} \text{ kg}) and a 1 kg1 \text{ kg} object at Earth's surface (r=6.37×106 mr = 6.37 \times 10^6 \text{ m}). Use G=6.674×1011 N m2/kg2G = 6.674 \times 10^{-11} \text{ N m}^2/\text{kg}^2.

Solution

  1. 1
    Apply Newton's law of gravitation: F=GMmr2F = \frac{GMm}{r^2}
  2. 2
    Substitute: F=6.674×1011×5.97×1024×1(6.37×106)2F = \frac{6.674 \times 10^{-11} \times 5.97 \times 10^{24} \times 1}{(6.37 \times 10^6)^2}
  3. 3
    Calculate: F=3.98×10144.06×10139.8 NF = \frac{3.98 \times 10^{14}}{4.06 \times 10^{13}} \approx 9.8 \text{ N}

Answer

F9.8 NF \approx 9.8 \text{ N}
This calculation confirms that g9.8 m/s2g \approx 9.8 \text{ m/s}^2 at Earth's surface. Gravity is the attractive force between any two masses, governed by the universal law of gravitation.

About Gravity

The universal attractive force between any two objects with mass, decreasing with the square of distance.

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