Gravitational Force Formula:
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Definition: Newton's law of universal gravitation calculates the attractive force between two masses.
Purpose: This fundamental physics equation helps understand celestial mechanics, satellite orbits, and gravitational interactions.
The formula is:
Where:
Explanation: The force is directly proportional to the product of the masses and inversely proportional to the square of the distance.
Details: This fundamental force governs planetary motion, tides, and the structure of the universe. It's essential for space mission planning and understanding astrophysical phenomena.
Tips: Enter the masses of both objects in kilograms and their separation distance in meters. The gravitational constant is fixed at 6.67 × 10⁻¹¹ N m²/kg².
Q1: Why is the gravitational constant so small?
A: The value reflects the relative weakness of gravity compared to other fundamental forces. It means significant masses are needed to produce measurable forces.
Q2: Does this work for any distance?
A: The formula applies to point masses or spherical objects at any distance, though extremely small distances may require quantum gravity considerations.
Q3: How accurate is this calculation?
A: Extremely accurate for most applications, though Einstein's general relativity provides more precise results in strong gravitational fields.
Q4: What's a typical gravitational force between everyday objects?
A: Very small - for example, two 100kg people 1m apart experience about 0.000000667 N of force.
Q5: Why is the distance squared in the formula?
A: This inverse-square law reflects how gravity's influence spreads over an expanding spherical surface area as distance increases.