Acceleration Due To Gravity Formula:
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The acceleration due to gravity formula calculates the gravitational acceleration experienced by an object due to the gravitational force exerted by a celestial body. It is derived from Newton's law of universal gravitation.
The calculator uses the acceleration due to gravity formula:
Where:
Explanation: This formula calculates the gravitational acceleration at a specific distance from the center of a celestial body, showing how gravity decreases with the square of the distance.
Details: Calculating gravitational acceleration is essential for space missions, satellite orbits, planetary science, and understanding fundamental physics principles. It helps determine orbital velocities, escape velocities, and gravitational forces.
Tips: Enter the gravitational constant (default is 6.67430e-11), mass of the celestial body in kilograms, and distance from the center in meters. All values must be positive numbers.
Q1: What is the standard value of Earth's gravity?
A: The standard acceleration due to gravity on Earth's surface is approximately 9.80665 m/s².
Q2: How does gravity change with altitude?
A: Gravity decreases with the square of the distance from the center of the Earth, so it decreases as altitude increases.
Q3: What is the gravitational constant G?
A: G is a fundamental physical constant that measures the strength of the gravitational force between two objects.
Q4: Can this formula be used for any celestial body?
A: Yes, this formula works for any celestial body when you input the correct mass and distance values.
Q5: Why is the distance squared in the formula?
A: The inverse square law reflects how gravitational force spreads out over a spherical surface area as distance increases.