Gravitational Acceleration Formula:
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The gravitational acceleration formula calculates the acceleration due to gravity at a specific distance from a mass. It is derived from Newton's law of universal gravitation and describes how gravitational force decreases with the square of the distance from the mass center.
The calculator uses the gravitational acceleration formula:
Where:
Explanation: The formula shows that gravitational acceleration is directly proportional to the mass and inversely proportional to the square of the distance from the mass center.
Details: Calculating gravitational acceleration is essential for understanding orbital mechanics, planetary science, satellite deployment, and various engineering applications. It helps determine the gravitational field strength around celestial bodies.
Tips: Enter mass in kilograms, distance in meters, and gravitational constant in m³ kg⁻¹ s⁻². All values must be positive numbers. The default gravitational constant is set to 6.67430×10⁻¹¹, but you can modify it if needed.
Q1: What is the gravitational constant?
A: The gravitational constant (G) is a fundamental physical constant that determines the strength of the gravitational force between objects with mass.
Q2: Why does gravitational acceleration decrease with distance?
A: Gravitational acceleration follows an inverse-square law, meaning it decreases with the square of the distance from the mass center due to the spreading of gravitational field lines.
Q3: What is Earth's gravitational acceleration at surface?
A: Approximately 9.8 m/s², calculated using Earth's mass (5.972×10²⁴ kg) and radius (6.371×10⁶ m).
Q4: Can this formula be used for any mass?
A: Yes, the formula applies to any mass, from small objects to planets and stars, as long as the distance is measured from the center of mass.
Q5: How accurate is the gravitational constant?
A: The gravitational constant is known with relatively low precision compared to other fundamental constants, with current value 6.67430(15)×10⁻¹¹ m³ kg⁻¹ s⁻².