Gravity Equation:
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The acceleration due to gravity equation calculates the gravitational acceleration at a distance from a celestial body's center. It's derived from Newton's law of universal gravitation and is fundamental in physics and astronomy.
The calculator uses the gravity equation:
Where:
Explanation: This equation describes how the gravitational force between two objects decreases with the square of the distance between them.
Details: Calculating gravitational acceleration is essential for space missions, satellite operations, understanding planetary physics, and many engineering applications where gravity affects system behavior.
Tips: Enter mass in kilograms and radius in meters. Both values must be positive numbers. For Earth's surface gravity, use M = 5.972 × 10²⁴ kg and r = 6.371 × 10⁶ m.
Q1: What is the standard value of g on Earth's surface?
A: Approximately 9.8 m/s², though it varies slightly with location and altitude.
Q2: How does gravity change with altitude?
A: Gravity decreases with the square of the distance from the center of mass, so it decreases as altitude increases.
Q3: Why is the gravitational constant so small?
A: The gravitational constant is a fundamental physical constant that reflects the relative weakness of gravity compared to other fundamental forces.
Q4: Can this equation be used for any celestial body?
A: Yes, the equation works for any spherical body when you know its mass and the distance from its center.
Q5: How accurate is this calculation?
A: For spherical bodies with uniform density, it's highly accurate. For non-spherical bodies or those with non-uniform density, additional corrections may be needed.