Surface Gravity Equation:
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Surface gravity (g) is the gravitational acceleration experienced at the surface of a planet or celestial body. It depends on the body's mass and radius, and determines how much objects weigh on that surface.
The calculator uses the surface gravity equation:
Where:
Explanation: The equation shows that gravity decreases with the square of distance from the center and increases linearly with mass.
Details: Understanding surface gravity is crucial for space missions, planetary science, and determining if a planet can retain an atmosphere or support life as we know it.
Tips: Enter the gravitational constant (default is Earth's value), planet mass in kilograms, and distance from center in meters. All values must be positive numbers.
Q1: What's Earth's surface gravity?
A: Approximately 9.81 m/s² at sea level, though it varies slightly by location.
Q2: How does gravity change with altitude?
A: Gravity decreases with the square of distance from the planet's center, so higher altitudes experience slightly less gravity.
Q3: Why is G so small in value?
A: The gravitational constant is a fundamental physical constant that reflects the relative weakness of gravity compared to other forces.
Q4: Can this calculate gravity inside a planet?
A: No, this equation only works for points outside a planet's surface. Internal gravity calculations require different formulas.
Q5: What's the surface gravity of Mars?
A: About 3.71 m/s², which is roughly 38% of Earth's gravity.