Gravitational Force Equation:
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Surface gravitational pull refers to the acceleration due to gravity at the surface of a celestial body. It determines how strongly objects are pulled toward the center of the body and affects weight, orbital mechanics, and various physical phenomena.
The calculator uses the gravitational force equation:
Where:
Explanation: The equation calculates the acceleration due to gravity at the surface of a planet or other celestial body based on its mass and radius.
Details: Calculating surface gravity is essential for space exploration, understanding planetary characteristics, designing spacecraft trajectories, and studying the physical properties of celestial bodies.
Tips: Enter mass in kilograms, radius in meters, and gravitational constant in N·m²/kg². The default value for G is 6.674 × 10⁻¹¹ N·m²/kg². All values must be positive numbers.
Q1: What is the gravitational constant?
A: The gravitational constant (G) is a fundamental physical constant that appears in Newton's law of universal gravitation. Its value is approximately 6.674 × 10⁻¹¹ N·m²/kg².
Q2: How does gravity vary with altitude?
A: Gravity decreases with the square of the distance from the center of mass. At higher altitudes, the gravitational pull is weaker than at the surface.
Q3: What is Earth's surface gravity?
A: Earth's surface gravity is approximately 9.8 m/s², though it varies slightly depending on location due to factors like latitude and altitude.
Q4: Can this calculator be used for any celestial body?
A: Yes, this calculator can be used for any planet, moon, or celestial body by inputting the appropriate mass and radius values.
Q5: Why is surface gravity important for space missions?
A: Surface gravity determines the thrust needed for launch, affects orbital calculations, and influences the design of landing systems and surface operations.