Surface Gravity Formula:
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The surface gravity formula calculates the gravitational acceleration at the surface of a celestial body based on its density and radius. It's derived from Newton's law of universal gravitation and the relationship between mass, density, and volume.
The calculator uses the surface gravity formula:
Where:
Explanation: The formula accounts for the mass distribution within a spherical object, relating density directly to surface gravity without needing to calculate mass separately.
Details: Surface gravity is crucial in astrophysics for understanding planetary characteristics, atmospheric retention, and potential habitability. It's also important for space mission planning.
Tips: Enter the gravitational constant (default is Earth's value), density in kg/m³, and radius in meters. All values must be positive numbers.
Q1: Why use this formula instead of g = GM/R²?
A: This version is useful when you know the density rather than the total mass of the object. It's mathematically equivalent but uses different input parameters.
Q2: What are typical surface gravity values?
A: Earth's surface gravity is about 9.81 m/s². Moon's is 1.62 m/s², Jupiter's is 24.79 m/s² at the cloud tops.
Q3: Does this formula work for non-spherical objects?
A: It's an approximation that works best for roughly spherical objects. For irregular shapes, more complex calculations are needed.
Q4: How does density affect surface gravity?
A: Higher density leads to stronger surface gravity for a given radius, as it means more mass is concentrated in the same volume.
Q5: Can this be used for artificial objects?
A: Yes, it can calculate surface gravity for any spherical object, including artificial space habitats or theoretical constructs.