Formula Used:
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The gravitational constant (G) is the proportionality constant connecting the gravitational force between two bodies with the product of their masses and the inverse square of their distance. It is a fundamental constant of nature that appears in Newton's law of universal gravitation.
The calculator uses the formula:
Where:
Explanation: This formula derives the gravitational constant from Earth's gravitational acceleration, mean radius, and mass using Newton's law of universal gravitation.
Details: The gravitational constant is fundamental to understanding gravitational forces in the universe. It is essential for calculating planetary orbits, satellite trajectories, and cosmological phenomena. Accurate determination of G is crucial for precision measurements in astrophysics and space exploration.
Tips: Enter the mean radius of Earth in meters and gravitational acceleration in m/s². Standard values are approximately 6,371,000 meters for radius and 9.80665 m/s² for gravitational acceleration.
Q1: What is the accepted value of the gravitational constant?
A: The currently accepted value is approximately 6.67430 × 10⁻¹¹ N·m²/kg² as determined by precision laboratory measurements.
Q2: Why is the gravitational constant difficult to measure precisely?
A: Gravitational forces are extremely weak compared to other fundamental forces, making precise measurements challenging and susceptible to experimental errors.
Q3: How does this calculation compare to laboratory measurements?
A: This method provides a theoretical derivation based on Earth's parameters, while laboratory measurements use sensitive torsion balance experiments for direct measurement.
Q4: Can this formula be used for other celestial bodies?
A: Yes, the same principle applies to any celestial body when you know its mass, radius, and surface gravitational acceleration.
Q5: Why is Earth's mass used as a constant in this calculation?
A: Earth's mass (5.9722 × 10²⁴ kg) is a well-established value determined through various geophysical measurements and satellite observations.