Earth Gravity Formula:
From: | To: |
Earth's gravity (g) varies slightly depending on location due to factors like latitude and altitude. The standard gravity is defined as 9.80665 m/s², but actual values range from about 9.78 m/s² at the equator to 9.83 m/s² at the poles.
The calculator uses the international gravity formula:
Where:
Explanation: The formula accounts for Earth's oblate shape (greater gravity at poles) and reduced gravity at higher altitudes.
Details: Precise gravity values are essential for geophysical surveys, metrology, space missions, and scientific experiments requiring high precision measurements.
Tips: Enter latitude in decimal degrees (-90 to 90) and altitude in meters above sea level. For best results, use precise coordinates.
Q1: Why does gravity vary with latitude?
A: Earth's rotation creates centrifugal force that counteracts gravity, and the planet's oblate shape means you're farther from the center at the equator.
Q2: What is standard gravity?
A: 9.80665 m/s² is the conventional value representing average gravity at Earth's surface, used for definitions like kilogram-force.
Q3: How much does altitude affect gravity?
A: Gravity decreases by about 0.3086 mGal/meter (0.0003086 m/s² per meter) of elevation gain.
Q4: What's the difference between g and G?
A: g is local gravitational acceleration (m/s²), while G is the universal gravitational constant (6.674×10⁻¹¹ N·m²/kg²).
Q5: Does local geology affect gravity?
A: Yes, but this calculator doesn't account for local density variations which typically cause variations of ±0.01 m/s².