Surface Gravity Equation:
From: | To: |
Surface gravity (g) is the gravitational acceleration experienced at the surface of a celestial body. It determines the weight of objects and influences atmospheric retention and geological processes on planets and moons.
The calculator uses Newton's law of universal gravitation:
Where:
Explanation: The equation shows that surface gravity is directly proportional to mass and inversely proportional to the square of radius.
Details: Calculating surface gravity is essential for understanding planetary characteristics, space mission planning, exoplanet studies, and comparing different celestial bodies in our solar system and beyond.
Tips: Enter mass in kilograms and radius in meters. Both values must be positive numbers. For Earth: mass = 5.972 × 10²⁴ kg, radius = 6.371 × 10⁶ m.
Q1: Why is surface gravity different on other planets?
A: Surface gravity varies because planets have different masses and radii. Larger mass increases gravity, while larger radius decreases it.
Q2: What is Earth's surface gravity?
A: Earth's surface gravity is approximately 9.8 m/s², though it varies slightly depending on location and altitude.
Q3: How does surface gravity affect weight?
A: Weight = mass × gravity, so the same object will have different weights on celestial bodies with different surface gravities.
Q4: Can this formula be used for any celestial body?
A: Yes, this formula works for any spherical body where mass is evenly distributed, including planets, moons, and stars.
Q5: Why is the gravitational constant so small?
A: The gravitational constant is a fundamental physical constant that reflects the relative weakness of gravity compared to other fundamental forces.