Gravity Formula:
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The gravity formula calculates the acceleration due to gravity using Newton's law of universal gravitation. It determines the gravitational acceleration at a specific distance from the center of a celestial body.
The calculator uses the gravity formula:
Where:
Explanation: The formula shows that gravitational acceleration is directly proportional to the mass of the object and inversely proportional to the square of the distance from its center.
Details: Calculating gravitational acceleration is essential for space missions, satellite operations, geological studies, and understanding planetary characteristics in astronomy and astrophysics.
Tips: Enter mass in kilograms and radius in meters. Both values must be positive numbers greater than zero for accurate calculation.
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, with a value of approximately 6.67430 × 10⁻¹¹ m³/kg s².
Q2: How does gravity change with altitude?
A: Gravity decreases with the square of the distance from the center of the mass. As altitude increases, gravitational acceleration decreases.
Q3: What is Earth's surface gravity?
A: Approximately 9.8 m/s² at Earth's surface, though this varies slightly depending on location due to Earth's oblate shape and geological density variations.
Q4: Can this formula be used for any celestial body?
A: Yes, the formula applies to any spherical body with mass, including planets, moons, stars, and other astronomical objects.
Q5: Why is the gravitational constant so small?
A: The small value of G reflects the relative weakness of gravity compared to other fundamental forces, which is why we only notice gravitational effects with very large masses.