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Formula To Calculate Acceleration Of Gravity

Gravity Formula:

\[ g = \frac{G M}{r^2} \]

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m

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1. What Is The Gravity Formula?

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.

2. How Does The Calculator Work?

The calculator uses the gravity formula:

\[ g = \frac{G M}{r^2} \]

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.

3. Importance Of Gravity Calculation

Details: Calculating gravitational acceleration is essential for space missions, satellite operations, geological studies, and understanding planetary characteristics in astronomy and astrophysics.

4. Using The Calculator

Tips: Enter mass in kilograms and radius in meters. Both values must be positive numbers greater than zero for accurate calculation.

5. Frequently Asked Questions (FAQ)

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.

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