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Gravitational Force In Physics

Gravitational Force Formula:

\[ F = G \frac{m_1 m_2}{r^2} \]

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1. What is Gravitational Force?

Definition: Gravitational force is the attractive force between any two objects with mass, described by Newton's Law of Universal Gravitation.

Purpose: This calculator helps students, physicists, and engineers compute the gravitational attraction between two masses.

2. How Does the Calculator Work?

The calculator uses the formula:

\[ F = G \frac{m_1 m_2}{r^2} \]

Where:

Explanation: The force is directly proportional to the product of the masses and inversely proportional to the square of the distance between them.

3. Importance of Gravitational Force

Details: Understanding gravitational force is fundamental to celestial mechanics, satellite motion, and many engineering applications.

4. Using the Calculator

Tips: Enter the masses of both objects in kilograms and their separation distance in meters. All values must be > 0.

5. Frequently Asked Questions (FAQ)

Q1: Why is the gravitational constant so small?
A: The small value reflects the weakness of gravity compared to other fundamental forces at small scales.

Q2: Does this work for celestial bodies?
A: Yes, the same formula applies to planets, stars, and galaxies, though relativistic effects become important at extreme scales.

Q3: What if the distance is zero?
A: The formula breaks down at r=0, as objects can't occupy the same space and quantum effects become significant.

Q4: How accurate is this calculation?
A: It's accurate for classical physics problems, but doesn't account for general relativistic effects in strong gravitational fields.

Q5: Why does the result have so many decimal places?
A: Due to the extremely small gravitational constant, results are typically very small numbers requiring high precision.

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