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Formula To Calculate Gravitational Force

Newton's Law of Universal Gravitation:

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

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1. What is Newton's Law of Universal Gravitation?

Newton's Law of Universal Gravitation states that every particle attracts every other particle in the universe with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

2. How Does the Calculator Work?

The calculator uses Newton's gravitational formula:

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

Where:

Explanation: The force between two objects increases with their masses and decreases with the square of the distance between them.

3. Importance of Gravitational Force

Details: This fundamental force governs planetary motion, tides, and the structure of the universe. It's essential for understanding astrophysics, orbital mechanics, and many Earth-based phenomena.

4. Using the Calculator

Tips: Enter masses in kilograms and distance in meters. All values must be positive numbers (distance must be greater than zero).

5. Frequently Asked Questions (FAQ)

Q1: Why is the gravitational constant so small?
A: The gravitational force is extremely weak compared to other fundamental forces, which is reflected in the small value of G (6.674 × 10⁻¹¹ N·m²/kg²).

Q2: Does this work for any two objects?
A: Yes, the law applies to all objects with mass, though the force becomes negligible for everyday objects due to their small masses.

Q3: How accurate is this calculation?
A: It's accurate for point masses or spherical objects. For irregular shapes, integration over the volume is needed.

Q4: What about Einstein's theory of relativity?
A: Newton's law is an excellent approximation except in extreme gravitational fields or at velocities approaching light speed.

Q5: Why does distance have a squared relationship?
A: The inverse-square law comes from how gravitational influence spreads out in three-dimensional space.

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