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Calculate Gravity

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 equation:

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

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 galaxies. It's essential for understanding celestial mechanics and space exploration.

4. Using the Calculator

Tips: Enter masses in kilograms and distance in meters. All values must be positive numbers. The result shows the gravitational force in newtons (N).

5. Frequently Asked Questions (FAQ)

Q1: What is the gravitational constant (G)?
A: G is a fundamental physical constant that measures the strength of gravity. Its value is approximately 6.674×10⁻¹¹ N·m²/kg².

Q2: Why is the force so small for everyday objects?
A: Because G is extremely small, the gravitational force between everyday objects is negligible compared to other forces like electromagnetism.

Q3: Does this equation work for very large distances?
A: For astronomical distances, general relativity provides more accurate results, though Newton's law remains a good approximation in most cases.

Q4: What about very massive objects?
A: The equation works for any masses, but for extremely massive objects (like black holes), relativistic effects become significant.

Q5: How accurate is this calculation?
A: The calculation is mathematically exact based on Newton's law, though real-world measurements may have experimental uncertainties.

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