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  • Understanding Newton's Law of Universal Gravitation | Definition & Explanation
    The law of universal gravitation, often called Newton's law of gravity, states that:

    Every particle of matter in the universe attracts every other particle with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

    Here's a breakdown:

    * Every particle attracts every other particle: This means gravity is a universal force that applies to all objects with mass.

    * Proportional to the product of their masses: The more massive the objects, the stronger the gravitational force between them.

    * Inversely proportional to the square of the distance between their centers: The farther apart the objects are, the weaker the gravitational force between them. The force decreases rapidly as the distance increases.

    This law is represented mathematically by the following equation:

    F = G * (m1 * m2) / r²

    Where:

    * F is the force of gravity

    * G is the gravitational constant (approximately 6.674 x 10⁻¹¹ N⋅m²/kg²)

    * m1 and m2 are the masses of the two objects

    * r is the distance between the centers of the two objects

    This law explains why objects fall to the ground, why the planets orbit the sun, and why galaxies hold together. It's a fundamental law of physics that has had a profound impact on our understanding of the universe.

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