Gravity unit text

Unit 5 Lesson 9

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Gravity is the force that attracts two objects with mass towards each other. The strength of gravity depends on the mass of the objects and the distance between them. The formula to calculate the force of gravity between two objects is:

F = (G * m1 * m2) / r^2

where F is the force of gravity, G is the gravitational constant (approximately 6.673 * 10^-11 Nm^2/kg^2), m1 and m2 are the masses of the objects, and r is the distance between the centers of the objects.

Gravity is a fundamental force in the universe and affects all objects. It is responsible for keeping planets in orbit around the sun, causing objects to fall towards the Earth, and even influencing the motion of galaxies.

The force of gravity is always attractive, meaning it pulls objects towards each other. The larger the masses of the objects and the closer they are, the stronger the force of gravity. However, the force of gravity decreases rapidly with distance. This means that the farther apart two objects are, the weaker the force of gravity between them.

Gravity is also responsible for creating the shape of celestial bodies such as planets and stars. The force of gravity acts equally in all directions, pulling matter towards the center. This creates a spherical shape because the force of gravity compresses the matter towards the center, causing it to form a ball shape.

In summary, gravity is a force that attracts two objects with mass towards each other. Its strength depends on the masses of the objects and the distance between them. It is responsible for the motion of celestial bodies, the falling of objects on Earth, and the overall structure of the universe.

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