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Gravitation describes the force by which two masses attract each other, a fundamental concept governing planetary motion and the behavior of objects on Earth. Newton's Universal Law of Gravitation quantitatively expresses this interaction through a specific formula. Key phenomena like free fall, differences between mass and weight, and gravitational fields are explored, along with their implications in real-world applications such as satellite motion and structural design.
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References
p11-6.pdfClass Notes
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What we have learnt
Final Test
Revision Tests
Term: Gravitation
Definition: The force that pulls two objects toward each other, proportional to their masses and inversely proportional to the square of the distance between them.
Term: Newton's Universal Law of Gravitation
Definition: A law stating that every mass attracts every other mass in the universe with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between their centers.
Term: Free Fall
Definition: The motion of a body when it is falling solely under the influence of gravitational force.
Term: Weightlessness
Definition: A condition in which no net gravitational force is acting on an object, making it feel as if it has no weight.
Term: Gravitational Field
Definition: The region around a mass where its gravitational force can be felt, with strength diminishing as the distance from the mass increases.