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6. Gravitation
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.
Sections
Gravitation is the universal force of attraction between masses, significantly influencing celestial and terrestrial phenomena.
Gravitation is the force that attracts every object in the universe to every other object.
Newton’s Universal Law of Gravitation can be expressed through the formula F = G (m₁ × m₂) / r².
The concepts of mass and weight are distinct, with mass being a measure of matter while weight is the force of gravity acting on that mass.
Gravitation
The force that pulls two objects toward each other, proportional to their masses and inversely proportional to the square of the distance between them.
Newton's Universal Law of Gravitation
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.
Free Fall
The motion of a body when it is falling solely under the influence of gravitational force.
Weightlessness
A condition in which no net gravitational force is acting on an object, making it feel as if it has no weight.
Gravitational Field
The region around a mass where its gravitational force can be felt, with strength diminishing as the distance from the mass increases.
Practice Exercises
Total Questions
4
Estimated Time
8 min
Passing Score
70%
Instructions
- Read each question carefully
- You can use hints if you need help
- Complete all questions before submitting