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AQA / GCSE Science gravitation fully descriptive in depth notes including all exam related topics

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These comprehensive, 8-page physics revision notes are meticulously designed for the AQA GCSE Physics curriculum, focusing on the core principles of the meaning of gravitation... centripetal force...universal law of gravitation given by Sir Newton and its mathematical derivation...value and SI unit of G...importance of the law of gravitation...free fall and related topics...difference between G and g...equations of motion under gravity...sign convention...difference b/w mass and weight.....weight of an object on moon...thrust and pressure...buoyancy and archimedes principle...relative density...conceptual tricky topics for exam and many more..... The notes is perfect from exam POV since it is totally descriptive

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GRAVITATION (AQA / GCSE notes)




​​1. Introduction to Gravitation

​ ravitation is the force of attraction between any two
G
objects in the universe. Whether it's an apple falling
from a tree or the moon revolving around the Earth, the
universal force responsible is gravity.
​Centripetal Force

​ efore diving into gravity, it's important to understand
B
why objects move in circles (like planets around the
sun).

●​ ​Definition: The center-seeking force that causes an
object to move along a circular path is called the
centripetal force.
●​ ​If this force is removed, the object will fly off in a
straight line tangent to the circular path.

​2. Universal Law of Gravitation

​ roposed by Sir Isaac Newton, this law states that
P
every object in the universe attracts every other object
with a force.
​Statement

​The gravitational force between two objects is:

1.​​Directly proportional to the product of their
masses.

, 2.​​Inversely proportional to the square of the distance
between their centers.
​Mathematical Derivation

​ et two objects A and B have masses M and m,
L
separated by a distance d.

​According to the law:
Force(F) is directly proportional to M×m……………eq (1)


Force(F) is inveresly proportional to d^2……………eq (2)




Combining both equations:

Force(F) is directly proportional to M×m/d^2


To remove the proportionality sign, we introduce a constant G:


Force(F) = G M×m/d^2


Where:

●​ ​ = Gravitational force between the two bodies
F
●​ ​M, m = Masses of the two bodies
●​ ​d = Distance between the centers of the masses
●​ ​G = Universal Gravitational Constant




3. VALUE AND SI UNIT OF “G”


By rearranging the formula, we get:

G = F×d^2/M×m


●​ S​ I Unit of G: Nm^2/kg^2(Newton meter squared per kilogram squared)
●​ ​Value of G: 6.673 ×10^-11 Nm^2/kg^2(discovered by Henry Cavendish)

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