π Acceleration Due to Gravity (g)
πΉ Definition
The acceleration due to gravity is the acceleration produced in a body when it is freely falling towards the Earth under the influence of Earthβs gravitational force.
It is denoted by g.
Near the Earthβs surface, its average value is 9.8 m/sΒ².
This means that the velocity of a freely falling body increases by about 9.8 m/s every second in the absence of air resistance.
πΉ Derivation: Relation of g with Distance from Earthβs Center
The universal law of gravitation gives the force between the Earth and a body of mass m as:
F=GMm/r2
Where:
GΒ = Universal gravitational constant
MΒ = Mass of the Earth
rΒ = Distance between the center of the Earth and the body
From Newtonβs second law:
F=mg
Equating the two forces:
mg=GMm/r2
Cancelling m:
g=GM/r2
πΉ Important Points
At the surface of the Earth
r=R(radius of Earth)g=GM/R2
At a height (h) above the surface
r=R+hgh=GM/(R+h)2
At the center of the Earth
Effectively, g=0 because all forces cancel out.
πΉ Conclusion
The value of gΒ decreases as the distance from the Earthβs center increases.
Near the surface, gβ9.8βm/s2.
This explains why objects weigh less on mountains or in space compared to sea level.
