According to Newton’s second law of motion, if a force F acts on a body of mass ‘m’, it produces an acceleration ‘a’ i.e. F=ma.
If this force is due to gravity of earth, then this acceleration produced is called acceleration due to gravity denoted by ‘g’.
F=mg (equation-1)
The value of g on earth changes throughout the globe as it depends on factors like altitude, depth, radius of earth, etc. We will find out the reason behind this in this article later. We will also learn how to calculate the value of g (acceleration due to gravity value )when height or depth of a body w.r.t the surface of the earth changes. By equation-1 we can define g as the force of gravity acting on a body of mass m placed near or on the surface of the earth (i.e. at a nearby height or depth or on the surface of the earth).
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Since g=F/m, taking m=1 we get- g=F
g is not a universal constant like G. The value of g varies from planet to planet and therefore the weight of the body which is F=mg is different in different planets. However at the surface of the earth value of g is taken to be 9.8m/s2. Hence if a body is freely falling under the influence of earth’s gravity, the acceleration with which it falls is ‘g’.
The value of g is independent of shape, mass or size of a body. It only depends on the mass of earth and radius of earth (or any planet). Thus if 2 bodies of different masses are allowed to fall from the same height h, it reaches the earth’s surface simultaneously. Look at the picture below, Galileo was the first person to do this experiment by dropping 2 spheres of different masses from the top of Leaning Tower of Pisa and established the fact that both of them reached the surface simultaneously.
However if 2 bodies have the same masses but different volumes, they will not reach the earth’s surface at the same time because the larger the volume of the body, the larger is the upthrust from air. Hence the body with larger volume will take more time than the body with lower volume to reach the earth’s surface.
Acceleration due to gravity ‘g’ is a vector quantity and is always directed towards the centre of the earth. If we consider the freely falling body as the origin in Cartesian coordinates, the direction of g is always towards –Y axis. The S.I. unit of g is m/s2 or N/kg. The dimensional formula for g is M0L1T-2.Value of g in fps (feet per second squared) is 32.1741 feet per second squared.
Let us consider earth to be a sphere of mass M, radius R with the centre of earth as O. Now, if a body of mass m is placed on the surface of earth, g is the acceleration due to gravity acting on it.
(Fig-1)
See the above figure, the force on body of mass m due to earth (mass taken to be M) is-
F=GMm/R2 => mg= GMm/R2 =>g=GM/R2 (equation-2)
From the above equation we can see that the value of g doesn’t depend on mass, size, shape of the body but on mass and radius of the earth.
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Now you must be thinking ‘what is the radius of the earth?’ and ‘what is the mass of the earth?’ and how to calculate them.From equation-2 above, we can calculate the mass of the earth. We know that the radius of earth is R=6400km. By equation 2-
M=gR2 /G , where g= 9.8m/s2 and G=6.6710-11Nm2kg-2 - (equation-3)
( unit of gravitation constant in cgs unit is measured in centimeter cube per gram per second square)
Putting the above values, we get M=6.0181024kg
Thus mass of earth in kg is- M=6.0181024kg
Now since we are considering earth to be a spherical body of radius R, then densityρ=MassVolume=M/(43.πR3)=3M/4R3
Then putting equation-3 in equation-2-
ρ=3g4πRG
Putting values of g, G and R, we get- ρ=5.5103kgm-3
Similarly, we can similarly calculate the value of g on mars or value of g on jupiter, if we know the mass and radius of mars and vice versa.
The value of acceleration due to gravity g changes with height, depth and shape of the earth. Let us consider each case and find the formula for g.
a)Effect of altitude(height)- We consider earth to be a sphere of mass M and radius R having centre at O. Let acceleration due to gravity at P (on the surface of earth) be g.
Then, g=GM/R2 (equation-4)
(Fig-2)
If acceleration due to gravity at point Q is taken g’, at a height h above the surface of the earth, then-
g’=GM/(R+h)2 (equation-5)
Dividing equation-4 by equation-5, we get-
g’/g=[GM/(R+h)2]×[ R2/GM]
g’/g=R2/(R+h)2=R2/[R2(1+h/R)2]
g’/g=(1+h/R)2 (equation-6)
If h<<R, then h/R is small enough as compared to 1 so we can neglect its higher powers. So expanding the above equation-6 through binomial distribution, we get-
g’/g=1- 2h/R => g’=g(1- 2h/R) (equation-7)
Thus from the above equation, we can conclude that the value of g decreases with increase in height h above the surface of earth. That’s why the value of g is lesser at mountains as compared to that on flatlands.
b)Effect of depth- We consider earth to be a homogeneous sphere of mass M and radius R with centre at O. Let g be the acceleration due to gravity at the surface of the earth. Then-
g=GM/R2
(Fig-3)
Let acceleration due to gravity at the depth d be g’. If is the uniform density of earth, then- M=(4/3)πR3
Therefore- g= G×[(4/3)πR3]/ R2 =4/3πGR (equation-8)
Now we need to find the value of g at a point below d distance of earth’s surface. So, the distance of that point from the centre of earth is (R-d). Of course this sphere is smaller than earth. Let its mass be M’ while its density will be the same as we have taken earth to be a homogeneous sphere.
Therefore, g’=GM’/(R-d)2 where M’=4/3(R-d)3 (equation-9)
Now, dividing equation-9 by equation-8, we get-
g’/g=(R-d)/R=1-d/R =>g’=g(1-d/R) (equation-10)
Thus, from the above equation we conclude that acceleration due to gravity decreases with depth.
From (equation-10) we can find the value of g at the centre of the earth. That is-
At centre R=d, then g’=1-R/R=0
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c)Effect of shape of earth- In both the above cases we have taken earth to be a sphere but in reality it is not a perfect sphere. Its shape is an Oblate spheroid. It bulges out at the equator and flattens at the poles.(Fig-5)
Hence, the equatorial radius ‘a’ is about 21km larger than the polar radius ‘b’.
Since, g=GM/R2 => g is proportional to 1/R2 as G and M are constants.
And a>b, therefore the value of g is least at equator and keeps increasing towards poles and becomes maximum at poles.
The value of g also varies with rotation of g about its own axis. However we will not cover the derivation in this article.
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NCERT Physics Notes:
Decrease in value of g is- g-g’=2hg/R.
Thus fractional decrease in value of g is (g-g’)/g=2h/R
Then, percentage decrease in value of g= [(g-g’)/g]×100=[2h/R]×100
If gravity suddenly disappears,
all the bodies will be suddenly thrown away from the surface due to earth’s centrifugal
force.
Motion of the satellites around earth, both natural and artificial will not be possible as no centripetal force will be provided.
All the materials will lose their weights, etc.
Ability of a celestial body to hold its atmosphere depends on 2 factors mainly- acceleration due to gravity i.e. value of g and its surface temperature.
1.625meter per second squared.
Using equation-2 and putting values of the sun's mass and radius, the value of g on the sun
is found to be 274.13 meter per second squared.
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