
GRAVITATION 103
calculations, we can take g to be more or less
constant on or near the earth. But for objects
far from the earth, the acceleration due to
gravitational force of earth is given by
Eq. (9.7).
9.2.1 TO CALCULATE THE VALUE OF
g
To calculate the value of g, we should put the
values of G, M and R in Eq. (9.9), namely,
universal gravitational constant, G = 6.7 × 10
–
11
N m
2
kg
-2
, mass of the earth, M = 6 × 10
24
kg,
and radius of the earth, R = 6.4 × 10
6
m.
= 9.8 m s
–2
.
Thus, the value of acceleration due to gravity
of the earth, g = 9.8 m s
–2
.
9.2.2 MOTION OF OBJECTS UNDER THE
INFLUENCE OF
GRAVITATIONAL
FORCE OF THE EARTH
Let us do an activity to understand whether
all objects hollow or solid, big or small, will
fall from a height at the same rate.
Activity ______________ 9.3
• Take a sheet of paper and a stone.
Drop them simultaneously from the
first floor of a building. Observe
whether both of them reach the
ground simultaneously.
• We see that paper reaches the ground
little later than the stone. This happens
because of air resistance. The air offers
resistance due to friction to the motion
of the falling objects. The resistance
offered by air to the paper is more than
the resistance offered to the stone. If
we do the experiment in a glass jar
from which air has been sucked out,
the paper and the stone would fall at
the same rate.
change in the velocity of falling objects? While
falling, there is no change in the direction of
motion of the objects. But due to the earth’s
attraction, there will be a change in the
magnitude of the velocity. Any change in
velocity involves acceleration. Whenever an
object falls towards the earth, an acceleration
is involved. This acceleration is due to the
earth’s gravitational force. Therefore, this
acceleration is called the acceleration due to
the gravitational force of the earth (or
acceleration due to gravity). It is denoted by
g. The unit of g is the same as that of
acceleration, that is, m s
–2
.
We know from the second law of motion
that force is the product of mass and
acceleration. Let the mass of the stone in
activity 9.2 be m. We already know that there
is acceleration involved in falling objects due
to the gravitational force and is denoted by g.
Therefore the magnitude of the gravitational
force F will be equal to the product of mass
and acceleration due to the gravitational
force, that is,
F = m g (9.6)
From Eqs. (9.4) and (9.6) we have
or
(9.7)
where M is the mass of the earth, and d is the
distance between the object and the earth.
Let an object be on or near the surface of
the earth. The distance d in Eq. (9.7) will be
equal to R, the radius of the earth. Thus, for
objects on or near the surface of the earth,
(9.8)
(9.9)
The earth is not a perfect sphere. As the
radius of the earth increases from the poles to
the equator, the value of g becomes greater at
the poles than at the equator. For most