Class 11-science H C VERMA Solutions Physics Chapter 11 - Gravitation
Gravitation Exercise 225
Solution 1
F=
F = Gravitational force between two bodies
G = Gravitational constant
m1, m2 = Masses of the two bodies
r = Distance between the bodies
Here, m1=m2=10 kg
G=6.67×10-11
F =
F = 6.67×10-7N
Solution 2
= (2)=2k
Here and are on the same straight line.
Thus, Resultant force= -[ because >]
= 6K - 2k = 4K
and are on the same straight line.
Resultant force= - [because >]
= 8K - 4k = 4K
Total resultant force =
Here cos𝜃 = 0 because 𝜃 = 90°
=
Resultant force on 'm' is= 4
Gravitation Exercise 226
Solution 3
Mass 'm' is at mid-point of side PR.
(a) OP = OR = a/2
= K=
= = 4K
= = 4K
Altitude OQ =
= = = K
Here, FOP and FOR are equal in magnitude and opposite in direction.
So, FOP + FOR = 0
Total resultant force(F)
= + +
= 0 +
= K
= (Along OQ)
(b) If particle at centroid, All forces 'F' are equal in magnitude.
F= FGP = FGQ = FGR =
Resultant of FGQ and FGR
FR =
=
FR =F
The resultant is 0, because they have equal magnitude and are in opposite direction.
Solution 4
Let us assume that the center of mass of spheres are located at point P, Q and R. So, re-drawing the figure, it is an equilateral triangle.
Force on mass M at point P
FPR = FPQ = = k (let)
Resultant
FR =
FR =
FR=
FR =
Solution 5
Here,
Now, force on particle 1
Due to particle 4:
Due to particle 2:
Due to particle 1:
Resultant of
(along direction)
Net resultant force,
Since particle is revolving in a circle. So, this is centripetal force.
Solution 6
The acceleration due to gravity at a point at height 'h' from the surface of moon of radius R is
g =
=
= 0.65 m/s2
Solution 7
Initially,
Finally,
If both bodies are taken as system.
Now, applying law of conservation of energy,
On solving,
m/s
and
m/s
Solution 8
Consider two small elements at an angle 𝜃 from horizontal length of the element =Rd𝜃
Mass of each element dm = (Rd𝜃)
Force by elemental mass on particle
dF =
dF =
dF =
Resultant of the both elemental forces = 2dFsinθ
Net Force
FN =
= sinθ
=
=
FN = ( because
Solution 9
Consider two small elements of length dx at a distance x from center on both sides of center.
Mass of each element, dm = dx
Field due to each element at point P
=
dE =
Resultant of the elemental field= 2dE cosθ
Net electric force =
=
=
On integrating,
EN =
Solution 10
Here,
The gravitational force of mass m due to shell of is zero as gravitational field inside shell is zero.
Gravitational field due to shell of mass outside the shell at mass m=
So, force
Solution 11
Method 1:
The gravitational field inside a sphere of radius R at a distance x from center is
So, force on particle of mass m is
Method 2:
Acceleration due to gravity at depth d from surface
Here,
So, force on particle of mass m is= mg
Solution 12
Distance of the particle from earth's center
Force on the particle=massgravitational field intensity
Force exerted by wall on particle=Force exerted by particle on wall
Solution 13
(a)
Gravitational field intensity inside shell is zero. So, force by shell on mass is zero.
Now, for solid sphere.
Gravitational field inside sphere at a distance (x-r) from center is
So, force by sphere on mass is
Net force
(b)
Gravitational field intensity inside shell is zero. So, force by shell on mass is zero.
Now, for solid sphere.
Gravitational field intensity outside sphere at distance (x-r) is given by
So, force by sphere on mass is
Net force
(c)
Force=massGravitational field intensity
Force by shell= (towards center)
Force by sphere= (towards center)
Solution 14
(a) At point
Net gravitational field=field due to shell+ field due to sphere
(b) At point
Net gravitational field=field due to shell+ field due to sphere
Solution 15
Resultant field inside any spherical shell is zero at all points. So, at point a and B, field is zero. The field due to upper part and lower part and are equal and opposite.
Solution 16
Let mass 0.5kg is placed at distance x from 2kg between both masses.
Since, particle is in equilibrium.
Force due to 2kg= Force due to 4kg
On solving,
x=0.83m
Now, gravitational potential energy
J
Solution 17
Work done
=ΔU = final P.E - initial P.E
=Uf -Ui
=3() - 3()
=()
Solution 18
Work done against gravitational force = change in potential energy
J
Solution 19
(a) Force,
N
(b)
at (0,0), potential =0
C=0
So, V=-5x-12y
At point (12,0)
At point (0,5)
(c) Potential at (12,5)
and potential at (0, 0) is 0.
So, change in gravitational potential energy
(d)
Gravitation Exercise 227
Solution 20
Dimension of L.H.S =[V]
Dimension of RHS=
Hence, dimensionally correct.
(b)
(c)
Solution 21
Gravitational field in the region is given by
E = 2 î + 3
Slope of gravitational field, m1 = tanθ1 = 3/2
The line 3 y + 2 x = 5 can be written with the slope, m2 = 2 = -2/3
m1 × m2 = -1
Thus, m1, m2 lines are perpendicular.
So, no work is done in by gravitational force when a particle is moved on the given line.
Solution 22
Let height be h
=
2=
h = (-1)R
Solution 23
g'=g (1- )
g' be the acceleration due to gravity at Mount Everest
h=8848
g'=9.8×(1- )
= 9.77 m/s2
Solution 24
g'= g(1- )
g' be the acceleration due to gravity at surface
= 9.8×(1- )
=9.79 m/s2
Solution 25
Let gp be the gravity at the poles ,ge be the gravity at the equator
ge= gp - ω2R
=9.81 -
= 9.766 N/m2
Now, mge = 1kg × 9.766 N/m2
=9.766 N
Thus the body weighs 9.766 N at the equator.
Solution 26
At equator, let stretch in spring be x
Spring force=
-(1)
Now, at height h above surface, stretch in spring is x
Spring force=
-(2)
From (1) and (2)
Km
Solution 27
Apparent acceleration due to gravity at equator becomes 0.
G'=g - ω2R = 0
g = ω2R
ω=
=
= 1.2rad/s
Time period = T = = = 1.41 hrs
Solution 28
(a) Since, ship is at rest with respect to water.
So, Angular speed of ship=Angular speed of earth
(b) The tension in string is given by
(c) If ship sails at speed v, then tension
[Here R>>>V ]
Solution 29
Kepler's law of planetary motion says ,
T2 ∝ R3
=
= = 1.52
Solution 30
Time period of the moon around the earth is given by,
T =2π
m = mass of earth
r = Distance between center of the moon and earth
27.3 × 86400= 2×3.14
M = kg
Solution 31
Time period of revolution of satellite around the mars is given by
T =2π
M = Mars mass
r = Distance of the satellite from center of the planet
27540 = 2×3.14
M = 6.5 × 1023kgs
Solution 32
(a) Speed of satellite in its orbit
V0=
V0= = 6.9 km/sec
(b) Kinetic energy of satellite = (½)×1000×
= 2.38×
(c) Potential energy of satellite = P.E =
=
= -4.76 J
(d) Time period of the satellite
T=7645.2 sec
=2.1 hrs
Solution 33
(a) Since, angular speed of satellite is equal to angular speed of earth.
So, time period of satellite=24hrs
T=24hrs
h=42300 Km
(b) Time taken from North pole to equatorial plane
hrs
Solution 34
Weight at North pole = 10 N
W = mg
10 = mg
Weight of body in a satellite at height 'h' is
WS =mg'
= m [g (]
For a geo-stationary satellite, R = 6.4×103 km
h = 3.6 ×103 km
N
Solution 35
Time period of the revolution of the satellite around a planet in terms of the radius of the orbit of the satellite is given by:
T =2π
T2 =4 π2 (
g =
Where 'g' is acceleration due to gravity.
Solution 36
Consider that 'B' is the position of the geo- stationary satellite.
Here R= 6400 kms ( Radius of earth)
d = altitude
θ = colatitude of the plane which can directly receive a signal from the satellite.
Take ∆OAB,
cos 𝜙 = =
𝜙 =
= (0.15)
Now θ + 𝜙 =
θ = -
θ =
Solution 37
Upon Earth's surface, its total energy is
E = K.E +P.E
= mv2 +(- (1)
In space at maximum height , its K.E =0 and P.E =-
Es = 0+ (2)
Total energy must be conserved , therefore (1) = (2)
mv2 +(- =
Here h= R, so
mv2 = (
mv2 =
V=
=
= 7.9 km/s
Solution 38
Velocity of particle on the Earth surface = Ve = 15 km/s
Let Vs be the particle velocity in space.
Total Energy must be conserved.
Change in K.E. = Change in P.E.
∆K.E.=∆P.E.
m() =
[(225) - ] =
On solving
Vs = 10 km/s
Solution 39
Escape velocity = Ve =
Mass = 6× 1024 kgs.
Ve = 3×108 m/s.
i.e., 3×108=
On solving,
R = 8.89×10-3
=9×10-3
= 9mm.