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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=mass gravitational 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=mass Gravitational 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=   

=  

= 1.2 rad/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. 

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