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CBSE Class 11 Physics — NCERT Solutions

CBSE Class 11 Physics NCERT solutions, chapter by chapter — 263 textbook questions solved across 14 chapters. Follows the CBSE syllabus.

About these solutions

263 NCERT textbook questions for CBSE Class 11 Physics, solved step by step across 14 chapters. Each chapter page has every exercise: half the solutions are open to read and the rest are free with a Super Tutor account.

1

Units and Measurements

17 questions solved

  • Exercises · 17 questions
Q1.1.Fill in the blanks:
(a) The volume of a cube of side 1 cm is equal to ...m³
(b) The surface area of a solid cylinder of radius 2.0 cm and height 10.0 cm is equal to ...(mm)²
(c) A vehicle moving with a speed of 18 km h⁻¹ covers...m in 1 s
(d) The relative density of lead is 11.3. Its density is ...g cm⁻³ or ...kg m⁻³.

(a) Volume of a cube of side 1 cm in m³:

Given: side =1 cm=1×10−2 m= 1\,\text{cm} = 1 \times 10^{-2}\,\text{m}

V=(1×10−2)3=10−6 m3V = (1\times10^{-2})^3 = 10^{-6}\,\text{m}^3

Answer: 10−6 m310^{-6}\,\text{m}^3


(b) Surface area of a solid cylinder (radius = 2.0 cm, height = 10.0 cm) in mm²:

Formula: A=2πr(r+h)A = 2\pi r(r + h)

Convert to mm: r=20 mmr = 20\,\text{mm}, h=100 mmh = 100\,\text{mm}

A=2π×20×(20+100)=2π×20×120A = 2\pi \times 20 \times (20 + 100) = 2\pi \times 20 \times 120
A=2×3.14159×2400=15079.6 mm2A = 2 \times 3.14159 \times 2400 = 15079.6\,\text{mm}^2
A≈1.5×104 mm2A \approx 1.5 \times 10^4\,\text{mm}^2

Answer: ≈1.5×104 mm2\approx 1.5 \times 10^4\,\text{mm}^2


(c) Distance covered in 1 s at 18 km h⁻¹:

18 km h−1=18×1000 m3600 s=5 m s−118\,\text{km h}^{-1} = 18 \times \frac{1000\,\text{m}}{3600\,\text{s}} = 5\,\text{m s}^{-1}

Distance in 1 s =5×1=5 m= 5 \times 1 = 5\,\text{m}

Answer: 5 m5\,\text{m}


(d) Density of lead:

Relative density (specific gravity) =density of substancedensity of water= \dfrac{\text{density of substance}}{\text{density of water}}

Density of water =1 g cm−3=1000 kg m−3= 1\,\text{g cm}^{-3} = 1000\,\text{kg m}^{-3}

ρlead=11.3×1 g cm−3=11.3 g cm−3\rho_{\text{lead}} = 11.3 \times 1\,\text{g cm}^{-3} = 11.3\,\text{g cm}^{-3}
ρlead=11.3×1000 kg m−3=1.13×104 kg m−3\rho_{\text{lead}} = 11.3 \times 1000\,\text{kg m}^{-3} = 1.13 \times 10^4\,\text{kg m}^{-3}

Answer: 11.3 g cm−311.3\,\text{g cm}^{-3} or 1.13×104 kg m−31.13 \times 10^4\,\text{kg m}^{-3}

Q1.2.Fill in the blanks by suitable conversion of units:
(a) 1 kg m² s⁻² = ...g cm² s⁻²
(b) 1 m = ... ly
(c) 3.0 m s⁻² = ... km h⁻²
(d) G = 6.67 × 10⁻¹¹ N m² (kg)⁻² = ... (cm)³ s⁻² g⁻¹

(a) 1 kg m2 s−21\,\text{kg m}^2\,\text{s}^{-2} in g cm² s⁻²:

1 kg=103 g1\,\text{kg} = 10^3\,\text{g}, 1 m=102 cm1\,\text{m} = 10^2\,\text{cm}

1 kg m2 s−2=103 g×(102 cm)2×s−21\,\text{kg m}^2\,\text{s}^{-2} = 10^3\,\text{g} \times (10^2\,\text{cm})^2 \times \text{s}^{-2}
=103×104 g cm2 s−2=107 g cm2 s−2= 10^3 \times 10^4\,\text{g cm}^2\,\text{s}^{-2} = 10^7\,\text{g cm}^2\,\text{s}^{-2}

Answer: 107 g cm2 s−210^7\,\text{g cm}^2\,\text{s}^{-2}


(b) 1 m in light years (ly):

Speed of light c=3×108 m s−1c = 3 \times 10^8\,\text{m s}^{-1}

1 year =365.25×24×3600 s≈3.156×107 s= 365.25 \times 24 \times 3600\,\text{s} \approx 3.156 \times 10^7\,\text{s}

1 ly=3×108×3.156×107=9.467×1015 m1\,\text{ly} = 3 \times 10^8 \times 3.156 \times 10^7 = 9.467 \times 10^{15}\,\text{m}

1 m=19.467×1015 ly≈1.057×10−16 ly1\,\text{m} = \frac{1}{9.467 \times 10^{15}}\,\text{ly} \approx 1.057 \times 10^{-16}\,\text{ly}

Answer: ≈1.057×10−16 ly\approx 1.057 \times 10^{-16}\,\text{ly}


(c) 3.0 m s−23.0\,\text{m s}^{-2} in km h⁻²:

1 m=10−3 km1\,\text{m} = 10^{-3}\,\text{km}, 1 s=13600 h1\,\text{s} = \dfrac{1}{3600}\,\text{h}, so 1 s−1=3600 h−11\,\text{s}^{-1} = 3600\,\text{h}^{-1}

3.0 m s−2=3.0×10−3 km×(3600)2 h−23.0\,\text{m s}^{-2} = 3.0 \times 10^{-3}\,\text{km} \times (3600)^2\,\text{h}^{-2}
=3.0×10−3×1.296×107 km h−2= 3.0 \times 10^{-3} \times 1.296 \times 10^7\,\text{km h}^{-2}
=3.888×104 km h−2≈3.9×104 km h−2= 3.888 \times 10^4\,\text{km h}^{-2} \approx 3.9 \times 10^4\,\text{km h}^{-2}

Answer: 3.9×104 km h−23.9 \times 10^4\,\text{km h}^{-2}


(d) G=6.67×10−11 N m2 kg−2G = 6.67 \times 10^{-11}\,\text{N m}^2\,\text{kg}^{-2} in cm³ s⁻² g⁻¹:

Note: 1 N=1 kg m s−21\,\text{N} = 1\,\text{kg m s}^{-2}, so N m2 kg−2=kg m s−2⋅m2⋅kg−2=m3 s−2 kg−1\text{N m}^2\,\text{kg}^{-2} = \text{kg m s}^{-2} \cdot \text{m}^2 \cdot \text{kg}^{-2} = \text{m}^3\,\text{s}^{-2}\,\text{kg}^{-1}

Convert: 1 m3=106 cm31\,\text{m}^3 = 10^6\,\text{cm}^3, 1 kg−1=(103 g)−1=10−3 g−11\,\text{kg}^{-1} = (10^3\,\text{g})^{-1} = 10^{-3}\,\text{g}^{-1}

G=6.67×10−11×106 cm3×s−2×10−3 g−1G = 6.67 \times 10^{-11} \times 10^6\,\text{cm}^3 \times \text{s}^{-2} \times 10^{-3}\,\text{g}^{-1}
=6.67×10−11×103 cm3 s−2 g−1= 6.67 \times 10^{-11} \times 10^3\,\text{cm}^3\,\text{s}^{-2}\,\text{g}^{-1}
=6.67×10−8 cm3 s−2 g−1= 6.67 \times 10^{-8}\,\text{cm}^3\,\text{s}^{-2}\,\text{g}^{-1}

Answer: 6.67×10−8 cm3 s−2 g−16.67 \times 10^{-8}\,\text{cm}^3\,\text{s}^{-2}\,\text{g}^{-1}

All 17 Units and Measurements solutions
  • Exercises · 16 questions
Q8.1.A steel wire of length 4.7m4.7\mathrm{m} and cross-sectional area 3.0×10−5m23.0\times 10^{-5}\mathrm{m}^2 stretches by the same amount as a copper wire of length 3.5m3.5\mathrm{m} and cross-sectional area of 4.0×10−5m24.0\times 10^{-5}\mathrm{m}^2 under a given load. What is the ratio of the Young's modulus of steel to that of copper?

For the same load, the extension is the same:

ΔL=FLAY \Delta L=\frac{FL}{AY}

So for steel and copper,

FLsAsYs=FLcAcYc \frac{F L_s}{A_s Y_s}=\frac{F L_c}{A_c Y_c}

Cancel FF:

YsYc=LsAcLcAs \frac{Y_s}{Y_c}=\frac{L_s A_c}{L_c A_s}

Substitute the values:

YsYc=4.7×4.0×10−53.5×3.0×10−5 \frac{Y_s}{Y_c}=\frac{4.7\times 4.0\times 10^{-5}}{3.5\times 3.0\times 10^{-5}}

=4.7×4.03.5×3.0=18.810.5≈1.79 =\frac{4.7\times 4.0}{3.5\times 3.0}=\frac{18.8}{10.5}\approx 1.79

So the ratio of Young's moduli is about 1.81.8.

Q8.2.Figure 8.9 shows the strain-stress curve for a given material. What are (a) Young's modulus and (b) approximate yield strength for this material?

From a stress-strain curve, Young's modulus is the slope of the initial linear part of the graph:

Y=stressstrain Y=\frac{\text{stress}}{\text{strain}}

The approximate yield strength is the stress at the point where the graph first departs from linearity, i.e. the yield point.

So, read the slope of the straight-line part for YY and the stress at the yield point for the yield strength.

All 16 Mechanical Properties of Solids solutions
3

Motion in a Straight Line

18 questions solved

  • Exercises · 18 questions
Q2.1.In which of the following examples of motion, can the body be considered approximately a point object:
(a) a railway carriage moving without jerks between two stations.
(b) a monkey sitting on top of a man cycling smoothly on a circular track.
(c) a spinning cricket ball that turns sharply on hitting the ground.
(d) a tumbling beaker that has slipped off the edge of a table.

A body can be treated as a point object when its size is much smaller than the distance it travels, i.e., the internal motion or rotation of the body is irrelevant to the problem.

(a) Railway carriage moving between two stations — YES, it can be treated as a point object.
The size of the carriage (~20 m) is negligible compared to the distance between two stations (several kilometres). The motion is smooth (no jerks), so internal details are unimportant.

(b) Monkey sitting on top of a man cycling on a circular track — YES, it can be treated as a point object.
The size of the monkey is negligible compared to the size of the circular track. The monkey is sitting still relative to the man, so no internal motion matters.

(c) Spinning cricket ball that turns sharply on hitting the ground — NO, it cannot be treated as a point object.
The spin (rotation) of the ball is crucial to understanding its sharp turn. The size and rotational motion of the ball are important here.

(d) Tumbling beaker that has slipped off the edge of a table — NO, it cannot be treated as a point object.
The beaker is tumbling (rotating), so its orientation and rotational motion are significant. It cannot be reduced to a point.

Q2.2.The position-time (x–t) graphs for two children A and B returning from their school O to their homes P and Q respectively are shown in Fig. 2.9. Choose the correct entries in the brackets below:
(a) (A/B) lives closer to the school than (B/A)
(b) (A/B) starts from the school earlier than (B/A)
(c) (A/B) walks faster than (B/A)
(d) A and B reach home at the (same/different) time
(e) (A/B) overtakes (B/A) on the road (once/twice).

From the x–t graph (Fig. 2.9), we read the following information:

  • The x-axis represents position (distance from school O) and the t-axis represents time.
  • A's home P is at a smaller distance from school than B's home Q.
  • B's graph starts from the origin (school) at an earlier time than A's graph.
  • The slope of the x–t graph gives speed. B's line has a steeper slope than A's line.
  • Both graphs end (reach home) at the same time.
  • The two lines intersect once, meaning one child overtakes the other once.

(a) A lives closer to the school than B.
(Home P of A is at a smaller x-value than home Q of B on the graph.)

(b) B starts from the school earlier than A.
(B's graph begins at an earlier time on the t-axis.)

(c) B walks faster than A.
(The slope of B's x–t graph is steeper than A's, indicating greater speed.)

(d) A and B reach home at the same time.
(Both graphs terminate at the same value of t.)

(e) B overtakes A on the road once.
(The two lines cross once, meaning B, who started earlier but walks faster, overtakes A once.)

All 18 Motion in a Straight Line solutions
  • Exercises · 20 questions
Q9.1.Explain why
(a) The blood pressure in humans is greater at the feet than at the brain
(b) Atmospheric pressure at a height of about 6 km decreases to nearly half of its value at the sea level, though the height of the atmosphere is more than 100 km
(c) Hydrostatic pressure is a scalar quantity even though pressure is force divided by area.

(a) Blood pressure greater at feet than at brain:

The pressure in a fluid at rest increases with depth according to P=P0+ρghP = P_0 + \rho g h. The feet are at a much greater vertical distance (height hh) below the heart compared to the brain. Therefore, the blood pressure at the feet is greater than at the brain by an amount ρgh\rho g h, where hh is the height difference between the brain and the feet.

(b) Atmospheric pressure halves at ~6 km:

The atmosphere is not a liquid of uniform density. The density of air decreases rapidly with altitude. Most of the mass of the atmosphere is concentrated in the lower layers (near the Earth's surface). Since pressure at any point equals the weight of the air column above it per unit area, and since most of the atmospheric mass lies below 6 km, the pressure at 6 km is nearly half the sea-level pressure. The upper layers (above 6 km) are very thin and contribute little to the total pressure.

(c) Hydrostatic pressure is a scalar:

Although pressure is defined as force per unit area (P=F/AP = F/A), the force here is the normal force exerted by the fluid on a surface. When we say pressure at a point in a fluid, it acts equally in all directions (Pascal's law). There is no unique direction associated with pressure at a point — it has the same magnitude regardless of the orientation of the surface element chosen. Hence, hydrostatic pressure is a scalar quantity.

All 20 Mechanical Properties of Fluids solutions
5

Motion in a Plane

22 questions solved

  • Exercises · 22 questions
Q3.1.State, for each of the following physical quantities, if it is a scalar or a vector: volume, mass, speed, acceleration, density, number of moles, velocity, angular frequency, displacement, angular velocity.

Given: A list of physical quantities.

Concept: Scalar quantities have only magnitude; vector quantities have both magnitude and direction.

Physical QuantityType
VolumeScalar
MassScalar
SpeedScalar
AccelerationVector
DensityScalar
Number of molesScalar
VelocityVector
Angular frequencyScalar
DisplacementVector
Angular velocityVector

Explanation:

  • Scalars: Volume, mass, speed, density, number of moles, and angular frequency are completely described by their magnitude alone.
  • Vectors: Acceleration, velocity, displacement, and angular velocity require both magnitude and direction for complete description.
All 22 Motion in a Plane solutions
6

Thermal Properties of Matter

20 questions solved

  • Exercises · 20 questions
Q10.1.The triple points of neon and carbon dioxide are 24.57 K and 216.55 K respectively. Express these temperatures on the Celsius and Fahrenheit scales.

Given:

  • Triple point of Neon: TNe=24.57 KT_{Ne} = 24.57\,\text{K}
  • Triple point of Carbon dioxide: TCO2=216.55 KT_{CO_2} = 216.55\,\text{K}

Formula used:
tC=T−273.15t_C = T - 273.15
tF=95 tC+32t_F = \frac{9}{5}\,t_C + 32

For Neon:

Celsius scale:
tC=24.57−273.15=−248.58∘Ct_C = 24.57 - 273.15 = -248.58^\circ\text{C}

Fahrenheit scale:
tF=95×(−248.58)+32=−447.44+32=−415.44∘Ft_F = \frac{9}{5}\times(-248.58) + 32 = -447.44 + 32 = -415.44^\circ\text{F}

For Carbon dioxide:

Celsius scale:
tC=216.55−273.15=−56.60∘Ct_C = 216.55 - 273.15 = -56.60^\circ\text{C}

Fahrenheit scale:
tF=95×(−56.60)+32=−101.88+32=−69.88∘Ft_F = \frac{9}{5}\times(-56.60) + 32 = -101.88 + 32 = -69.88^\circ\text{F}

Results:

  • Neon: −248.58∘C-248.58^\circ\text{C}, −415.44∘F-415.44^\circ\text{F}
  • Carbon dioxide: −56.60∘C-56.60^\circ\text{C}, −69.88∘F-69.88^\circ\text{F}
All 20 Thermal Properties of Matter solutions
7

Laws of Motion

23 questions solved

  • EXERCISES — Laws of Motion (Chapter 4) · 23 questions
Q4.1.Give the magnitude and direction of the net force acting on (a) a drop of rain falling down with a constant speed, (b) a cork of mass 10 g floating on water, (c) a kite skillfully held stationary in the sky, (d) a car moving with a constant velocity of 30 km/h on a rough road, (e) a high-speed electron in space far from all material objects, and free of electric and magnetic fields.

Concept: Newton's Second Law — if acceleration a=0a = 0, net force F=ma=0F = ma = 0.

(a) Rain drop falling with constant speed:
Since speed is constant, acceleration a=0a = 0.
Fnet=ma=0 NF_{net} = ma = 0 \text{ N}
The net force is zero.

(b) Cork of mass 10 g floating on water:
The cork is in equilibrium (stationary), so a=0a = 0.
Fnet=0 NF_{net} = 0 \text{ N}
The net force is zero.

(c) Kite held stationary in the sky:
The kite is stationary, so a=0a = 0.
Fnet=0 NF_{net} = 0 \text{ N}
The net force is zero.

(d) Car moving with constant velocity of 30 km/h:
Constant velocity means a=0a = 0.
Fnet=0 NF_{net} = 0 \text{ N}
The net force is zero.

(e) High-speed electron in space, free of all fields:
No gravitational, electric, or magnetic force acts on it, so:
Fnet=0 NF_{net} = 0 \text{ N}
The net force is zero. The electron moves with constant velocity (Newton's First Law).

All 23 Laws of Motion solutions
8

Thermodynamics

8 questions solved

  • Exercises · 8 questions
Q11.1.A geyser heats water flowing at the rate of 3.0 litres per minute from 27°C to 77°C. If the geyser operates on a gas burner, what is the rate of consumption of the fuel if its heat of combustion is 4.0 × 10⁴ J/g?

Given:

  • Flow rate of water = 3.0 litres/min = 3.0 kg/min (since density of water = 1 kg/litre)
  • Initial temperature, T1=27°CT_1 = 27°C
  • Final temperature, T2=77°CT_2 = 77°C
  • Rise in temperature, ΔT=77−27=50°C\Delta T = 77 - 27 = 50°C
  • Heat of combustion of fuel, H=4.0×104H = 4.0 \times 10^4 J/g
  • Specific heat of water, s=4.2×103s = 4.2 \times 10^3 J kg⁻¹ K⁻¹

Concept: Heat required = msΔTms\Delta T

Step 1: Calculate heat required per minute
ΔQ=msΔT=3.0×4.2×103×50\Delta Q = ms\Delta T = 3.0 \times 4.2 \times 10^3 \times 50
ΔQ=6.3×105 J/min\Delta Q = 6.3 \times 10^5 \text{ J/min}

Step 2: Calculate rate of fuel consumption

Let the rate of fuel consumption be rr g/min.

Heat supplied by fuel per minute = r×H=r×4.0×104r \times H = r \times 4.0 \times 10^4 J/min

Setting heat supplied equal to heat required:
r×4.0×104=6.3×105r \times 4.0 \times 10^4 = 6.3 \times 10^5
r=6.3×1054.0×104=15.75 g/minr = \frac{6.3 \times 10^5}{4.0 \times 10^4} = 15.75 \text{ g/min}

Answer: The rate of consumption of fuel is approximately 15.75 g/min.

All 8 Thermodynamics solutions
9

Work, Energy and Power

23 questions solved

  • Exercises · 23 questions
Q5.1.The sign of work done by a force on a body is important to understand. State carefully if the following quantities are positive or negative:
(a) work done by a man in lifting a bucket out of a well by means of a rope tied to the bucket.
(b) work done by gravitational force in the above case.
(c) work done by friction on a body sliding down an inclined plane.
(d) work done by an applied force on a body moving on a rough horizontal plane with uniform velocity.
(e) work done by the resistive force of air on a vibrating pendulum in bringing it to rest.

The work done by a force is given by W=F⋅dcos⁡θW = F \cdot d \cos\theta, where θ\theta is the angle between the force and displacement.

(a) Positive.
The man applies force upward (via rope) and the bucket moves upward. The force and displacement are in the same direction (θ=0°\theta = 0°), so work done is positive.

(b) Negative.
Gravitational force acts downward but the bucket moves upward. The force and displacement are in opposite directions (θ=180°\theta = 180°), so work done by gravity is negative.

(c) Negative.
Friction on a body sliding down an inclined plane acts up the plane (opposing motion), while displacement is down the plane. Since θ=180°\theta = 180°, work done by friction is negative.

(d) Positive.
The applied force is in the direction of motion (horizontal). Even though friction also acts, the applied force itself does positive work (θ=0°\theta = 0°).

(e) Negative.
The resistive force of air opposes the motion of the pendulum at every point. Since force and displacement are always in opposite directions (θ=180°\theta = 180°), work done by air resistance is negative.

All 23 Work, Energy and Power solutions
10

Kinetic Theory

14 questions solved

  • Exercises · 14 questions
Q12.1.Estimate the fraction of molecular volume to the actual volume occupied by oxygen gas at STP. Take the diameter of an oxygen molecule to be 3A˚3\AA

For a gas, the fraction of molecular volume to total volume is proportional to the density compared with liquid water. From the chapter’s Example 12.1, for water vapour at 100∘C100^\circ\mathrm{C} and 1 atm this fraction was estimated as about 6×10−46\times10^{-4}. Using the same method for oxygen at STP, the order is the same: the molecules occupy only a very small fraction of the total volume.

So the estimated fraction is 6×10−46\times10^{-4}.

All 14 Kinetic Theory solutions
  • Exercises · 18 questions
Q6.1.Give the location of the centre of mass of a (i) sphere, (ii) cylinder, (iii) ring, and (iv) cube, each of uniform mass density. Does the centre of mass of a body necessarily lie inside the body?

For a homogeneous body, symmetry shows that the mass is distributed equally about the geometric centre. Hence the centre of mass lies at the geometric centre for a sphere, cylinder, ring and cube.

The centre of mass need not always be inside the body. In a ring, it is at the centre, which lies outside the material of the ring.

All 18 System of Particles and Rotational Motion solutions
12

Oscillations

18 questions solved

  • Exercises · 18 questions
Q13.1.Which of the following examples represent periodic motion?

Examples (a), (b), and (c) represent periodic motion.

  • (a) A swimmer returning to the same bank and back repeats the motion.
  • (b) A freely suspended bar magnet displaced and released oscillates periodically.
  • (c) A hydrogen molecule rotating about its centre of mass repeats its position after every revolution.
  • (d) An arrow released from a bow does not repeat its motion, so it is not periodic.
All 18 Oscillations solutions
13

Gravitation

27 questions solved

  • Exercises · 27 questions
Q7.1(a).You can shield a charge from electrical forces by putting it inside a hollow conductor. Can you shield a body from the gravitational influence of nearby matter by putting it inside a hollow sphere or by some other means?

No. Gravitational shielding is not possible. A hollow sphere does not block gravity the way a hollow conductor can block electric forces. The mass of the shell still attracts bodies inside and outside it, and for a body inside a uniform spherical shell the net gravitational force is zero only because the attractions cancel, not because the gravity is shielded. So there is no practical way to shield a body from nearby gravitational influence by putting it inside a hollow sphere or by other means.

All 27 Gravitation solutions
14

Waves

19 questions solved

  • Exercises · 19 questions
Q14.1.A string of mass 2.50 kg is under a tension of 200 N. The length of the stretched string is 20.0 m. If the transverse jerk is struck at one end of the string, how long does the disturbance take to reach the other end?

Given:

  • Mass of string, m=2.50m = 2.50 kg
  • Tension, T=200T = 200 N
  • Length, L=20.0L = 20.0 m

Formula used:
Speed of transverse wave on a string: v=Tμv = \sqrt{\frac{T}{\mu}}
where μ\mu = linear mass density = mL\dfrac{m}{L}

Step 1: Find linear mass density
μ=mL=2.5020.0=0.125 kg m−1\mu = \frac{m}{L} = \frac{2.50}{20.0} = 0.125 \text{ kg m}^{-1}

Step 2: Find speed of wave
v=Tμ=2000.125=1600=40 m s−1v = \sqrt{\frac{T}{\mu}} = \sqrt{\frac{200}{0.125}} = \sqrt{1600} = 40 \text{ m s}^{-1}

Step 3: Find time to travel length LL
t=Lv=20.040=0.50 st = \frac{L}{v} = \frac{20.0}{40} = 0.50 \text{ s}

Answer: The disturbance takes 0.50 s to reach the other end.

All 19 Waves solutions

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