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NCERT Solutions for Class 11 Physics

Chapter 1: Units and Measurements

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Complete NCERT Solution PDF for Chapter 1: Units and Measurements

NCERT Solutions For Class 11 Physics Chapter 1 Units and Measurements helps students understand the fundamental concepts required for accurate measurement in Physics. The page provides detailed NCERT Solutions that explain physical quantities, SI units, dimensions, measurement errors, and significant figures with clear examples. NCERT Solutions For Class 11 Physics make it easier for students to learn the importance of standard units and apply dimensional analysis in solving problems. This chapter builds the foundation for numerical problem-solving and scientific calculations throughout Physics. The solutions provide step-by-step explanations for textbook questions and help students strengthen their conceptual understanding. Students can access the chapter PDF for revision, practice, and exam preparation. The detailed approach helps learners develop accuracy and confidence in handling measurements.

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Examples 1.1-1.5

Example 1.1 Each side of a cube is measured to be $$7.203 \, \mathrm{m}$$. What are the total surface area and the volume of the cube to appropriate significant figures?

Solution

The side of the cube is given to four significant figures, so both derived quantities must be reported to four significant figures.

Total surface area of the cube (six identical square faces of side $$a = 7.203 \, \mathrm{m}$$):

$$S = 6a^2 = 6 \times (7.203)^2 \, \mathrm{m^2}$$

$$S = 6 \times 51.883209 \, \mathrm{m^2} = 311.299254 \, \mathrm{m^2}$$

Rounding to four significant figures, $$S = 311.3 \, \mathrm{m^2}$$.

Volume of the cube:

$$V = a^3 = (7.203)^3 \, \mathrm{m^3} = 373.714754 \, \mathrm{m^3}$$

Rounding to four significant figures, $$V = 373.7 \, \mathrm{m^3}$$.

Answer

Surface area $$= 311.3 \, \mathrm{m^2}$$; Volume $$= 373.7 \, \mathrm{m^3}$$.

Example 1.2 $$5.74 \, \mathrm{g}$$ of a substance occupies $$1.2 \, \mathrm{cm^3}$$. Express its density by keeping the significant figures in view.

Solution

The density is defined as mass per unit volume.

$$\rho = \dfrac{m}{V} = \dfrac{5.74 \, \mathrm{g}}{1.2 \, \mathrm{cm^3}} = 4.7833\ldots \, \mathrm{g \, cm^{-3}}$$

For multiplication or division, the result must be expressed to the same number of significant figures as the factor with the fewest. Mass $$5.74 \, \mathrm{g}$$ has $$3$$ significant figures and volume $$1.2 \, \mathrm{cm^3}$$ has $$2$$ significant figures. Hence the density is reported to $$2$$ significant figures.

$$\rho = 4.8 \, \mathrm{g \, cm^{-3}}$$

Answer

$$\rho = 4.8 \, \mathrm{g \, cm^{-3}}$$.

Example 1.3 Let us consider an equation $$\frac{1}{2} m v^2 = m g h$$ where $$m$$ is the mass of the body, $$v$$ its velocity, $$g$$ is the acceleration due to gravity and $$h$$ is the height. Check whether this equation is dimensionally correct.

Solution

We compare the dimensions of the left-hand side (LHS) and the right-hand side (RHS) using $$[M]$$, $$[L]$$ and $$[T]$$ for mass, length and time.

Dimensions of LHS: $$\tfrac{1}{2}$$ is a pure number and is dimensionless.

$$[\tfrac{1}{2} m v^2] = [m][v]^2 = [M][L \, T^{-1}]^2 = [M \, L^2 \, T^{-2}]$$

Dimensions of RHS:

$$[m g h] = [M][L \, T^{-2}][L] = [M \, L^2 \, T^{-2}]$$

The dimensions on both sides are identical: $$[M^1 \, L^2 \, T^{-2}]$$. Hence the equation is dimensionally correct.

Note: Dimensional correctness does not by itself prove physical correctness; for instance, a missing dimensionless factor (such as $$\tfrac{1}{2}$$) cannot be detected by this method.

Answer

The equation is dimensionally correct; both sides have dimensions $$[M \, L^2 \, T^{-2}]$$.

Example 1.4

The SI unit of energy is $$\mathrm{J = kg \, m^2 \, s^{-2}}$$; that of speed $$v$$ is $$\mathrm{m \, s^{-1}}$$ and of acceleration $$a$$ is $$\mathrm{m \, s^{-2}}$$. Which of the formulae for kinetic energy ($$K$$) given below can you rule out on the basis of dimensional arguments ($$m$$ stands for the mass of the body):

(a) $$K = m^2 v^3$$

Solution

Energy has dimensions $$[M \, L^2 \, T^{-2}]$$.

$$[m^2 v^3] = [M]^2 [L \, T^{-1}]^3 = [M^2 \, L^3 \, T^{-3}]$$

This is not equal to $$[M \, L^2 \, T^{-2}]$$, so the formula is dimensionally incorrect and is ruled out.

Answer

Ruled out (dimensions $$[M^2 \, L^3 \, T^{-3}] \ne [M \, L^2 \, T^{-2}]$$).

(b) $$K = (1/2) m v^2$$

Solution

$$\tfrac{1}{2}$$ is a dimensionless factor.

$$\left[\tfrac{1}{2} m v^2\right] = [M][L \, T^{-1}]^2 = [M \, L^2 \, T^{-2}]$$

These are precisely the dimensions of energy. The formula is dimensionally consistent and cannot be ruled out. (This is in fact the correct expression for kinetic energy.)

Answer

Dimensionally correct; cannot be ruled out.

(c) $$K = m a$$

Solution

$$[m a] = [M][L \, T^{-2}] = [M \, L \, T^{-2}]$$

These are the dimensions of force, not energy. Hence the formula is dimensionally incorrect and is ruled out.

Answer

Ruled out ($$[M \, L \, T^{-2}]$$ are the dimensions of force, not energy).

(d) $$K = (3/16) m v^2$$

Solution

$$\tfrac{3}{16}$$ is a dimensionless number.

$$\left[\tfrac{3}{16} m v^2\right] = [M][L \, T^{-1}]^2 = [M \, L^2 \, T^{-2}]$$

These are the dimensions of energy, so the formula is dimensionally consistent and cannot be ruled out on dimensional grounds alone. (Dimensional analysis cannot detect a wrong numerical factor.)

Answer

Dimensionally correct; cannot be ruled out by dimensional analysis.

(e) $$K = (1/2) m v^2 + m a$$

Solution

For an equation to be dimensionally correct, every term added on the right must have the same dimensions.

$$\left[\tfrac{1}{2} m v^2\right] = [M \, L^2 \, T^{-2}] \quad \text{(energy)}$$

$$[m a] = [M \, L \, T^{-2}] \quad \text{(force)}$$

The two terms have different dimensions, so they cannot be added. The formula is dimensionally inconsistent and is ruled out.

Answer

Ruled out (energy and force cannot be added).

Example 1.5 Consider a simple pendulum, having a bob attached to a string, that oscillates under the action of the force of gravity. Suppose that the period of oscillation of the simple pendulum depends on its length ($$l$$), mass of the bob ($$m$$) and acceleration due to gravity ($$g$$). Derive the expression for its time period using method of dimensions.

Solution

Assume the time period $$T$$ depends on the length $$l$$, mass $$m$$ and acceleration due to gravity $$g$$ as

$$T = k \, l^{a} \, m^{b} \, g^{c}$$

where $$k$$ is a dimensionless constant and $$a$$, $$b$$, $$c$$ are exponents to be found.

Writing the dimensions of each quantity:

$$[T] = [T^{1}], \quad [l] = [L], \quad [m] = [M], \quad [g] = [L \, T^{-2}]$$

Substituting,

$$[T^{1}] = [L]^{a} [M]^{b} [L \, T^{-2}]^{c} = [M^{b} \, L^{a+c} \, T^{-2c}]$$

Comparing exponents of $$M$$, $$L$$ and $$T$$ on both sides:

$$b = 0, \qquad a + c = 0, \qquad -2c = 1$$

Solving: $$c = -\tfrac{1}{2}$$ and hence $$a = +\tfrac{1}{2}$$, with $$b = 0$$.

Therefore

$$T = k \, l^{1/2} \, g^{-1/2} = k \sqrt{\dfrac{l}{g}}$$

Experimentally (or from a detailed analysis of the equation of motion) it is found that $$k = 2\pi$$, giving the well-known formula

$$T = 2\pi \sqrt{\dfrac{l}{g}}$$

Note that the time period is independent of the mass of the bob — a result predicted by dimensional analysis itself.

Answer

$$T = 2\pi \sqrt{l/g}$$; independent of mass.

Exercises

1.1 Fill in the blanks

(a) The volume of a cube of side $$1 \, \mathrm{cm}$$ is equal to .....$$\mathrm{m^3}$$

Solution

Side $$a = 1 \, \mathrm{cm} = 10^{-2} \, \mathrm{m}$$.

$$V = a^3 = (10^{-2} \, \mathrm{m})^3 = 10^{-6} \, \mathrm{m^3}$$

Answer

$$1 \, \mathrm{cm^3} = 10^{-6} \, \mathrm{m^3}$$.

(b) The surface area of a solid cylinder of radius $$2.0 \, \mathrm{cm}$$ and height $$10.0 \, \mathrm{cm}$$ is equal to ...$$\mathrm{(mm)^2}$$

Solution

The total surface area of a solid (closed) cylinder is the lateral area plus the two end discs:

$$S = 2\pi r h + 2\pi r^2 = 2\pi r (r + h)$$

Substituting $$r = 2.0 \, \mathrm{cm}$$ and $$h = 10.0 \, \mathrm{cm}$$:

$$S = 2\pi \times 2.0 \times (2.0 + 10.0) \, \mathrm{cm^2} = 48\pi \, \mathrm{cm^2}$$

$$S \approx 48 \times 3.14159 \, \mathrm{cm^2} \approx 150.8 \, \mathrm{cm^2}$$

Convert to square millimetres: $$1 \, \mathrm{cm} = 10 \, \mathrm{mm}$$, so $$1 \, \mathrm{cm^2} = 100 \, \mathrm{mm^2} = 10^{2} \, \mathrm{mm^2}$$.

$$S = 150.8 \times 10^{2} \, \mathrm{mm^2} \approx 1.5 \times 10^{4} \, \mathrm{mm^2}$$

Answer

$$S \approx 1.5 \times 10^{4} \, \mathrm{mm^2}$$.

(c) A vehicle moving with a speed of $$18 \, \mathrm{km \, h^{-1}}$$ covers....$$\mathrm{m}$$ in $$1 \, \mathrm{s}$$

Solution

Convert the speed to SI units.

$$1 \, \mathrm{km \, h^{-1}} = \dfrac{1000 \, \mathrm{m}}{3600 \, \mathrm{s}} = \dfrac{5}{18} \, \mathrm{m \, s^{-1}}$$

$$18 \, \mathrm{km \, h^{-1}} = 18 \times \dfrac{5}{18} \, \mathrm{m \, s^{-1}} = 5 \, \mathrm{m \, s^{-1}}$$

Therefore, in $$1 \, \mathrm{s}$$ the vehicle covers $$5 \, \mathrm{m}$$.

Answer

$$5 \, \mathrm{m}$$.

(d) The relative density of lead is $$11.3$$. Its density is ....$$\mathrm{g \, cm^{-3}}$$ or ....$$\mathrm{kg \, m^{-3}}$$.

Solution

Relative density (specific gravity) is the ratio of the density of a material to the density of water at $$4 \, \mathrm{^{\circ}C}$$.

Density of water $$= 1 \, \mathrm{g \, cm^{-3}} = 10^{3} \, \mathrm{kg \, m^{-3}}$$.

$$\rho_{\mathrm{lead}} = 11.3 \times 1 \, \mathrm{g \, cm^{-3}} = 11.3 \, \mathrm{g \, cm^{-3}}$$

Converting to SI:

$$\rho_{\mathrm{lead}} = 11.3 \times 10^{3} \, \mathrm{kg \, m^{-3}} = 1.13 \times 10^{4} \, \mathrm{kg \, m^{-3}}$$

Answer

$$11.3 \, \mathrm{g \, cm^{-3}}$$ or $$1.13 \times 10^{4} \, \mathrm{kg \, m^{-3}}$$.

1.2 Fill in the blanks by suitable conversion of units

(a) $$1 \, \mathrm{kg \, m^2 \, s^{-2}} = ....\mathrm{g \, cm^2 \, s^{-2}}$$

Solution

Use $$1 \, \mathrm{kg} = 10^{3} \, \mathrm{g}$$ and $$1 \, \mathrm{m} = 10^{2} \, \mathrm{cm}$$, so $$1 \, \mathrm{m^2} = 10^{4} \, \mathrm{cm^2}$$.

$$1 \, \mathrm{kg \, m^2 \, s^{-2}} = (10^{3} \, \mathrm{g}) \times (10^{4} \, \mathrm{cm^2}) \times \mathrm{s^{-2}}$$

$$= 10^{3+4} \, \mathrm{g \, cm^2 \, s^{-2}} = 10^{7} \, \mathrm{g \, cm^2 \, s^{-2}}$$

Answer

$$10^{7} \, \mathrm{g \, cm^2 \, s^{-2}}$$.

(b) $$1 \, \mathrm{m} = .....\mathrm{ly}$$

Solution

One light year ($$\mathrm{ly}$$) is the distance light travels in vacuum in one year.

$$1 \, \mathrm{ly} = c \times (1 \, \mathrm{year})$$

Taking $$c = 3 \times 10^{8} \, \mathrm{m \, s^{-1}}$$ and $$1 \, \mathrm{year} \approx 365.25 \times 24 \times 3600 \, \mathrm{s} = 3.156 \times 10^{7} \, \mathrm{s}$$,

$$1 \, \mathrm{ly} = (3 \times 10^{8}) \times (3.156 \times 10^{7}) \, \mathrm{m} \approx 9.46 \times 10^{15} \, \mathrm{m}$$

Therefore

$$1 \, \mathrm{m} = \dfrac{1}{9.46 \times 10^{15}} \, \mathrm{ly} \approx 1.057 \times 10^{-16} \, \mathrm{ly}$$

Answer

$$1 \, \mathrm{m} \approx 1.057 \times 10^{-16} \, \mathrm{ly}$$.

(c) $$3.0 \, \mathrm{m \, s^{-2}} = .... \mathrm{km \, h^{-2}}$$

Solution

Use $$1 \, \mathrm{m} = 10^{-3} \, \mathrm{km}$$ and $$1 \, \mathrm{s} = \dfrac{1}{3600} \, \mathrm{h}$$, so $$1 \, \mathrm{s^{-2}} = 3600^2 \, \mathrm{h^{-2}} = 1.296 \times 10^{7} \, \mathrm{h^{-2}}$$.

$$3.0 \, \mathrm{m \, s^{-2}} = 3.0 \times 10^{-3} \, \mathrm{km} \times 1.296 \times 10^{7} \, \mathrm{h^{-2}}$$

$$= 3.0 \times 1.296 \times 10^{4} \, \mathrm{km \, h^{-2}}$$

$$= 3.888 \times 10^{4} \, \mathrm{km \, h^{-2}} \approx 3.9 \times 10^{4} \, \mathrm{km \, h^{-2}}$$

Answer

$$3.9 \times 10^{4} \, \mathrm{km \, h^{-2}}$$.

(d) $$G = 6.67 \times 10^{-11} \, \mathrm{N \, m^2 \, (kg)^{-2}} = .... \mathrm{(cm)^3 \, s^{-2} \, g^{-1}}$$.

Solution

The SI unit of $$G$$ is $$\mathrm{N \, m^2 \, kg^{-2}}$$. Expressing newton in base SI units, $$1 \, \mathrm{N} = 1 \, \mathrm{kg \, m \, s^{-2}}$$, so

$$\mathrm{N \, m^2 \, kg^{-2}} = (\mathrm{kg \, m \, s^{-2}}) \, \mathrm{m^2 \, kg^{-2}} = \mathrm{m^3 \, kg^{-1} \, s^{-2}}$$

Hence $$G = 6.67 \times 10^{-11} \, \mathrm{m^3 \, kg^{-1} \, s^{-2}}$$.

Now convert to CGS: $$1 \, \mathrm{m^3} = 10^{6} \, \mathrm{cm^3}$$ and $$1 \, \mathrm{kg^{-1}} = 10^{-3} \, \mathrm{g^{-1}}$$.

$$G = 6.67 \times 10^{-11} \times 10^{6} \times 10^{-3} \, \mathrm{cm^3 \, g^{-1} \, s^{-2}}$$

$$= 6.67 \times 10^{-11 + 6 - 3} \, \mathrm{cm^3 \, g^{-1} \, s^{-2}} = 6.67 \times 10^{-8} \, \mathrm{cm^3 \, s^{-2} \, g^{-1}}$$

Answer

$$G = 6.67 \times 10^{-8} \, \mathrm{cm^3 \, s^{-2} \, g^{-1}}$$.

1.3 A calorie is a unit of heat (energy in transit) and it equals about $$4.2 \, \mathrm{J}$$ where $$1 \mathrm{J} = 1 \, \mathrm{kg \, m^2 \, s^{-2}}$$. Suppose we employ a system of units in which the unit of mass equals $$\alpha \, \mathrm{kg}$$, the unit of length equals $$\beta \, \mathrm{m}$$, the unit of time is $$\gamma \, \mathrm{s}$$. Show that a calorie has a magnitude $$4.2 \, \alpha^{-1} \beta^{-2} \gamma^{2}$$ in terms of the new units.

Solution

The dimensional formula of energy is $$[E] = [M^1 \, L^2 \, T^{-2}]$$, so the numerical value of energy in any system is

$$n \propto \dfrac{1}{(\text{unit of mass})^1 \, (\text{unit of length})^2 \, (\text{unit of time})^{-2}}$$

If $$n_1$$ is the numerical value in one system (with units $$M_1, L_1, T_1$$) and $$n_2$$ in another (with units $$M_2, L_2, T_2$$), then

$$n_1 \, M_1^{1} L_1^{2} T_1^{-2} = n_2 \, M_2^{1} L_2^{2} T_2^{-2}$$

so

$$n_2 = n_1 \left(\dfrac{M_1}{M_2}\right)^{1} \left(\dfrac{L_1}{L_2}\right)^{2} \left(\dfrac{T_1}{T_2}\right)^{-2}$$

System 1 (SI): $$M_1 = 1 \, \mathrm{kg}$$, $$L_1 = 1 \, \mathrm{m}$$, $$T_1 = 1 \, \mathrm{s}$$, and $$n_1 = 4.2$$ (since $$1 \, \mathrm{cal} = 4.2 \, \mathrm{J} = 4.2 \, \mathrm{kg \, m^2 \, s^{-2}}$$).

System 2 (new): $$M_2 = \alpha \, \mathrm{kg}$$, $$L_2 = \beta \, \mathrm{m}$$, $$T_2 = \gamma \, \mathrm{s}$$.

Substituting,

$$n_2 = 4.2 \times \left(\dfrac{1 \, \mathrm{kg}}{\alpha \, \mathrm{kg}}\right)^{1} \left(\dfrac{1 \, \mathrm{m}}{\beta \, \mathrm{m}}\right)^{2} \left(\dfrac{1 \, \mathrm{s}}{\gamma \, \mathrm{s}}\right)^{-2}$$

$$n_2 = 4.2 \, \alpha^{-1} \, \beta^{-2} \, \gamma^{2}$$

Hence in the new units the magnitude of $$1 \, \mathrm{cal}$$ is $$4.2 \, \alpha^{-1} \beta^{-2} \gamma^{2}$$, as required.

Answer

Shown: $$n_{\text{new}} = 4.2 \, \alpha^{-1} \, \beta^{-2} \, \gamma^{2}$$.

1.4

Explain this statement clearly :

"To call a dimensional quantity 'large' or 'small' is meaningless without specifying a standard for comparison". In view of this, reframe the following statements wherever necessary :

(a) atoms are very small objects

Solution

Calling atoms 'small' has no absolute meaning — small compared to what? A grain of sand is also small compared to a building, but enormous compared to an atom. We must specify the standard of comparison.

Reframed: Atoms are very small objects compared to a tip of a sharp pin (or compared to everyday macroscopic objects).

Answer

Reframed: atoms are very small compared to everyday macroscopic objects (e.g. the tip of a pin).

(b) a jet plane moves with great speed

Solution

'Great speed' is meaningless without a benchmark. A jet at $$800 \, \mathrm{km \, h^{-1}}$$ is fast compared to a bicycle but slow compared to light.

Reframed: A jet plane moves with great speed compared to a bicycle (or to ordinary land vehicles).

Answer

Reframed: a jet plane moves with great speed compared to ordinary land vehicles such as a bicycle or car.

(c) the mass of Jupiter is very large

Solution

'Large mass' must be relative to some standard. Jupiter is heavy compared to the Earth, but tiny compared to the Sun.

Reframed: The mass of Jupiter is very large compared to the mass of the Earth (about $$318$$ times the Earth's mass).

Answer

Reframed: the mass of Jupiter is very large compared to the mass of the Earth (or of other planets).

(d) the air inside this room contains a large number of molecules

Solution

The number of molecules is itself a dimensionless count, but the word 'large' is still relative. The statement is meaningful only when we say large compared to what.

A typical room ($$\sim 50 \, \mathrm{m^3}$$ of air) contains roughly $$10^{27}$$ molecules, which is enormous compared to the number of atoms in, say, a pinhead of metal (which is itself huge, $$\sim 10^{20}$$). Thus the statement is correct in spirit but requires a standard of comparison.

Reframed: The air inside this room contains a number of molecules far greater than the number of molecules in a small drop of water (or any everyday small sample).

Answer

Reframed: the number of molecules in the room is very large compared to the number of molecules in a small drop of water (or in any small sample of matter for comparison).

(e) a proton is much more massive than an electron

Solution

This statement already contains the standard of comparison (the electron). The proton mass is $$m_p \approx 1.67 \times 10^{-27} \, \mathrm{kg}$$ and the electron mass is $$m_e \approx 9.11 \times 10^{-31} \, \mathrm{kg}$$, giving

$$\dfrac{m_p}{m_e} \approx 1836$$

The statement is therefore correct as it stands; no reframing is needed.

Answer

Correct as stated — the proton mass is compared with the electron mass ($$m_p / m_e \approx 1836$$).

(f) the speed of sound is much smaller than the speed of light.

Solution

This statement explicitly compares two well-defined quantities: $$v_{\text{sound}} \approx 340 \, \mathrm{m \, s^{-1}}$$ in air and $$c \approx 3 \times 10^{8} \, \mathrm{m \, s^{-1}}$$.

$$\dfrac{v_{\text{sound}}}{c} \sim 10^{-6}$$

The statement is correct as it stands; no reframing is required.

Answer

Correct as stated — the speed of sound is compared with the speed of light (ratio $$\sim 10^{-6}$$).

1.5 A new unit of length is chosen such that the speed of light in vacuum is unity. What is the distance between the Sun and the Earth in terms of the new unit if light takes $$8 \, \mathrm{min}$$ and $$20 \, \mathrm{s}$$ to cover this distance ?

Solution

In the new system the speed of light is unity, i.e. $$c = 1 \, (\text{new unit of length}) \, \mathrm{s^{-1}}$$. The new unit of length is therefore the distance light travels in $$1 \, \mathrm{s}$$ (a 'light-second').

Convert the travel time to seconds:

$$t = 8 \, \mathrm{min} + 20 \, \mathrm{s} = 8 \times 60 \, \mathrm{s} + 20 \, \mathrm{s} = 500 \, \mathrm{s}$$

The Sun–Earth distance is

$$d = c \, t = 1 \times 500 \, (\text{new unit}) = 500 \, \text{new units of length}$$

Answer

$$d = 500$$ (new units of length).

1.6 Which of the following is the most precise device for measuring length :

(a) a vernier callipers with $$20$$ divisions on the sliding scale

Solution

For vernier callipers the least count is

$$\text{LC} = \dfrac{\text{value of 1 main-scale division}}{\text{number of vernier divisions}} = \dfrac{1 \, \mathrm{mm}}{20} = 0.05 \, \mathrm{mm} = 5 \times 10^{-5} \, \mathrm{m}$$

Answer

Least count $$= 0.05 \, \mathrm{mm} = 5 \times 10^{-5} \, \mathrm{m}$$.

(b) a screw gauge of pitch $$1 \, \mathrm{mm}$$ and $$100$$ divisions on the circular scale

Solution

For a screw gauge,

$$\text{LC} = \dfrac{\text{pitch}}{\text{number of circular-scale divisions}} = \dfrac{1 \, \mathrm{mm}}{100} = 0.01 \, \mathrm{mm} = 10^{-5} \, \mathrm{m}$$

Answer

Least count $$= 0.01 \, \mathrm{mm} = 10^{-5} \, \mathrm{m}$$.

(c) an optical instrument that can measure length to within a wavelength of light ?

Solution

The wavelength of visible light is in the range $$400 \text{–} 700 \, \mathrm{nm}$$. Taking a representative value $$\lambda \sim 600 \, \mathrm{nm}$$,

$$\text{LC} \sim \lambda \sim 6 \times 10^{-7} \, \mathrm{m}$$

Comparison of the three least counts:

  • Vernier callipers: $$5 \times 10^{-5} \, \mathrm{m}$$
  • Screw gauge: $$1 \times 10^{-5} \, \mathrm{m}$$
  • Optical instrument: $$\sim 6 \times 10^{-7} \, \mathrm{m}$$

The optical instrument has the smallest least count and is therefore the most precise of the three.

Answer

The optical instrument (least count $$\sim 10^{-7} \, \mathrm{m}$$) is the most precise.

1.7 A student measures the thickness of a human hair by looking at it through a microscope of magnification $$100$$. He makes $$20$$ observations and finds that the average width of the hair in the field of view of the microscope is $$3.5 \, \mathrm{mm}$$. What is the estimate on the thickness of hair ?

Solution

The microscope produces a magnified image whose linear dimension is

$$\text{(image size)} = M \times \text{(object size)}$$

where $$M = 100$$ is the linear magnification. Hence

$$\text{(thickness of hair)} = \dfrac{\text{image width}}{M} = \dfrac{3.5 \, \mathrm{mm}}{100}$$

$$= 3.5 \times 10^{-2} \, \mathrm{mm} = 0.035 \, \mathrm{mm} = 3.5 \times 10^{-5} \, \mathrm{m}$$

Answer

Thickness $$\approx 3.5 \times 10^{-2} \, \mathrm{mm} = 3.5 \times 10^{-5} \, \mathrm{m}$$.

1.8 Answer the following :

(a) You are given a thread and a metre scale. How will you estimate the diameter of the thread ?

Solution

A metre scale cannot measure a length as small as the diameter of a thread directly (its least count is $$1 \, \mathrm{mm}$$). We exploit the fact that many turns of the thread laid side-by-side make a measurable length.

Procedure:

  1. Wrap the thread tightly around a uniform pencil (or a thin cylinder) in close, non-overlapping turns, so that consecutive turns just touch each other.
  2. Count the number of turns, say $$n$$.
  3. Measure the length $$L$$ occupied by these $$n$$ turns using the metre scale.
  4. The diameter of the thread is then

$$d = \dfrac{L}{n}$$

Taking a large $$n$$ reduces the relative error since the smallest measurable length on the scale is divided over many turns.

Answer

Wind $$n$$ tight turns of thread on a pencil, measure the total length $$L$$, and take $$d = L/n$$.

(b) A screw gauge has a pitch of $$1.0 \, \mathrm{mm}$$ and $$200$$ divisions on the circular scale. Do you think it is possible to increase the accuracy of the screw gauge arbitrarily by increasing the number of divisions on the circular scale ?

Solution

The least count is $$\text{LC} = \text{pitch}/N$$. Increasing $$N$$ does reduce the LC arithmetically; for example $$N = 200$$ gives

$$\text{LC} = \dfrac{1.0 \, \mathrm{mm}}{200} = 0.005 \, \mathrm{mm} = 5 \, \mu\mathrm{m}$$

However, the accuracy of an actual measurement is limited by several practical factors that do not improve when we cram more divisions onto the circular scale:

  • The physical width of the divisions on the circular scale becomes smaller than the human eye (or even an aided eye) can resolve. Reading errors then dominate.
  • Mechanical imperfections — backlash, screw wear, non-uniform pitch, and zero-error drift — set a lower floor on what is reliable.
  • Random errors from the observer (parallax, judgment of coincidence) become comparable to the nominal least count.

Therefore, beyond a certain point increasing $$N$$ improves the nominal least count but not the actual accuracy. So no, the accuracy cannot be increased arbitrarily.

Answer

No — increasing $$N$$ reduces the nominal least count but practical limits (visibility of divisions, mechanical imperfections, observer error) prevent accuracy from improving arbitrarily.

(c) The mean diameter of a thin brass rod is to be measured by vernier callipers. Why is a set of $$100$$ measurements of the diameter expected to yield a more reliable estimate than a set of $$5$$ measurements only ?

Solution

Repeated measurements suffer from random errors (small unpredictable fluctuations in the observer's reading, slight misalignment, slight variations in jaw pressure, etc.). These errors are equally likely to be positive or negative, so they tend to cancel on averaging.

If individual measurements have a standard deviation $$\sigma$$, the standard error of the mean of $$n$$ independent observations is

$$\sigma_{\bar{x}} = \dfrac{\sigma}{\sqrt{n}}$$

Comparing $$n = 100$$ with $$n = 5$$:

$$\dfrac{\sigma_{\bar{x}}(100)}{\sigma_{\bar{x}}(5)} = \sqrt{\dfrac{5}{100}} = \dfrac{1}{\sqrt{20}} \approx 0.22$$

So the uncertainty in the mean from $$100$$ readings is about $$4.5$$ times smaller than from $$5$$ readings, making the estimate substantially more reliable.

Answer

The mean of $$n$$ readings has uncertainty $$\sigma/\sqrt{n}$$, so $$100$$ readings give about $$\sqrt{100/5} \approx 4.5$$ times better precision than $$5$$ readings.

1.9 The photograph of a house occupies an area of $$1.75 \, \mathrm{cm^2}$$ on a $$35 \, \mathrm{mm}$$ slide. The slide is projected on to a screen, and the area of the house on the screen is $$1.55 \, \mathrm{m^2}$$. What is the linear magnification of the projector-screen arrangement.

Solution

Area magnification is the square of the linear magnification:

$$M_{\text{area}} = M_{\text{linear}}^{2}$$

Convert both areas to the same unit. With $$1 \, \mathrm{m^2} = 10^{4} \, \mathrm{cm^2}$$,

$$A_{\text{screen}} = 1.55 \, \mathrm{m^2} = 1.55 \times 10^{4} \, \mathrm{cm^2}$$

$$M_{\text{area}} = \dfrac{A_{\text{screen}}}{A_{\text{slide}}} = \dfrac{1.55 \times 10^{4} \, \mathrm{cm^2}}{1.75 \, \mathrm{cm^2}} = 8.857 \times 10^{3}$$

Hence

$$M_{\text{linear}} = \sqrt{M_{\text{area}}} = \sqrt{8857.14} \approx 94.1$$

Answer

Linear magnification $$\approx 94.1$$.

1.10 State the number of significant figures in the following :

(a) $$0.007 \, \mathrm{m^2}$$

Solution

Leading zeros that fix only the position of the decimal point are not significant. In $$0.007$$ the only significant digit is the final $$7$$.

(Equivalently, $$0.007 = 7 \times 10^{-3}$$.)

Answer

$$1$$ significant figure.

(b) $$2.64 \times 10^{24} \, \mathrm{kg}$$

Solution

In scientific notation, only the digits in the mantissa $$2.64$$ are counted as significant; the power of $$10$$ merely fixes the magnitude. The mantissa has three digits: $$2$$, $$6$$ and $$4$$.

Answer

$$3$$ significant figures.

(c) $$0.2370 \, \mathrm{g \, cm^{-3}}$$

Solution

The leading zero (before the decimal point) is not significant. The digits $$2$$, $$3$$, $$7$$ are significant, and the trailing $$0$$ after the decimal point is also significant (it conveys precision).

Answer

$$4$$ significant figures.

(d) $$6.320 \, \mathrm{J}$$

Solution

All four digits — $$6$$, $$3$$, $$2$$ and the trailing $$0$$ after the decimal point — are significant.

Answer

$$4$$ significant figures.

(e) $$6.032 \, \mathrm{N \, m^{-2}}$$

Solution

All non-zero digits are significant; zeros sandwiched between non-zero digits are also significant. So $$6$$, $$0$$, $$3$$, $$2$$ all count.

Answer

$$4$$ significant figures.

(f) $$0.0006032 \, \mathrm{m^2}$$

Solution

Leading zeros (before and after the decimal point but before the first non-zero digit) are not significant; they only locate the decimal. The significant digits are $$6$$, $$0$$, $$3$$, $$2$$.

(In scientific notation, $$0.0006032 = 6.032 \times 10^{-4}$$, which makes the four significant figures explicit.)

Answer

$$4$$ significant figures.

1.11 The length, breadth and thickness of a rectangular sheet of metal are $$4.234 \, \mathrm{m}$$, $$1.005 \, \mathrm{m}$$, and $$2.01 \, \mathrm{cm}$$ respectively. Give the area and volume of the sheet to correct significant figures.

Solution

Convert the thickness to metres: $$t = 2.01 \, \mathrm{cm} = 0.0201 \, \mathrm{m}$$. The three measurements have $$4$$, $$4$$ and $$3$$ significant figures respectively; products must therefore be quoted to $$3$$ significant figures.

Total surface area of a rectangular sheet (parallelepiped) of length $$L$$, breadth $$B$$, thickness $$t$$:

$$S = 2(LB + Bt + tL)$$

Computing each pair-wise product:

$$LB = 4.234 \times 1.005 \, \mathrm{m^2} = 4.25517 \, \mathrm{m^2}$$

$$Bt = 1.005 \times 0.0201 \, \mathrm{m^2} = 0.0202005 \, \mathrm{m^2}$$

$$tL = 0.0201 \times 4.234 \, \mathrm{m^2} = 0.0851034 \, \mathrm{m^2}$$

Sum $$= 4.25517 + 0.0202005 + 0.0851034 = 4.36047 \, \mathrm{m^2}$$

$$S = 2 \times 4.36047 = 8.72095 \, \mathrm{m^2}$$

To three significant figures, $$S \approx 8.72 \, \mathrm{m^2}$$.

Volume:

$$V = L \, B \, t = 4.234 \times 1.005 \times 0.0201 \, \mathrm{m^3}$$

$$V = 4.25517 \times 0.0201 = 0.0855289 \, \mathrm{m^3}$$

To three significant figures, $$V \approx 0.0855 \, \mathrm{m^3} = 8.55 \times 10^{-2} \, \mathrm{m^3}$$.

Answer

Surface area $$\approx 8.72 \, \mathrm{m^2}$$; Volume $$\approx 0.0855 \, \mathrm{m^3}$$.

1.12 The mass of a box measured by a grocer's balance is $$2.30 \, \mathrm{kg}$$. Two gold pieces of masses $$20.15 \, \mathrm{g}$$ and $$20.17 \, \mathrm{g}$$ are added to the box. What is (a) the total mass of the box, (b) the difference in the masses of the pieces to correct significant figures ?

Solution

For addition and subtraction the result must be expressed to the same number of decimal places as the term with the fewest decimal places (i.e. with the largest uncertainty).

Express the gold-piece masses in kilograms: $$20.15 \, \mathrm{g} = 0.02015 \, \mathrm{kg}$$ and $$20.17 \, \mathrm{g} = 0.02017 \, \mathrm{kg}$$.

(a) Total mass of the box (box + two gold pieces):

$$m_{\text{total}} = 2.30 + 0.02015 + 0.02017 \, \mathrm{kg} = 2.34032 \, \mathrm{kg}$$

The least precise term is $$2.30 \, \mathrm{kg}$$, known to two decimal places. Rounding the sum to two decimal places:

$$m_{\text{total}} \approx 2.34 \, \mathrm{kg}$$

(b) Difference between the gold pieces (both known to two decimal places in grams):

$$\Delta m = 20.17 - 20.15 = 0.02 \, \mathrm{g}$$

The result $$0.02 \, \mathrm{g}$$ is correctly written to two decimal places (matching the precision of the inputs).

Answer

(a) Total mass $$\approx 2.34 \, \mathrm{kg}$$; (b) difference $$= 0.02 \, \mathrm{g}$$.

1.13 A famous relation in physics relates 'moving mass' $$m$$ to the 'rest mass' $$m_0$$ of a particle in terms of its speed $$v$$ and the speed of light, $$c$$. (This relation first arose as a consequence of special relativity due to Albert Einstein). A boy recalls the relation almost correctly but forgets where to put the constant $$c$$. He writes : $$m = \frac{m_0}{\left(1 - v^2\right)^{1/2}}$$ Guess where to put the missing $$c$$.

Solution

For the expression to make dimensional sense, the quantity inside the square root, $$1 - v^{2}$$, must be dimensionless — because we can only subtract a pure number from $$1$$.

$$v$$ has dimensions $$[L \, T^{-1}]$$, so $$v^2$$ has dimensions $$[L^{2} T^{-2}]$$ and is not dimensionless.

To make $$v^{2}$$ dimensionless, divide it by another quantity with the same dimensions. The only such constant available is the speed of light $$c$$ (with the same dimensions $$[L \, T^{-1}]$$). Hence the missing factor is $$c^{2}$$ in the denominator of $$v^{2}$$:

$$m = \dfrac{m_0}{\sqrt{1 - v^{2}/c^{2}}}$$

Now $$v/c$$ is dimensionless and the formula is dimensionally consistent. This is the standard relativistic mass formula.

Answer

$$m = m_0 / \sqrt{1 - v^{2}/c^{2}}$$.

1.14 The unit of length convenient on the atomic scale is known as an angstrom and is denoted by $$\mathrm{\AA}$$: $$1 \, \mathrm{\AA} = 10^{-10} \, \mathrm{m}$$. The size of a hydrogen atom is about $$0.5 \, \mathrm{\AA}$$. What is the total atomic volume in $$\mathrm{m^3}$$ of a mole of hydrogen atoms ?

Solution

Treat a hydrogen atom as a sphere of radius

$$r = 0.5 \, \mathrm{\AA} = 0.5 \times 10^{-10} \, \mathrm{m} = 5 \times 10^{-11} \, \mathrm{m}$$

Volume of one atom:

$$V_{1} = \dfrac{4}{3}\pi r^{3} = \dfrac{4}{3} \times 3.14159 \times (5 \times 10^{-11})^{3} \, \mathrm{m^3}$$

$$(5 \times 10^{-11})^{3} = 125 \times 10^{-33} = 1.25 \times 10^{-31}$$

$$V_{1} = \dfrac{4}{3} \times 3.14159 \times 1.25 \times 10^{-31} \, \mathrm{m^3} \approx 5.236 \times 10^{-31} \, \mathrm{m^3}$$

Total atomic volume in one mole (Avogadro's number $$N_A = 6.022 \times 10^{23}$$):

$$V_{\text{mole}} = N_A \times V_{1} = 6.022 \times 10^{23} \times 5.236 \times 10^{-31} \, \mathrm{m^3}$$

$$V_{\text{mole}} \approx 3.15 \times 10^{-7} \, \mathrm{m^3}$$

Answer

$$V_{\text{mole}} \approx 3.15 \times 10^{-7} \, \mathrm{m^3}$$.

1.15 One mole of an ideal gas at standard temperature and pressure occupies $$22.4 \, \mathrm{L}$$ (molar volume). What is the ratio of molar volume to the atomic volume of a mole of hydrogen ? (Take the size of hydrogen molecule to be about $$1 \, \mathrm{\AA}$$). Why is this ratio so large ?

Solution

Take the 'size' of the hydrogen molecule to be its diameter $$\sim 1 \, \mathrm{\AA}$$, so its radius is $$r = 0.5 \, \mathrm{\AA} = 5 \times 10^{-11} \, \mathrm{m}$$.

Volume of one molecule:

$$V_{1} = \dfrac{4}{3}\pi r^{3} = \dfrac{4}{3} \times 3.14159 \times (5 \times 10^{-11})^{3} \, \mathrm{m^3} \approx 5.236 \times 10^{-31} \, \mathrm{m^3}$$

Total molecular (atomic) volume in one mole:

$$V_{\text{atomic}} = N_A V_{1} = 6.022 \times 10^{23} \times 5.236 \times 10^{-31} \, \mathrm{m^3} \approx 3.15 \times 10^{-7} \, \mathrm{m^3}$$

Molar volume of the gas at STP:

$$V_{\text{molar}} = 22.4 \, \mathrm{L} = 22.4 \times 10^{-3} \, \mathrm{m^3} = 2.24 \times 10^{-2} \, \mathrm{m^3}$$

Required ratio:

$$\dfrac{V_{\text{molar}}}{V_{\text{atomic}}} = \dfrac{2.24 \times 10^{-2}}{3.15 \times 10^{-7}} \approx 7.1 \times 10^{4}$$

This is large because in a gas the molecules are separated by distances much greater than their own size. Most of the gas volume is empty space — the molecules occupy only about $$1/70{,}000$$ of the total volume at STP. (Equivalently, the mean intermolecular separation is roughly the cube-root, $$\sim (7 \times 10^{4})^{1/3} \approx 40$$ times the molecular diameter.)

Answer

$$V_{\text{molar}}/V_{\text{atomic}} \approx 7.1 \times 10^{4}$$. So large because most of a gas is empty space — intermolecular separations are much larger than molecular sizes.

1.16 Explain this common observation clearly : If you look out of the window of a fast moving train, the nearby trees, houses etc. seem to move rapidly in a direction opposite to the train's motion, but the distant objects (hill tops, the Moon, the stars etc.) seem to be stationary. (In fact, since you are aware that you are moving, these distant objects seem to move with you).

Solution

The apparent motion of an external object as seen from a moving observer is governed by the rate at which the line of sight from observer to object turns — i.e. its angular velocity.

If $$v$$ is the train's speed and $$r$$ is the perpendicular distance of an object from the line of motion of the train, then in a short interval the line of sight to the object rotates through an angle

$$\Delta\theta \approx \dfrac{v \, \Delta t}{r}$$

so the apparent angular velocity is

$$\omega = \dfrac{\Delta\theta}{\Delta t} = \dfrac{v}{r}$$

For nearby objects (trees, houses, $$r$$ small) this $$\omega$$ is large; the objects sweep rapidly across the field of view, opposite to the train's motion.

For distant objects (hilltops, Moon, stars, $$r$$ very large) $$\omega \to 0$$; their angular position barely changes over the time of observation, so they appear practically stationary and seem to 'travel along with' the observer.

(The Moon, for example, is about $$3.8 \times 10^{8} \, \mathrm{m}$$ away; even at a train speed of $$30 \, \mathrm{m \, s^{-1}}$$ its line of sight rotates by only about $$8 \times 10^{-8} \, \mathrm{rad \, s^{-1}}$$, far too slow to perceive.)

Answer

Apparent angular velocity of an external object is $$\omega = v/r$$, where $$r$$ is its distance. Nearby objects (small $$r$$) have large $$\omega$$ and appear to rush backward; distant objects (huge $$r$$) have negligible $$\omega$$ and seem fixed.

1.17 The Sun is a hot plasma (ionized matter) with its inner core at a temperature exceeding $$10^7 \, \mathrm{K}$$, and its outer surface at a temperature of about $$6000 \, \mathrm{K}$$. At these high temperatures, no substance remains in a solid or liquid phase. In what range do you expect the mass density of the Sun to be, in the range of densities of solids and liquids or gases ? Check if your guess is correct from the following data : mass of the Sun $$= 2.0 \times 10^{30} \, \mathrm{kg}$$, radius of the Sun $$= 7.0 \times 10^8 \, \mathrm{m}$$.

Solution

Treat the Sun as a uniform sphere of radius $$R = 7.0 \times 10^{8} \, \mathrm{m}$$ and mass $$M = 2.0 \times 10^{30} \, \mathrm{kg}$$.

Volume:

$$V = \dfrac{4}{3}\pi R^{3} = \dfrac{4}{3} \times 3.14159 \times (7.0 \times 10^{8})^{3} \, \mathrm{m^3}$$

$$(7.0 \times 10^{8})^{3} = 343 \times 10^{24} = 3.43 \times 10^{26}$$

$$V = \dfrac{4}{3} \times 3.14159 \times 3.43 \times 10^{26} \, \mathrm{m^3} \approx 1.437 \times 10^{27} \, \mathrm{m^3}$$

Mean mass density:

$$\rho = \dfrac{M}{V} = \dfrac{2.0 \times 10^{30}}{1.437 \times 10^{27}} \, \mathrm{kg \, m^{-3}}$$

$$\rho \approx 1.39 \times 10^{3} \, \mathrm{kg \, m^{-3}} \approx 1.4 \, \mathrm{g \, cm^{-3}}$$

This is comparable to the density of water ($$10^{3} \, \mathrm{kg \, m^{-3}}$$) and lies in the range characteristic of solids and liquids, not gases (which at ordinary pressures have densities $$\sim 1 \, \mathrm{kg \, m^{-3}}$$).

The reason: although the Sun's material is a hot plasma (cannot be solid or liquid), the enormous self-gravitational compression squeezes the matter to a density typical of condensed matter. So the simple thermodynamic phase classification (solid/liquid/gas) does not directly predict density at astrophysical scales.

Answer

$$\rho \approx 1.4 \times 10^{3} \, \mathrm{kg \, m^{-3}}$$ — in the range of solids/liquids, not gases. Gravitational compression keeps the density high in spite of the high temperature.

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