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      Class 11 PHYSICS – JEE

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      • Class 11
      • Class 11 PHYSICS – JEE
      CoursesClass 11PhysicsClass 11 PHYSICS – JEE
      • 1.Basic Maths (1) : Vectors
        7
        • Lecture1.1
          Vector and Scalar, Representation of Vectors, Need for Co-ordinate System, Distance & Displacement 39 min
        • Lecture1.2
          Mathematics of Vectors, Triangle Law and Parallelogram Law 01 hour
        • Lecture1.3
          Addition More than Two Vectors, Subtraction of Vectors- Displacement vector 28 min
        • Lecture1.4
          Elementary Maths 14 min
        • Lecture1.5
          Unit Vectors, Special Unit Vectors, Resolution of Vectors 49 min
        • Lecture1.6
          Addition & Subtract using Unit Vectors, 3 D Vectors, Product of Vectors 54 min
        • Lecture1.7
          Chapter Notes – Basic Maths (1) : Vectors
      • 2.Basic Maths (2) : Calculus
        4
        • Lecture2.1
          Delta, Concept of Infinity, Time Instant Interval, Rate of Change, Position and Velocity 40 min
        • Lecture2.2
          Fundamental Idea of Differentiation- Constant Multiplication Rule, Sum/Difference Rule 29 min
        • Lecture2.3
          Trigonometric functions, Log function, Product Rule, Quotient Rule, Chain Rule 25 min
        • Lecture2.4
          Integration- Formulas of Integration, Use of Integration 45 min
      • 3.Unit and Measurement
        13
        • Lecture3.1
          Unit, History of Unit of Length-Metre, Properties of a Good Unit 21 min
        • Lecture3.2
          Concept of Derived Units, Fundamental Physics Quantities and Prefix of Units 38 min
        • Lecture3.3
          Unit-less Derived Quantities, Supplementary Quantities, Systems of Unit, Unit Conversion 39 min
        • Lecture3.4
          Dimensional Analysis, Dimension and Unit, Dimensionless Quantities 32 min
        • Lecture3.5
          Principle of Homogeneity 34 min
        • Lecture3.6
          Dimensionally Correct/Incorrect Equations, Use of Dimensional Analysis 41 min
        • Lecture3.7
          More Units of Length and Measurement of Length 47 min
        • Lecture3.8
          Errors and Their Reasons 36 min
        • Lecture3.9
          Combination of Errors 42 min
        • Lecture3.10
          Round Off, Significant Figures, Exponent Form of Numbers/Scientific Notation 27 min
        • Lecture3.11
          Chapter Notes – Unit and Measurement
        • Lecture3.12
          NCERT Solutions – Unit and Measurement
        • Lecture3.13
          Revision Notes – Unit and Measurement
      • 4.Motion (1) : Straight Line Motion
        10
        • Lecture4.1
          Meaning of Dimension; Position; Distance & Displacement 25 min
        • Lecture4.2
          Average Speed & Velocity; Instantaneous Speed & Velocity 31 min
        • Lecture4.3
          Photo Diagram; Acceleration- Direction of acceleration, Conceptual Examples 22 min
        • Lecture4.4
          Constant Acceleration; Equations of constant acceleration 43 min
        • Lecture4.5
          Average Velocity Examples and Concepts; Reaction Time 19 min
        • Lecture4.6
          Free Fall under Gravity 30 min
        • Lecture4.7
          Variable Acceleration; Derivation of Constant Acceleration Equations 48 min
        • Lecture4.8
          Chapter Notes – Motion (1) : Straight Line Motion
        • Lecture4.9
          NCERT Solutions – Straight Line Motion
        • Lecture4.10
          Revision Notes Straight Line Motion
      • 5.Motion (2) : Graphs
        3
        • Lecture5.1
          Tangent & Chord; Slope of Line- Chord & Tangent; Meaning of x/t graph, v/t graph, a/t graph 59 min
        • Lecture5.2
          Graph Conversion 51 min
        • Lecture5.3
          Area Under Curve 22 min
      • 6.Motion (3) : Two Dimensional Motion
        6
        • Lecture6.1
          Projectile on Level Ground 32 min
        • Lecture6.2
          Terms Related to Projectile on Level Ground 31 min
        • Lecture6.3
          Not Level to Level Projectile, Problem Solving, Dot Product 34 min
        • Lecture6.4
          Equation of Trajectory and Some Miscellaneous Questions 35 min
        • Lecture6.5
          Projectile on Inclined Plane 39 min
        • Lecture6.6
          Collision of Projectile and Avg. Acceleration in 2D Motion 16 min
      • 7.Motion (4) : Relative Motion
        7
        • Lecture7.1
          Reference Frame and Distance of Closest Approach 45 min
        • Lecture7.2
          Relative Motion in 2D 26 min
        • Lecture7.3
          Free Fall & Relative Motion 26 min
        • Lecture7.4
          Throwing Object from Moving Body 32 min
        • Lecture7.5
          Rain Problem (theory)- and Wind in Rain Problem 32 min
        • Lecture7.6
          River Based Problem 26 min
        • Lecture7.7
          Crossing River by Shortest Distance- Least Time to Cross River; Wind Problems; Relative Approach 27 min
      • 8.Newton's Laws of Motion
        8
        • Lecture8.1
          Force and Newton’s Laws 33 min
        • Lecture8.2
          Normal Reaction, Free Body Diagram(F.B.D), Normal on circular bodies, Mass and Weight 57 min
        • Lecture8.3
          Tension Force(Ideal Pulley, Clamp Force), Internal & External Force, Heavy Rope 01 hour
        • Lecture8.4
          Spring Force(Sudden Change, Series and Parallel Cutting of Spring) 01 hour
        • Lecture8.5
          Inertia and Non-Inertial Frames(Pseudo Force), Action-Reactin Pair, Monkey Problem 49 min
        • Lecture8.6
          Chapter Notes – Newton’s Laws of Motion
        • Lecture8.7
          NCERT Solutions – Laws of Motion
        • Lecture8.8
          Revision Notes Laws of Motion
      • 9.Constrain Motion
        3
        • Lecture9.1
          Force of mass-less body; Constrain Motion- Pulley Constrain 1 01 hour
        • Lecture9.2
          Pulley constrain 2, Alternate Method; Wedge Constrain- Proof 49 min
        • Lecture9.3
          Relative Constrain 01 hour
      • 10.Friction
        6
        • Lecture10.1
          Kinetic friction Theory- Theory, Angle of friction 32 min
        • Lecture10.2
          Static Friction Theory- Based on Example 2, Direction of friction Theory 01 min
        • Lecture10.3
          Some Advanced Examples 18 min
        • Lecture10.4
          Block Over Block Theory 01 hour
        • Lecture10.5
          Conveyor belt, Static and kinetic co-eff. of friction, Friction on wheels, Theoretical examples 27 min
        • Lecture10.6
          Chapter Notes – Friction
      • 11.Circular Motion
        6
        • Lecture11.1
          Ex. on Average Acc. and Angular Variables Theory and Ref. Frame 52 min
        • Lecture11.2
          Uniform Circular Motion and Centripetal Force 40 min
        • Lecture11.3
          Non-Uniform Center of Mass – Theory by Ex 2; Friction 01 hour
        • Lecture11.4
          Centrifugal Force and Banking of Roads 01 hour
        • Lecture11.5
          Radius of Curvature- Radius of Curvature; Axial Vector; Well of Death 34 min
        • Lecture11.6
          Chapter Notes – Circular Motion
      • 12.Work Energy Power
        15
        • Lecture12.1
          Work & its calculation and Work-done on curved path 31 min
        • Lecture12.2
          Work-done by Different Forces 01 hour
        • Lecture12.3
          Work Energy Theorem and W.E. th in Non-inertial frame, W.E. th and Time 23 min
        • Lecture12.4
          Work Energy Theorem for System 55 min
        • Lecture12.5
          Energy and Different Forms of Energy-and Energy of Chain; Potential Energy & Reference Frame 28 min
        • Lecture12.6
          Potential Energy Curve and Power 01 hour
        • Lecture12.7
          Normal Reaction, Vertical Circular Motion, Motion in Co-Concentric Spheres 27 min
        • Lecture12.8
          Motion on Outer Surface of Sphere, Motion on Inner Surface of Fixed Sphere 59 min
        • Lecture12.9
          Motion on Rope, Motion on Rod 32 min
        • Lecture12.10
          VCM – 1 31 min
        • Lecture12.11
          VCM – 2 01 hour
        • Lecture12.12
          VCM – 3 22 min
        • Lecture12.13
          Chapter Notes – Work Energy Power
        • Lecture12.14
          NCERT Solutions – Work Energy Power
        • Lecture12.15
          Revision Notes Work Energy Power
      • 13.Momentum
        9
        • Lecture13.1
          Introduction and Conservation of Momentum 35 min
        • Lecture13.2
          Impulsive Force – Characteristics of Impulsive Force 30 min
        • Lecture13.3
          Momentum Conservation in Presence of External Force – Two Steps Problems 41 min
        • Lecture13.4
          Questions Involving Momentum & Work Energy Theorem 27 min
        • Lecture13.5
          Collision – Head – on Collision and Special Cases of Head – on Collision 39 min
        • Lecture13.6
          Oblique Collision 24 min
        • Lecture13.7
          Collision of Ball with Flat Surface 38 min
        • Lecture13.8
          Impulse and Average Force 58 min
        • Lecture13.9
          Advanced Questions 50 min
      • 14.Center of Mass
        5
        • Lecture14.1
          Center of Mass (CM) Frame and Kinetic Energy in C – Frame 29 min
        • Lecture14.2
          Finding Center of Mass by Replacement Method and Finding CM of Plate with Hole 36 min
        • Lecture14.3
          Finding CM by Integration and CM of Some Standard Objects 57 min
        • Lecture14.4
          Motion of CM; Newton’s 2nd Law for CM; CM in Circular Motion 41 min
        • Lecture14.5
          Revision Notes Center of Mass
      • 15.Rotational Motion
        14
        • Lecture15.1
          Rigid Body – Motion of Rigid Body; Axis of Rotation 14 min
        • Lecture15.2
          Vector Product/ Cross Product; Torque 44 min
        • Lecture15.3
          Couple and Principle of Moments 48 min
        • Lecture15.4
          Pseudo Force and Toppling – Overturning of Car 01 hour
        • Lecture15.5
          Moment of Inertia 01 hour
        • Lecture15.6
          Parallel Axis Theorem; Perpendicular Axis Theorem; Quantitative Analysis; Radius of Gyra 01 hour
        • Lecture15.7
          Analogy b/w Transnational & Rotational Motion; Relation b/w Linear and Angular Velocity; Dynamics of Rotation 40 min
        • Lecture15.8
          Angular Momentum 30 min
        • Lecture15.9
          Angular Momentum of a Particle 32 min
        • Lecture15.10
          Rotational Collision 49 min
        • Lecture15.11
          Kinetic Energy, Work, Power; Potential Energy; Linear & Angular Acceleration; Hinge Force; Angular Impulse 02 hour
        • Lecture15.12
          Chapter Notes – Rotational Motion and Rolling Motion
        • Lecture15.13
          NCERT Solutions – Rotational Motion
        • Lecture15.14
          Revision Notes Rotational Motion
      • 16.Rolling Motion
        11
        • Lecture16.1
          Introduction to Rolling Motion 40 min
        • Lecture16.2
          Rolling Motion on Spool 24 min
        • Lecture16.3
          Friction 59 min
        • Lecture16.4
          Direction of Friction 01 hour
        • Lecture16.5
          Rolling on Moving Platform and Motion of Touching Spheres 44 min
        • Lecture16.6
          Rope Based Questions 55 min
        • Lecture16.7
          Work-done by Friction in Rolling Motion, Kinetic Energy in Transnational + Rotational Motion 29 min
        • Lecture16.8
          Angular Momentum in Rotation + Translation 01 hour
        • Lecture16.9
          Angular Collision 01 hour
        • Lecture16.10
          Instantaneous Axis of Rotation 50 min
        • Lecture16.11
          De-Lambart’s Theorem 50 min
      • 17.Gravitation
        8
        • Lecture17.1
          Gravitation force, Universal Law of Gravitation, Gravitational Force due to Hollow Sphere and Solid Sphere 35 min
        • Lecture17.2
          Acceleration due to Gravity and Rotation of Earth 42 min
        • Lecture17.3
          Potential Energy, Questions and Solutions 56 min
        • Lecture17.4
          Satellites, Circular Motion, Geostationary Satellites and Polar Satellites 42 min
        • Lecture17.5
          Polar Satellites, Weightlessness in Satellites, Trajectories and Kepler’s Laws 29 min
        • Lecture17.6
          Chapter Notes – Gravitation
        • Lecture17.7
          NCERT Solutions – Gravitation
        • Lecture17.8
          Revision Notes Gravitation
      • 18.Simple Harmonic Motion
        13
        • Lecture18.1
          Oscillatory Motion – Horizontal Spring Block System, Qualitative Analysis of Horizontal Spring System 33 min
        • Lecture18.2
          Quantitative Analysis of Horizontal Spring System; Frequency and Angular Frequency; Velocity and Acceleration; Mechanical Energy 47 min
        • Lecture18.3
          Relating Uniform Circular Motion and SHM and Phasor Diagram 30 min
        • Lecture18.4
          Equation of SHM and Problem Solving using Phasor Diagram 39 min
        • Lecture18.5
          Questions 40 min
        • Lecture18.6
          More Oscillating Systems – Vertical Spring Block System 41 min
        • Lecture18.7
          Angular Oscillations – Simple Pendulum 34 min
        • Lecture18.8
          Compound / Physical Pendulum, Torsional Pendulum, Equilibrium of Angular SHM; Differentiation by Chain Rule 38 min
        • Lecture18.9
          Energy Method to find Time Period 30 min
        • Lecture18.10
          Finding Amplitude of SHM 30 min
        • Lecture18.11
          Block Over Block and Elastic Rope 33 min
        • Lecture18.12
          Superposition of Horizontal SHMs and Perpendicular 30 min
        • Lecture18.13
          Damped Oscillations 28 min
      • 19.Waves (Part-1)
        11
        • Lecture19.1
          Wave, Plotting and Shifting of Curves, Meaning of y/t and y/x Graph, Wave is an Illusion!, 1D Wave on String 55 min
        • Lecture19.2
          Wave Equation, Analysis of Wave Equation and Wave Velocity 55 min
        • Lecture19.3
          Sinusoidal Wave (Harmonic Wave), Wave Equation for Sinusoidal Wave, Particle Velocity, Slope of Rope, Wave Velocity 01 hour
        • Lecture19.4
          Superposition of Waves 44 min
        • Lecture19.5
          Reflection of Waves 37 min
        • Lecture19.6
          Standing Waves 01 hour
        • Lecture19.7
          Tuning Fork, Sonometer and Equation of Standing Waves 54 min
        • Lecture19.8
          Energy in Waves 54 min
        • Lecture19.9
          Chapter Notes – Waves
        • Lecture19.10
          NCERT Solutions – Waves
        • Lecture19.11
          Revision Notes Waves
      • 20.Waves (Part-2)
        10
        • Lecture20.1
          Waves, Propagation of Sound Wave and Wave Equation 27 min
        • Lecture20.2
          Sound as a Pressure Wave 38 min
        • Lecture20.3
          Speed of Sound, Laplace Correction and Intensity of Sound Waves 59 min
        • Lecture20.4
          Spherical and Cylindrical Sound Waves 31 min
        • Lecture20.5
          Addition of Sin Functions, Interference of Sound Waves of Same Frequency, Interference of Coherent Sources 01 hour
        • Lecture20.6
          Quinke’s Apparatus 32 min
        • Lecture20.7
          Interference of Sound Waves of Slightly Different Frequencies (Beats) 39 min
        • Lecture20.8
          Reflection of Sound Waves, Standing Waves, End Correction 39 min
        • Lecture20.9
          Standing Waves in Terms of Pressure, Standing Waves on Rods, Kund’s Tube, Resonance Tube Experiment 49 min
        • Lecture20.10
          Doppler Effect, Reflection from Wall, Doppler Effect in 2 Dimension 01 hour
      • 21.Mechanical Properties of Solids
        6
        • Lecture21.1
          Rigid body,Strain, Stress,Hook’s Law 25 min
        • Lecture21.2
          Breaking Stress 26 min
        • Lecture21.3
          Shear Stress and Strain, Bulk Modulus, Elasticity and Plasticity, Stress-Strain Curve, Young’s Modulus 34 min
        • Lecture21.4
          Chapter Notes – Mechanical Properties of Solids
        • Lecture21.5
          NCERT Solutions – Mechanical Properties of Solids
        • Lecture21.6
          Revision Notes Mechanical Properties of Solids
      • 22.Thermal Expansion
        5
        • Lecture22.1
          Linear Expansion; Second’s Pendulum; Bimetallic Strip; Expansion of Hole; Thermal Stress 01 hour
        • Lecture22.2
          Areal/Superficial Expansion; Volume Expansion; Thermal Expansion of Liquid; Measurement of Temperature; Anomal 01 hour
        • Lecture22.3
          Arial/Superficial Expansion; Volume Expansion; Thermal Expansion of Liquid; Measurement of Temperature 38 min
        • Lecture22.4
          Chapter Notes – Thermal Expansion
        • Lecture22.5
          NCERT Solutions – Thermal Expansion
      • 23.Heat and Calorimetry
        2
        • Lecture23.1
          Internal Energy; Heat Energy; Thermal Equilibrium; Zeroth Law of Thermodynamics; Specific Heat Capacity; Latent Heat 48 min
        • Lecture23.2
          Mixing of Substances; Water Equivalent; Units; Calorimeter; Melting Point and Boiling Point; Sublimation 01 hour
      • 24.Heat Transfer
        6
        • Lecture24.1
          Conduction; Comparison between Charge Flow & Heat Flow 42 min
        • Lecture24.2
          Equivalent Thermal Conductivity; Heat Transfer and Calorimetry; Use of Integration; Length Variation 44 min
        • Lecture24.3
          Convection; Radiation, Black Body, Prevost Theory, Emissive Power & Emissivity, Kirchoff’s Law, Stefan – Boltzman Law 01 hour
        • Lecture24.4
          Newton’s Law of Cooling, Cooling Curve; Wien’s Displacement Law; Thermo Flask 48 min
        • Lecture24.5
          Chapter Notes – Heat Transfer
        • Lecture24.6
          Revision Notes Heat Transfer
      • 25.Kinetic Theory of Gases
        6
        • Lecture25.1
          Model of Gas,Postulates of Kinetic Theory of Gases, Ideal Gas, Mean free Path, Maxwell’s speed Distribution 37 min
        • Lecture25.2
          Volume, Pressure of Gases, Kinetic Energy, Temperature, Ideal Gas Equation 45 min
        • Lecture25.3
          Gas Laws, Internal energy of Gas, Degree of Freedom, Degree of Freedom of Mono-atomic and Diatomic Gas 56 min
        • Lecture25.4
          Chapter Notes – Kinetic Theory of Gases
        • Lecture25.5
          NCERT Solutions – Kinetic Theory of Gases
        • Lecture25.6
          Revision Notes Kinetic Theory of Gases
      • 26.Thermodynamics
        9
        • Lecture26.1
          State Equation; Thermodynamic Process; Process Equation & Graph; Work done by Gas 01 hour
        • Lecture26.2
          Heat – Work Equivalence; 1st Law of Thermodynamics; Adiabatic Process 57 min
        • Lecture26.3
          Workdone in Adiabatic Process; Specific Molar Heat Capacity 39 min
        • Lecture26.4
          Poly-tropic Process, Bulk Modulus; Free Expansion; Mixture of Gases 54 min
        • Lecture26.5
          Heat Engine, Refrigerator or Heat Pump, Energy Conservation, Kelvin-Plank Statement, Clausius Statement 01 hour
        • Lecture26.6
          Carnot Cycle, Reversible and Irreversible Process, Specific Heat Capacity of Solids and Water 01 hour
        • Lecture26.7
          Chapter Notes – Thermodynamics
        • Lecture26.8
          NCERT Solutions – Thermodynamics
        • Lecture26.9
          Revision Notes Thermodynamics
      • 27.Fluids
        14
        • Lecture27.1
          Introduction, Pressure of Liquid 47 min
        • Lecture27.2
          Manometer, Barometer 41 min
        • Lecture27.3
          Pascal Law, Hydraulic Lift 35 min
        • Lecture27.4
          Accelerated Liquid, Vertical and Horizontal Acceleration, Pressure Variation in Horizontally Accelerated Liquid 57 min
        • Lecture27.5
          Rotating Liquid, Rotating Liquid in U-Tube 28 min
        • Lecture27.6
          Archimedes’ Principle, Hollow Objects 59 min
        • Lecture27.7
          Apparent Weight, Variation of Liquid Force with Height 01 hour
        • Lecture27.8
          Multiple Liquids 34 min
        • Lecture27.9
          Center of Bouyancy 28 min
        • Lecture27.10
          Fluid Dynamics, Equation of Continuity 48 min
        • Lecture27.11
          Magnus Effect 37 min
        • Lecture27.12
          Venturimeter, Pitot Tube 27 min
        • Lecture27.13
          Questions and Solutions 31 min
        • Lecture27.14
          Chapter Notes – Fluids
      • 28.Surface Tension and Viscosity
        6
        • Lecture28.1
          Surface Tension, Surface Energy 52 min
        • Lecture28.2
          Force of Cohesion, Force of Adhesion, Angle of Contact, Radius of Meniscus, Capillary Rise 54 min
        • Lecture28.3
          Pressure Difference Across Meniscus, Variation of Surface tension with Temperature 27 min
        • Lecture28.4
          Viscous Force 35 min
        • Lecture28.5
          Terminal Velocity, Velocity Gradient, Renolds Number, Turbulent Flow, Streamline Flow 41 min
        • Lecture28.6
          Chapter Notes – Surface Tension and Viscosity

        NCERT Solutions – Unit and Measurement

        2.1. 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–1covers ____m in 1 s
        (d) The relative density of lead is 11.3. Its density is ____ g cm–3or ____ kg m–3. 

        Answer

        (a) Length of edge = 1cm = 1/100 m
        Volume of the cube = side3
        Putting the value of side, we get
        Volume of the cube = (1/100 m)3

        The volume of a cube of side 1 cm is equal to 10-6 m3

        (b) Given,
        Radius, r = 2.0 cm = 20 mm (convert cm to mm)
        Height, h = 10.0 cm =100 mm
        The formula of total surface area of a cylinder S = 2πr (r + h)
        Putting the values in this formula, we get
        Surface area of a cylinder S = 2πr (r + h = 2 x 3.14 x 20 (20+100)
        = 15072 = 1.5 × 104 mm2
        The surface area of a solid cylinder of radius 2.0 cm and height 10.0 cm is equal to 1.5 × 104 mm2

        (c) Using the conversion,
        Given,
        Time, t = 1 sec
        speed = 18 km h-1 = 18 km / hour
        1 km = 1000 m and 1hour = 3600 sec
        Speed = 18 × 1000 /3600 sec = 5 m /sec
        Use formula
        Speed = distance / time
        Cross multiply it, we get
        Distance = Speed × Time = 5 × 1 = 5 m
        A vehicle moving with a speed of 18 km h–1covers 5 m in 1 s.

        (d) Density of lead = Relative density of lead × Density of water
        Density of water = 1 g/cm3
        Putting the values, we get
        Density of lead = 11.3 × 1 g/ cm3
        = 11.3 g cm-3
        1 cm = (1/100 m) =10–2 m3
        1 g = 1/1000 kg = 10-3 kg
        Density of lead = 11.3 g cm-3 = 11.3
        Putting the value of 1 cm and 1 gram
        11.3 g/cm3 = 11.3 × 10-3 kg (10-2m)-3 = 11.3 ×10–3 × 106 kg m-3 =1.13 × 103 kg m–3
        The relative density of lead is 11.3. Its density is 11.3 g cm-3 g cm–3 or 1.13 × 103 kg m–3.

        2.2. Fill in the blanks by suitable conversion of units:
        (a) 1 kg m2s–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)3s–2 g–1.

        Answer

        (a) 1 kg = 103 g
        1 m2 = 104 cm2
        1 kg m2 s–2 = 1 kg × 1 m2 × 1 s–2
        =103 g × 104 cm2 × 1 s–2 = 107 g cm2 s–2
        1 kg m2s–2= 107 g cm2 s–2

        (b) Distance = Speed × Time
        Speed of light = 3 × 108 m/s
        Time = 1 year = 365 days = 365 × 24 hours = 365 × 24 × 60 × 60 sec
        Putting these values in above formula we get
        1 light year distance = (3 × 108 m/s) × (365 × 24 × 60 × 60 s) = 9.46 × 1015 m
        9.46 × 1015 m = 1 ly
        So that 1 m = 1/ 9.46 × 1015 ly = 1.06 × 10-16 ly

        (c) 1 hour = 3600 sec so that 1 sec = 1/3600 hour
        1 km = 1000 m so that 1 m = 1/1000 km
        3.0 m s–2 = 3.0 (1/1000 km)( 1/3600 hour)-2 = 3.0 × 10–3 km × ((1/3600)-2 h–2)
        = 3.0 × 10–3 km × (3600)2 h–2 = 3.88 × 104 km h–2
        3.0 m s–2= 3.88 × 104 km h–2

        (d) Given,
        G= 6.67 × 10–11 N m2 (kg)–2
        We know that
        1 N = 1 kg m s–2
        1 kg = 103 g
        1 m = 100 cm = 102 cm
        Putting above values, we get
        6.67 × 10–11 N m2 kg–2 = 6.67 × 10–11 × (1 kg m s–2) (1 m2) (1Kg–2)
        Solve and cancel out the units we get
        ⇒ 6.67 × 10–11 × (1 kg–1 × 1 m3 × 1 s–2)
        Putting above values to convert Kg to g and m to cm
        ⇒ 6.67 × 10–11 × (103 g)-1 × (102 cm)3 × (1 s–2)
        ⇒ 6.67 × 10–11 × 10-3 g-1 × 106 cm3 × (1 s–2)
        ⇒ 6.67 × 10–8 cm3 s–2 g–1
        G= 6.67 × 10–11 N m2 (kg)–2= 6.67 × 10–8 (cm)3s–2 g–1.

        2.3. A calorie is a unit of heat or energy and it equals about 4.2 J where 1J = 1 kg m2s–2. Suppose we employ a system of units in which the unit of mass equals α kg, the unit of length equals β m, the unit of time is γ s. Show that a calorie has a magnitude 4.2 α–1 β–2 γ2 in terms of the new units.

        Answer 

        Given that,
        1 Calorie=4.2 J = 4.2 Kg m2 s-2                …… (i)
        As new unit of mass = α Kg
        ∴ 1 Kg = 1/α new unit of mass
        Similarly, 1 m = β-1 new unit of length
        1 s = γ-1 new unit of time
        Putting these values in (i), we get
        1 calorie = 4.2 (α-1 new unit of mass) (β-1 new unit of length)2 (γ-1 new unit of time)-2
        = 4.2 α-1 β-2 γ2 new unit of energy (Proved)

        2.4. 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
        (b) a jet plane moves with great speed
        (c) the mass of Jupiter is very large
        (d) the air inside this room contains a large number of molecules
        (e) a proton is much more massive than an electron
        (f) the speed of sound is much smaller than the speed of light. 

        Answer

        The given statement is true because a dimensionless quantity may be large or small in comparision to some standard reference. For example, the coefficient of friction is dimensionless. The coefficient of sliding friction is greater than the coefficient of rolling friction, but less than static friction.
        (a) An atom is a very small object in comparison to a soccer ball.
        (b) A jet plane moves with a speed greater than that of a bicycle.
        (c) Mass of Jupiter is very large as compared to the mass of a cricket ball.
        (d) The air inside this room contains a large number of molecules as compared to that present in a geometry box.
        (e) A proton is more massive than an electron.
        (f) Speed of sound is less than the speed of light.

        2.5. 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 min and 20 s to cover this distance?

        Answer

        Distance between the Sun and the Earth = Speed of light x Time taken by light to cover the distance
        Given that in the new unit, speed of light = 1 unit
        Time taken, t = 8 min 20 s = 500 s
        ∴Distance between the Sun and the Earth = 1 x 500 = 500 units 

        2.6. Which of the following is the most precise device for measuring length:
        (a) a vernier callipers with 20 divisions on the sliding scale
        (b) a screw gauge of pitch 1 mm and 100 divisions on the circular scale
        (c) an optical instrument that can measure length to within a wavelength of light?

        Answer
        (a) Least count of this vernier callipers = 1SD – 1 VD  = 1 SD – 19/20 SD = 1/20 SD
        = 1.20 mm = 1/200 cm = 0.005 cm 

        (b) Least count of screw gauge = Pitch/Number of divisions = 1/1000 = 0.001 cm.

        (c) Wavelength of light, λ ≈ 10-5 cm = 0.00001 cm

        Hence, it can be inferred that an optical instrument is the most suitable device to measure length.

        2.7. 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 mm. What is the estimate on the thickness of hair?

        Answer
        Magnification of the microscope = 100
        Average width of the hair in the field of view of the microscope = 3.5 mm
        ∴Actual thickness of the hair is 3.5/100 = 0.035 mm.

        2.8. Answer the following:

        (a) You are given a thread and a metre scale. How will you estimate the diameter of the thread?
        Answer
        Wrap the thread on a uniform smooth rod in such a way that the coils thus formed are very close to each other. Measure the length of the thread using a metre scale. The diameter of the thread is given by the relation,
        Diameter = Length of thread/Number of turns 

        (b) A screw gauge has a pitch of 1.0 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?

        Answer

        It is not possible to increase the accuracy of a screw gauge by increasing the number of divisions of the circular scale. Increasing the number divisions of the circular scale will increase its accuracy to a certain extent only.

        (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?

        Answer

        A set of 100 measurements is more reliable than a set of 5 measurements because random errors involved in the former are very less as compared to the latter.

        2.9. The photograph of a house occupies an area of 1.75 cm2on a 35 mm slide. The slide is projected on to a screen, and the area of the house on the screen is 1.55 m2. What is the linear magnification of the projector-screen arrangement?

        Answer

        Area of the house on the slide = 1.75 cm2
        Area of the image of the house formed on the screen = 1.55 m2 = 1.55 × 104 cm2

        2.10. State the number of significant figures in the following:

        (a) 0.007 m2
        ► 1
        (b) 2.64 x 1024 kg
        ► 3
        (c) 0.2370 g cm-3
        ► 4
        (d) 6.320 J
        ► 4
        (e) 6.032 N m-2
        ► 4
        (f) 0.0006032 m2
        ► 4
        2.11. The length, breadth and thickness of a rectangular sheet of metal are 4.234 m, 1.005 m, and 2.01 cm respectively. Give the area and volume of the sheet to correct significant figures. 

        Answer

        Given that,
        length, l = 4.234 m
        breadth,b = 1.005 m
        thickness, t = 2.01 cm = 2.01 × 10-2 m
        Area of the sheet = 2 (l × 0 + b × t + t × l) = 2 (4.234 × 1.005 + 1.005 × 0.0201 + 0.0201 × 4.234)
        = 2 (4.3604739) = 8.7209478 m2
        As area can contain a maximum of three significant digits, therefore, rounding off, we get
        Area = 8.72 m2
        Also, volume = l × b × t
        V = 4.234 × 1.005 × 0.0201 = 0.0855289 = 0.0855 m3        (Significant Figures = 3)

        2.12. The mass of a box measured by a grocer’s balance is 2.300 kg. Two gold pieces of masses 20.15 g and 20.17 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?

        Answer

        Mass of grocer’s box = 2.300 kg
        Mass of gold piece I = 20.15g = 0.02015 kg
        Mass of gold piece II = 20.17 g = 0.02017 kg

        (a) Total mass of the box = 2.3 + 0.02015 + 0.02017 = 2.34032 kg
        In addition, the final result should retain as many decimal places as there are in the number with the least decimal places. Hence, the total mass of the box is 2.3 kg.

        (b) Difference in masses = 20.17 – 20.15 = 0.02 g
        In subtraction, the final result should retain as many decimal places as there are in the number with the least decimal places.

        2.13. A physical quantity P is related to four observables a, b, c and d as follows:
        The percentage errors of measurement in a, b, c and d are 1%, 3%, 4% and 2%, respectively. What is the percentage error in the quantity P? If the value of P calculated using the above relation turns out to be 3.763, to what value should you round off the result?

        Answer

        Percentage error in P = 13 %
        Value of P is given as 3.763.
        By rounding off the given value to the first decimal place, we get P = 3.8.

        2.14. A book with many printing errors contains four different formulas for the displacement y of a particle undergoing a certain periodic motion:

        (a = maximum displacement of the particle, v = speed of the particle. T = time-period of motion). Rule out the wrong formulas on dimensional grounds.

        Answer

        The displacement y has the dimension of length, therefore, the formula for it should also have the dimension of length. Trigonometric functions are dimensionless and their arguments are also dimensionless. Based on these considerations now check each formula dimensionally.

        The formulas in (ii) and (iii) are dimensionally wrong.
        2.15. A famous relation in physics relates ‘moving mass’ m to the ‘rest mass’ m0 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 = m0 / (1-v2)1/2
        Guess where to put the missing c. 

        Answer

        Given the relation,
        m = m0 / (1-v2)1/2
        Dimension of m = M1 L0 T0
        Dimension of m0 = M1 L0 T0
        Dimension of v = M0 L1 T–1
        Dimension of v2 = M0 L2 T–2
        Dimension of c = M0 L1 T–1
        The given formula will be dimensionally correct only when the dimension of L.H.S is the same as that of R.H.S. This is only possible when the factor, (1-v2)1/2 is dimensionless i.e., (1 – v2) is dimensionless. This is only possible if v2 is divided by c2. Hence, the correct relation is
        m = m0 / (1 – v2/c2)1/2

        2.16. The unit of length convenient on the atomic scale is known as an angstrom and is denoted by Å: 1 Å = 10-10 m. The size of a hydrogen atom is about 0.5 Å. What is the total atomic volume in m3 of a mole of hydrogen atoms ?

        Answer

        Radius of hydrogen atom, r = 0.5 Å = 0.5 × 10-10 m
        Volume of hydrogen atom = (4/3) π r3
        = (4/3) × (22/7) × (0.5 × 10-10)3
        = 0.524 × 10-30 m3
        1 mole of hydrogen contains 6.023 × 1023 hydrogen atoms.
        ∴ Volume of 1 mole of hydrogen atoms = 6.023 × 1023 × 0.524 × 10–30
        = 3.16 × 10–7 m3

        2.17. One mole of an ideal gas at standard temperature and pressure occupies 22.4 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 Å). Why is this ratio so large ?

        Answer

        Radius of hydrogen atom, r = 0.5 Å = 0.5 × 10-10 m
        Volume of hydrogen atom = (4/3) π r3
        = (4/3) × (22/7) × (0.5 × 10-10)3
        = 0.524 × 10-30 m3
        Now, 1 mole of hydrogen contains 6.023 × 1023 hydrogen atoms.
        ∴ Volume of 1 mole of hydrogen atoms, Va = 6.023 × 1023 × 0.524 × 10–30
        = 3.16 × 10–7 m3
        Molar volume of 1 mole of hydrogen atoms at STP,
        Vm = 22.4 L = 22.4 × 10–3 m3

        Hence, the molar volume is 7.08 × 104 times higher than the atomic volume. For this reason, the inter-atomic separation in hydrogen gas is much larger than the size of a hydrogen atom.

        2.18. 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).

        Answer

        Line of sight is defined as an imaginary line joining an object and an observer’s eye. When we observe nearby stationary objects such as trees, houses, etc. while sitting in a moving train, they appear to move rapidly in the opposite direction because the line of sight changes very rapidly.
        On the other hand, distant objects such as trees, stars, etc. appear stationary because of the large distance. As a result, the line of sight does not change its direction rapidly.

        2.19. The principle of ‘parallax’ in section 2.3.1 is used in the determination of distances of very distant stars. The baseline AB is the line joining the Earth’s two locations six months apart in its orbit around the Sun. That is, the baseline is about the diameter of the Earth’s orbit ≈ 3 × 1011 m. However, even the nearest stars are so distant that with such a long baseline, they show parallax only of the order of 1“ (second) of arc or so. A parsec is a convenient unit of length on the astronomical scale. It is the distance of an object that will show a parallax of 1“ (second) of arc from opposite ends of a baseline equal to the distance from the Earth to the Sun. How much is a parsec in terms of meters?

        Answer

        Diameter of Earth’s orbit = 3 × 1011 m
        Radius of Earth’s orbit, r = 1.5 × 1011 m
        Let the distance parallax angle be 1″ = 4.847 × 10–6 rad.
        Let the distance of the star be D.
        Parsec is defined as the distance at which the average radius of the Earth’s orbit subtends an angle of 1″

        = 0.309 × 10-6 ≈ 3.09 × 1016 m
        Hence, 1 parsec ≈ 3.09 × 1016 m

        2.20. The nearest star to our solar system is 4.29 light years away. How much is this distance in terms of parsecs? How much parallax would this star (named Alpha Centauri) show when viewed from two locations of the Earth six months apart in its orbit around the Sun?

        Answer

        Distance of the star from the solar system = 4.29 ly
        1 light year is the distance travelled by light in one year.
        1 light year = Speed of light × 1 year
        = 3 × 108 × 365 × 24 × 60 × 60 = 94608 × 1011 m
        ∴ 4.29 ly = 405868.32 × 1011 m
        ∵ 1 parsec = 3.08 × 1016 m
        ∴ 4.29 ly = 405868.32 × 1011 / 3.08 × 1016  =  1.32 parsec
        Using the relation,
        θ = d / D
        where,
        Diameter of Earth’s orbit, d = 3 × 1011 m
        Distance of the star from the earth, D = 405868.32 × 1011 m
        ∴ θ = 3 × 1011 / 405868.32 × 1011  =  7.39 × 10-6 rad
        But, 1 sec = 4.85 × 10–6 rad
        ∴ 7.39 × 10-6 rad = 7.39 × 10-6 / 4.85 × 10-6 =  1.52“

        2.21. Precise measurements of physical quantities are a need of science. For example, to ascertain the speed of an aircraft, one must have an accurate method to find its positions at closely separated instants of time. This was the actual motivation behind the discovery of radar in World War II. Think of different examples in modern science where precise measurements of length, time, mass etc. are needed. Also, wherever you can, give a quantitative idea of the precision needed.

        Answer

        It is indeed very true that precise measurements of physical quantities are essential for the development of science. For example, ultra-shot laser pulses (time interval ∼ 10–15 s) are used to measure time intervals in several physical and chemical processes.
        X-ray spectroscopy is used to determine the inter-atomic separation or inter-planer spacing.

        The development of mass spectrometer makes it possible to measure the mass of atoms precisely.

        2.22.  Just as precise measurements are necessary in science, it is equally important to be able to make rough estimates of quantities using rudimentary ideas and common observations. Think of ways by which you can estimate the following (where an estimate is difficult to obtain, try to get an upper bound on the quantity):
        (a) the total mass of rain-bearing clouds over India during the Monsoon
        (b) the mass of an elephant
        (c) the wind speed during a storm
        (d) the number of strands of hair on your head
        (e) the number of air molecules in your classroom.

        Answer

        (a) During monsoons, a Metrologist records about 215 cm of rainfall in India i.e., the height of water column, h = 215 cm = 2.15 m
        Area of country, A = 3.3 × 1012 m2
        Hence, volume of rain water, V = A × h = 7.09 × 1012 m3
        Density of water, ρ = 1 × 103 kg m–3
        Hence, mass of rain water = ρ × V = 7.09 × 1015 kg
        Hence, the total mass of rain-bearing clouds over India is approximately 7.09 × 1015 kg.

        (b) Consider a ship of known base area floating in the sea. Measure its depth in sea (say d1).
        Volume of water displaced by the ship, Vb = A d1
        Now, move an elephant on the ship and measure the depth of the ship (d2) in this case.
        Volume of water displaced by the ship with the elephant on board, Vbe= Ad2
        Volume of water displaced by the elephant = Ad2 – Ad1
        Density of water = D
        Mass of elephant = AD (d2 – d1)

        (c) Wind speed during a storm can be measured by an anemometer. As wind blows, it rotates. The rotation made by the anemometer in one second gives the value of wind speed.

        (d) Area of the head surface carrying hair = A
        With the help of a screw gauge, the diameter and hence, the radius of a hair can be determined. Let it be r.
        ∴Area of one hair = πr2
        Number of strands of hair ≈ Total surface area / Area of one hair = A / πr2

         (e) Let the volume of the room be V.
        One mole of air at NTP occupies 22.4 l i.e., 22.4 × 10–3 m3 volume.
        Number of molecules in one mole = 6.023 × 1023
        ∴Number of molecules in room of volume V
        = 6.023 × 1023 × V / 22.4 × 10-3  =  134.915 × 1026 V  =  1.35 × 1028 V

        2.23. The Sun is a hot plasma (ionized matter) with its inner core at a temperature exceeding 107 K, and its outer surface at a temperature of about 6000 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 × 1030 kg, radius of the Sun = 7.0 × 108 m.

        Answer

        Mass of the Sun, M = 2.0 × 1030 kg
        Radius of the Sun, R = 7.0 × 108 m
        Density, ρ = ?

        The density of the Sun is in the density range of solids and liquids. This high density is attributed to the intense gravitational attraction of the inner layers on the outer layer of the Sun.

        2.24. When the planet Jupiter is at a distance of 824.7 million kilometers from the Earth, its angular diameter is measured to be 35.72“ of arc. Calculate the diameter of Jupiter.

        Answer

        Distance of Jupiter from the Earth, D = 824.7 × 106 km = 824.7 × 109 m
        Angular diameter = 35.72“ = 35.72 × 4.874 × 10-6 rad
        Diameter of Jupiter = d
        Using the relation,
        θ = d/ D
        d = θ D = 824.7 × 109 × 35.72 × 4.872 × 10-6
        = 143520.76 × 103 m = 1.435 × 105 Km

        Additional Exercises

        2.25. A man walking briskly in rain with speed v must slant his umbrella forward making an angle θ with the vertical. A student derives the following relation between θ and v : tan θ = v and checks that the relation has a correct limit: as v → 0, θ → 0, as expected. (We are assuming there is no strong wind and that the rain falls vertically for a stationary man). Do you think this relation can be correct ? If not, guess the correct relation.

        Answer

        Incorrect; on dimensional ground
        The relation is tan θ = ν
        Dimension of R.H.S = M0 L1 T–1
        Dimension of L.H.S = M0 L0 T0
        (∵ The trigonometric function is considered to be a dimensionless quantity)
        Dimension of R.H.S is not equal to the dimension of L.H.S. Hence, the given relation is not correct dimensionally.

        To make the given relation correct, the R.H.S should also be dimensionless. One way to achieve this is by dividing the R.H.S by the speed of rainfall ν’
        Therefore, the relation reduces to
        tan θ = ν / ν’
        This relation is dimensionally correct. 

        2.26. It is claimed that two cesium clocks, if allowed to run for 100 years, free from any disturbance, may differ by only about 0.02 s. What does this imply for the accuracy of the standard cesium clock in measuring a time-interval of 1 s?

        Answer

        Error in 100 years = 0.02 s

        Hence, the accuracy of a standard caesium clock in measuring a time interval of 1 s is 10-12 s.

        2.27. Estimate the average mass density of a sodium atom assuming its size to be about 2.5 Å. (Use the known values of Avogadro’s number and the atomic mass of sodium). Compare it with the density of sodium in its crystalline phase : 970 kg m-3. Are the two densities of the same order of magnitude ? If so, why ?

        Answer

        Diameter of sodium atom = Size of sodium atom = 2.5 Å
        Radius of sodium atom, r = (1/2) × 2.5 Å = 1.25 Å = 1.25 × 10-10 m
        Volume of sodium atom, V = (4/3) π r3
        = (4/3) × 3.14 × (1.25 × 10-10)3 = VSodium
        According to the Avogadro hypothesis, one mole of sodium contains 6.023 × 1023 atoms and has a mass of 23 g or 23 × 10–3 kg.
        ∴ Mass of one atom = 23 × 10-3 / 6.023 × 1023  Kg = m1
        Density of sodium atom, ρ = m1 / VSodium
        Substituting the value from above, we get
        Density of sodium atom, ρ =4.67 × 10-3 Kg m-3
        It is given that the density of sodium in crystalline phase is 970 kg m–3.

        Hence, the density of sodium atom and the density of sodium in its crystalline phase are not in the same order. This is because in solid phase, atoms are closely packed. Thus, the inter-atomic separation is very small in the crystalline phase.

        2.28. The unit of length convenient on the nuclear scale is a Fermi : 1 f = 10-15 m. Nuclear sizes obey roughly the following empirical relation :
        r = r0 A1/3
        where r is the radius of the nucleus, A its mass number, and r0 is a constant equal to about, 1.2 f. Show that the rule implies that nuclear mass density is nearly constant for different nuclei. Estimate the mass density of sodium nucleus. Compare it with the average mass density of a sodium atom obtained in Exercise. 2.27.

        Answer

        Radius of nucleus r is given by the relation,
        r = r0 A1/3
        r0 = 1.2 f = 1.2 × 10-15 m
        Volume of nucleus, V = (4 / 3) π r3
        = (4 / 3) π (r0 A1/3)3 = (4 / 3) π r0 A    ….. (i)

        Now, the mass of a nuclei M is equal to its mass number i.e.,
        M = A amu = A × 1.66 × 10–27 kg
        Density of nucleus, ρ = Mass of nucleus / Volume of nucleus
        = A X 1.66 × 10-27 / (4/3) π r03 A

        = 3 X 1.66 × 10-27 / 4 π r03  Kg m-3
        his relation shows that nuclear mass depends only on constant r0. Hence, the nuclear mass densities of all nuclei are nearly the same.
        Density of sodium nucleus is given by,
        ρSodium = 3 × 1.66 × 10-27 / 4 × 3.14 × (1.2 × 10-15)3
        = 4.98 × 1018 / 21.71 = 2.29 × 1017 Kg m-3

        2.29. A LASER is a source of very intense, monochromatic, and unidirectional beam of light. These properties of a laser light can be exploited to measure long distances. The distance of the Moon from the Earth has been already determined very precisely using a laser as a source of light. A laser light beamed at the Moon takes 2.56 s to return after reflection at the Moon’s surface. How much is the radius of the lunar orbit around the Earth?

        Answer

        Time taken by the laser beam to return to Earth after reflection from the Moon = 2.56 s
        Speed of light = 3 × 108 m/s
        Time taken by the laser beam to reach Moon  = 1 / 2 × 2.56 = 1.28 s
        Radius of the lunar orbit = Distance between the Earth and the Moon = 1.28 × 3 × 108 = 3.84 × 108 m = 3.84 × 105 km

        2.30. A SONAR (sound navigation and ranging) uses ultrasonic waves to detect and locate objects under water. In a submarine equipped with a SONAR the time delay between generation of a probe wave and the reception of its echo after reflection from an enemy submarine is found to be 77.0 s. What is the distance of the enemy submarine?
        (Speed of sound in water = 1450 m s-1).

        Answer

        Let the distance between the ship and the enemy submarine be ‘S’.
        Speed of sound in water = 1450 m/s
        Time lag between transmission and reception of Sonar waves = 77 s
        In this time lag, sound waves travel a distance which is twice the distance between the ship and the submarine (2S).
        Time taken for the sound to reach the submarine = 1/2 × 77 = 38.5 s
        ∴ Distance between the ship and the submarine (S) = 1450 × 38.5 = 55825 m = 55.8 km

        2.31. The farthest objects in our Universe discovered by modern astronomers are so distant that light emitted by them takes billions of years to reach the Earth. These objects (known as quasars) have many puzzling features, which have not yet been satisfactorily explained. What is the distance in km of a quasar from which light takes 3.0 billion years to reach us ?

        Answer

        Time taken by quasar light to reach Earth = 3 billion years
        = 3 × 109 years
        = 3 × 109 × 365 × 24 × 60 × 60 s
        Speed of light = 3 × 108 m/s
        Distance between the Earth and quasar
        = (3 × 108) × (3 × 109 × 365 × 24 × 60 × 60)
        = 283824 × 1020 m
        = 2.8 × 1022 km

        2.32. It is a well known fact that during a total solar eclipse the disk of the moon almost completely covers the disk of the Sun. From this fact and from the information you can gather from examples 2.3 and 2.4, determine the approximate diameter of the moon.

        Answer

        The position of the Sun, Moon, and Earth during a lunar eclipse is shown in the given figure.
        Position of sun moon during lunar eclipse
        Distance of the Moon from the Earth = 3.84 × 108 m
        Distance of the Sun from the Earth = 1.496 × 1011 m
        Diameter of the Sun = 1.39 × 109 m

        It can be observed that ΔTRS and ΔTPQ are similar. Hence, it can be written as:
        PQ / RS = VT / UT
        1.39 x 109 / RS = 1.496 × 1011 / 3.84 × 108
        RS = (1.39 × 3.84 / 1.496) × 106 = 3.57 × 106 m
        Hence, the diameter of the Moon is 3.57 × 106 m.

        2.33. A great physicist of this century (P.A.M. Dirac) loved playing with numerical values of Fundamental constants of nature. This led him to an interesting observation. Dirac found that from the basic constants of atomic physics (c, e, mass of electron, mass of proton) and the gravitational constant G, he could arrive at a number with the dimension of time. Further, it was a very large number, its magnitude being close to the present estimate on the age of the universe (~15 billion years). From the table of fundamental constants in this book, try to see if you too can construct this number (or any other interesting number you can think of). If its coincidence with the age of the universe were significant, what would this imply for the constancy of fundamental constants?

        Answer

        One relation consists of some fundamental constants that give the age of the Universe by:

        t = (e2/4πε0)2 × (1 / mpme2 c3G)

        Where,
        t = Age of Universe
        e = Charge of electrons = 1.6 ×10–19 C
        ε0 = Absolute permittivity
        mp = Mass of protons = 1.67 × 10–27 kg
        me = Mass of electrons = 9.1 × 10–31 kg
        c = Speed of light = 3 × 108 m/s
        G = Universal gravitational constant = 6.67 × 1011 Nm2 kg–2
        Also, 1 / 4πε0 = 9 × 109 Nm2/C2
        Substituting these values in the equation, we get
        t = (1.6 × 10-19)4 × (9 × 109)2 / (9.1 × 10-31)2 × 1.67 × 10-27 × (3 × 108)3 × 6.67 × 10-11

        =  [ (1.6)4 × 81 / 9.1 × 1.67 × 27 × 6.67 ] × 10-76+18-62+27-24+11 seconds
        = [(1.6)4 × 81 / 9.1 × 1.67 × 27 × 6.67 × 365 × 24 × 3600 ] × 10-76+18+62+27-24+11 years
        ≈  6 X 10-9 × 1018 years
        = 6 billion years.
        Prev Chapter Notes – Unit and Measurement
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