Chapter 02: Units and Measurements
Physics XI : Complete NCERT Exercise Solutions
Practice the actual NCERT textbook exercises with detailed solutions. These questions are essential for CBSE board exams and form the foundation for competitive exams.
Question 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⁻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) 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.
Answer & Explanation:
(a) 1 cm = 0.01 m
Volume = (side)³ = (0.01 m)³ = 10⁻⁶ m³
(b) Surface area of cylinder = 2πr(h + r)
r = 2.0 cm = 20 mm, h = 10.0 cm = 100 mm
Area = 2π × 20 mm × (100 mm + 20 mm)
= 2π × 20 × 120 mm² = 4800π mm²
≈ 1.5 × 10⁴ mm² (or 15072 mm²)
(c) 18 km h⁻¹ = 18 × (1000 m)/(3600 s) = 5 m s⁻¹
Distance in 1 s = 5 m
(d) Relative density = Density of substance/Density of water
Density of water = 1 g cm⁻³ = 1000 kg m⁻³
Density of lead = 11.3 × 1 g cm⁻³ = 11.3 g cm⁻³
= 11.3 × 1000 kg m⁻³ = 1.13 × 10⁴ kg m⁻³
Volume = (side)³ = (0.01 m)³ = 10⁻⁶ m³
(b) Surface area of cylinder = 2πr(h + r)
r = 2.0 cm = 20 mm, h = 10.0 cm = 100 mm
Area = 2π × 20 mm × (100 mm + 20 mm)
= 2π × 20 × 120 mm² = 4800π mm²
≈ 1.5 × 10⁴ mm² (or 15072 mm²)
(c) 18 km h⁻¹ = 18 × (1000 m)/(3600 s) = 5 m s⁻¹
Distance in 1 s = 5 m
(d) Relative density = Density of substance/Density of water
Density of water = 1 g cm⁻³ = 1000 kg m⁻³
Density of lead = 11.3 × 1 g cm⁻³ = 11.3 g cm⁻³
= 11.3 × 1000 kg m⁻³ = 1.13 × 10⁴ kg m⁻³
Question 2.2
Fill in the blanks by suitable conversion of units:
(a) 1 kg m² s⁻² = ....g cm² s⁻²
(b) 1 m = .... ly (light year)
(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⁻² = ....g cm² s⁻²
(b) 1 m = .... ly (light year)
(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
Answer & Explanation:
(a) 1 kg = 1000 g, 1 m = 100 cm
1 kg m² s⁻² = 1000 g × (100 cm)² × s⁻²
= 1000 × 10000 g cm² s⁻² = 10⁷ g cm² s⁻²
(b) 1 light year = 9.46 × 10¹⁵ m
1 m = 1/(9.46 × 10¹⁵) ly = 1.057 × 10⁻¹⁶ ly
(c) 1 m = 0.001 km, 1 s = 1/3600 h
3.0 m s⁻² = 3.0 × (0.001 km) × (3600 h⁻¹)²
= 3.0 × 0.001 × (3600)² km h⁻²
= 3.0 × 0.001 × 1.296 × 10⁷ km h⁻²
= 3.888 × 10⁴ km h⁻² ≈ 3.9 × 10⁴ km h⁻²
(d) G = 6.67 × 10⁻¹¹ N m² kg⁻²
1 N = 1 kg m s⁻², so G = 6.67 × 10⁻¹¹ m³ kg⁻¹ s⁻²
Convert: 1 m = 100 cm, 1 kg = 1000 g
G = 6.67 × 10⁻¹¹ × (100 cm)³ × (1000 g)⁻¹ × s⁻²
= 6.67 × 10⁻¹¹ × 10⁶ cm³ × 10⁻³ g⁻¹ × s⁻²
= 6.67 × 10⁻⁸ cm³ s⁻² g⁻¹
1 kg m² s⁻² = 1000 g × (100 cm)² × s⁻²
= 1000 × 10000 g cm² s⁻² = 10⁷ g cm² s⁻²
(b) 1 light year = 9.46 × 10¹⁵ m
1 m = 1/(9.46 × 10¹⁵) ly = 1.057 × 10⁻¹⁶ ly
(c) 1 m = 0.001 km, 1 s = 1/3600 h
3.0 m s⁻² = 3.0 × (0.001 km) × (3600 h⁻¹)²
= 3.0 × 0.001 × (3600)² km h⁻²
= 3.0 × 0.001 × 1.296 × 10⁷ km h⁻²
= 3.888 × 10⁴ km h⁻² ≈ 3.9 × 10⁴ km h⁻²
(d) G = 6.67 × 10⁻¹¹ N m² kg⁻²
1 N = 1 kg m s⁻², so G = 6.67 × 10⁻¹¹ m³ kg⁻¹ s⁻²
Convert: 1 m = 100 cm, 1 kg = 1000 g
G = 6.67 × 10⁻¹¹ × (100 cm)³ × (1000 g)⁻¹ × s⁻²
= 6.67 × 10⁻¹¹ × 10⁶ cm³ × 10⁻³ g⁻¹ × s⁻²
= 6.67 × 10⁻⁸ cm³ s⁻² g⁻¹
Question 2.3
A calorie is a unit of heat (energy in transit) and it equals about 4.2 J where 1J = 1 kg m² s⁻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 & Explanation:
Given: 1 cal = 4.2 J = 4.2 kg m² s⁻²
New units:
• Unit of mass = α kg → 1 kg = 1/α new mass unit
• Unit of length = β m → 1 m = 1/β new length unit
• Unit of time = γ s → 1 s = 1/γ new time unit
Conversion:
1 cal = 4.2 kg m² s⁻²
= 4.2 × (1/α new mass unit) × (1/β new length unit)² × (1/γ new time unit)⁻²
= 4.2 × (1/α) × (1/β²) × γ²
= 4.2 α⁻¹ β⁻² γ² in new units
Explanation: The numerical value of a physical quantity changes when units change. Energy has dimensions [M L² T⁻²], so when mass unit increases by factor α, energy value decreases by factor α, etc.
New units:
• Unit of mass = α kg → 1 kg = 1/α new mass unit
• Unit of length = β m → 1 m = 1/β new length unit
• Unit of time = γ s → 1 s = 1/γ new time unit
Conversion:
1 cal = 4.2 kg m² s⁻²
= 4.2 × (1/α new mass unit) × (1/β new length unit)² × (1/γ new time unit)⁻²
= 4.2 × (1/α) × (1/β²) × γ²
= 4.2 α⁻¹ β⁻² γ² in new units
Explanation: The numerical value of a physical quantity changes when units change. Energy has dimensions [M L² T⁻²], so when mass unit increases by factor α, energy value decreases by factor α, etc.
Question 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
(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 & Explanation:
The statement means that quantitative adjectives like 'large', 'small', 'fast', 'slow' are relative terms. They only make sense when compared with some standard reference.
Reframed statements:
(a) Atoms are very small compared to everyday objects like a tennis ball.
(b) A jet plane moves with speed much greater than that of a bicycle.
(c) The mass of Jupiter is very large compared to that of Earth.
(d) The air inside this room contains a large number of molecules compared to the number of people in the room.
(e) OK as stated - it provides direct comparison between proton and electron.
(f) OK as stated - it provides direct comparison between sound and light speeds.
Reframed statements:
(a) Atoms are very small compared to everyday objects like a tennis ball.
(b) A jet plane moves with speed much greater than that of a bicycle.
(c) The mass of Jupiter is very large compared to that of Earth.
(d) The air inside this room contains a large number of molecules compared to the number of people in the room.
(e) OK as stated - it provides direct comparison between proton and electron.
(f) OK as stated - it provides direct comparison between sound and light speeds.
Question 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 & Explanation:
Given: Speed of light in new units = 1 (unity)
Time taken by light = 8 min 20 s = 8 × 60 + 20 = 480 + 20 = 500 s
Distance = Speed × Time
In new units: Speed = 1 new unit of length/new unit of time
But we need to be careful: The new unit of time might be different.
Actually, if speed of light = 1, it means:
1 new length unit / 1 new time unit = c (3 × 10⁸ m/s)
So distance = (speed in new units) × (time in new units)
= 1 × (500 s)/(1 new time unit in seconds)
Simpler approach: In the new system, c = 1, so distance numerically equals time taken by light.
Distance = Time taken by light = 500 (in new units)
Answer: 500 new units
Interpretation: If we define 1 new time unit = 1 second, then 1 new length unit = 3 × 10⁸ m (light travels in 1 s). Then distance = 500 × (3 × 10⁸ m) = 1.5 × 10¹¹ m in SI.
Time taken by light = 8 min 20 s = 8 × 60 + 20 = 480 + 20 = 500 s
Distance = Speed × Time
In new units: Speed = 1 new unit of length/new unit of time
But we need to be careful: The new unit of time might be different.
Actually, if speed of light = 1, it means:
1 new length unit / 1 new time unit = c (3 × 10⁸ m/s)
So distance = (speed in new units) × (time in new units)
= 1 × (500 s)/(1 new time unit in seconds)
Simpler approach: In the new system, c = 1, so distance numerically equals time taken by light.
Distance = Time taken by light = 500 (in new units)
Answer: 500 new units
Interpretation: If we define 1 new time unit = 1 second, then 1 new length unit = 3 × 10⁸ m (light travels in 1 s). Then distance = 500 × (3 × 10⁸ m) = 1.5 × 10¹¹ m in SI.
Question 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?
(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 & Explanation:
Least Count Analysis:
(a) Vernier callipers:
Usually, vernier scale has 10 divisions = 9 main scale divisions
If main scale division = 1 mm, then least count = 1 mm/10 = 0.1 mm = 10⁻⁴ m
With 20 divisions: LC = 1 mm/20 = 0.05 mm = 5 × 10⁻⁵ m
(b) Screw gauge:
Pitch = 1 mm = 10⁻³ m
Divisions = 100
Least count = Pitch/Divisions = 10⁻³ m/100 = 10⁻⁵ m
(c) Optical instrument:
Wavelength of visible light ≈ 400-700 nm = 4-7 × 10⁻⁷ m
Can measure to within a wavelength ≈ 10⁻⁷ m
Comparison:
(a) LC ≈ 5 × 10⁻⁵ m = 50 μm
(b) LC = 10⁻⁵ m = 10 μm
(c) LC ≈ 10⁻⁷ m = 0.1 μm
Most precise: (c) Optical instrument (smallest least count)
Answer: (c)
(a) Vernier callipers:
Usually, vernier scale has 10 divisions = 9 main scale divisions
If main scale division = 1 mm, then least count = 1 mm/10 = 0.1 mm = 10⁻⁴ m
With 20 divisions: LC = 1 mm/20 = 0.05 mm = 5 × 10⁻⁵ m
(b) Screw gauge:
Pitch = 1 mm = 10⁻³ m
Divisions = 100
Least count = Pitch/Divisions = 10⁻³ m/100 = 10⁻⁵ m
(c) Optical instrument:
Wavelength of visible light ≈ 400-700 nm = 4-7 × 10⁻⁷ m
Can measure to within a wavelength ≈ 10⁻⁷ m
Comparison:
(a) LC ≈ 5 × 10⁻⁵ m = 50 μm
(b) LC = 10⁻⁵ m = 10 μm
(c) LC ≈ 10⁻⁷ m = 0.1 μm
Most precise: (c) Optical instrument (smallest least count)
Answer: (c)
Question 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 & Explanation:
Given:
• Magnification = 100
• Observed width in microscope = 3.5 mm (average of 20 observations)
Concept: Magnification = Observed size/Actual size
So, Actual size = Observed size/Magnification
Calculation:
Actual thickness = 3.5 mm / 100 = 0.035 mm
Convert to metres: 0.035 mm = 3.5 × 10⁻⁵ m
Answer: Thickness of hair = 3.5 × 10⁻⁵ m or 0.035 mm
Note: This is reasonable - human hair thickness is typically 0.02-0.04 mm.
• Magnification = 100
• Observed width in microscope = 3.5 mm (average of 20 observations)
Concept: Magnification = Observed size/Actual size
So, Actual size = Observed size/Magnification
Calculation:
Actual thickness = 3.5 mm / 100 = 0.035 mm
Convert to metres: 0.035 mm = 3.5 × 10⁻⁵ m
Answer: Thickness of hair = 3.5 × 10⁻⁵ m or 0.035 mm
Note: This is reasonable - human hair thickness is typically 0.02-0.04 mm.
Question 2.8
Answer the following:
(a) You are given a thread and a metre scale. How will you estimate the diameter of the thread?
(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?
(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?
(a) You are given a thread and a metre scale. How will you estimate the diameter of the thread?
(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?
(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 & Explanation:
(a) Estimating thread diameter with metre scale:
1. Wind the thread closely around a pencil/cylinder for many turns (say n turns)
2. Measure the total length L occupied by n turns using metre scale
3. Diameter d = L/n
4. Repeat for different n values and take average
(b) Increasing divisions on circular scale:
• Least count = Pitch/Number of divisions
• Increasing divisions decreases least count, increasing precision
• However, cannot increase arbitrarily due to:
- Mechanical limitations (smallest readable division)
- Backlash error in screw
- Human eye resolution limit
- Thermal expansion effects
• Practically, beyond certain limit, no improvement in accuracy
(c) 100 vs 5 measurements:
• Random errors tend to cancel out in average of many measurements
• Standard error of mean decreases as 1/√n
• 100 measurements: error reduces by factor 1/√100 = 1/10
• 5 measurements: error reduces by factor 1/√5 ≈ 1/2.24
• More measurements → more reliable mean value
1. Wind the thread closely around a pencil/cylinder for many turns (say n turns)
2. Measure the total length L occupied by n turns using metre scale
3. Diameter d = L/n
4. Repeat for different n values and take average
(b) Increasing divisions on circular scale:
• Least count = Pitch/Number of divisions
• Increasing divisions decreases least count, increasing precision
• However, cannot increase arbitrarily due to:
- Mechanical limitations (smallest readable division)
- Backlash error in screw
- Human eye resolution limit
- Thermal expansion effects
• Practically, beyond certain limit, no improvement in accuracy
(c) 100 vs 5 measurements:
• Random errors tend to cancel out in average of many measurements
• Standard error of mean decreases as 1/√n
• 100 measurements: error reduces by factor 1/√100 = 1/10
• 5 measurements: error reduces by factor 1/√5 ≈ 1/2.24
• More measurements → more reliable mean value
Question 2.9
The photograph of a house occupies an area of 1.75 cm² on 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 & Explanation:
Given:
• Area on slide, A₁ = 1.75 cm² = 1.75 × 10⁻⁴ m²
• Area on screen, A₂ = 1.55 m²
Concept: Area magnification = (Linear magnification)²
Because area ∝ (length)²
Calculation:
Area magnification = A₂/A₁ = 1.55 m² / (1.75 × 10⁻⁴ m²)
= (1.55 × 10⁴)/1.75 = 15500/1.75 ≈ 8857.14
Linear magnification, m = √(Area magnification)
m = √8857.14 ≈ 94.1
Answer: Linear magnification ≈ 94.1
Check: If linear dimensions increase by factor 94.1, area increases by (94.1)² ≈ 8854, consistent with given data.
• Area on slide, A₁ = 1.75 cm² = 1.75 × 10⁻⁴ m²
• Area on screen, A₂ = 1.55 m²
Concept: Area magnification = (Linear magnification)²
Because area ∝ (length)²
Calculation:
Area magnification = A₂/A₁ = 1.55 m² / (1.75 × 10⁻⁴ m²)
= (1.55 × 10⁴)/1.75 = 15500/1.75 ≈ 8857.14
Linear magnification, m = √(Area magnification)
m = √8857.14 ≈ 94.1
Answer: Linear magnification ≈ 94.1
Check: If linear dimensions increase by factor 94.1, area increases by (94.1)² ≈ 8854, consistent with given data.
Question 2.10
State the number of significant figures in the following:
(a) 0.007 m²
(b) 2.64 × 10²⁴ kg
(c) 0.2370 g cm⁻³
(d) 6.320 J
(e) 6.032 N m⁻²
(f) 0.0006032 m²
(a) 0.007 m²
(b) 2.64 × 10²⁴ kg
(c) 0.2370 g cm⁻³
(d) 6.320 J
(e) 6.032 N m⁻²
(f) 0.0006032 m²
Answer & Explanation:
Rules for significant figures:
1. All non-zero digits are significant
2. Leading zeros are not significant
3. Zeros between non-zero digits are significant
4. Trailing zeros in number with decimal point are significant
(a) 0.007 m²: 7 is only significant digit → 1 significant figure
(b) 2.64 × 10²⁴ kg: 2, 6, 4 are significant → 3 significant figures
(c) 0.2370 g cm⁻³: 2, 3, 7, 0 (trailing with decimal) → 4 significant figures
(d) 6.320 J: 6, 3, 2, 0 (trailing with decimal) → 4 significant figures
(e) 6.032 N m⁻²: 6, 0, 3, 2 (zero between non-zero) → 4 significant figures
(f) 0.0006032 m²: 6, 0, 3, 2 (zero between non-zero) → 4 significant figures
Note: Scientific notation makes it clearer: 0.0006032 = 6.032 × 10⁻⁴
1. All non-zero digits are significant
2. Leading zeros are not significant
3. Zeros between non-zero digits are significant
4. Trailing zeros in number with decimal point are significant
(a) 0.007 m²: 7 is only significant digit → 1 significant figure
(b) 2.64 × 10²⁴ kg: 2, 6, 4 are significant → 3 significant figures
(c) 0.2370 g cm⁻³: 2, 3, 7, 0 (trailing with decimal) → 4 significant figures
(d) 6.320 J: 6, 3, 2, 0 (trailing with decimal) → 4 significant figures
(e) 6.032 N m⁻²: 6, 0, 3, 2 (zero between non-zero) → 4 significant figures
(f) 0.0006032 m²: 6, 0, 3, 2 (zero between non-zero) → 4 significant figures
Note: Scientific notation makes it clearer: 0.0006032 = 6.032 × 10⁻⁴
Question 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 & Explanation:
Given:
Length, l = 4.234 m (4 significant figures)
Breadth, b = 1.005 m (4 significant figures)
Thickness, t = 2.01 cm = 0.0201 m (3 significant figures)
(a) Area of sheet:
Area = l × b = 4.234 m × 1.005 m = 4.25517 m²
Significant figures rule for multiplication: Result should have same SF as measurement with least SF.
All have 4 SF, so result should have 4 SF.
Area = 4.255 m² (rounded to 4 SF)
(b) Volume of sheet:
Volume = l × b × t = 4.234 m × 1.005 m × 0.0201 m
= 0.085528917 m³
Thickness has only 3 SF (2.01 cm), so result should have 3 SF.
Volume = 0.0855 m³ or 8.55 × 10⁻² m³ (3 SF)
Alternative: Could also express as 85.5 dm³ or 8.55 × 10⁴ cm³
Length, l = 4.234 m (4 significant figures)
Breadth, b = 1.005 m (4 significant figures)
Thickness, t = 2.01 cm = 0.0201 m (3 significant figures)
(a) Area of sheet:
Area = l × b = 4.234 m × 1.005 m = 4.25517 m²
Significant figures rule for multiplication: Result should have same SF as measurement with least SF.
All have 4 SF, so result should have 4 SF.
Area = 4.255 m² (rounded to 4 SF)
(b) Volume of sheet:
Volume = l × b × t = 4.234 m × 1.005 m × 0.0201 m
= 0.085528917 m³
Thickness has only 3 SF (2.01 cm), so result should have 3 SF.
Volume = 0.0855 m³ or 8.55 × 10⁻² m³ (3 SF)
Alternative: Could also express as 85.5 dm³ or 8.55 × 10⁴ cm³
Question 2.12
The mass of a box measured by a grocer's balance is 2.30 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 & Explanation:
Given:
• Mass of box = 2.30 kg = 2300 g (3 SF)
• Mass of gold piece 1 = 20.15 g (4 SF)
• Mass of gold piece 2 = 20.17 g (4 SF)
(a) Total mass of box with gold pieces:
Convert all to same unit (grams):
Box = 2.30 kg = 2300 g
Gold pieces total = 20.15 g + 20.17 g = 40.32 g
Total mass = 2300 g + 40.32 g = 2340.32 g
Significant figures rule for addition: Result should have decimal places equal to measurement with least decimal places.
• Box: 2300 g (no decimal places, or 0 decimal places)
• Gold total: 40.32 g (2 decimal places)
Least decimal places = 0, so result should have 0 decimal places.
Total mass = 2340 g or 2.34 kg (3 SF)
(b) Difference in masses of pieces:
Difference = 20.17 g - 20.15 g = 0.02 g
Both have 2 decimal places, so difference has 2 decimal places.
Difference = 0.02 g (1 SF actually, but written as 0.02)
Note: In subtraction, number of significant figures can reduce drastically. Here 20.17 - 20.15 = 0.02, which has only 1 SF.
• Mass of box = 2.30 kg = 2300 g (3 SF)
• Mass of gold piece 1 = 20.15 g (4 SF)
• Mass of gold piece 2 = 20.17 g (4 SF)
(a) Total mass of box with gold pieces:
Convert all to same unit (grams):
Box = 2.30 kg = 2300 g
Gold pieces total = 20.15 g + 20.17 g = 40.32 g
Total mass = 2300 g + 40.32 g = 2340.32 g
Significant figures rule for addition: Result should have decimal places equal to measurement with least decimal places.
• Box: 2300 g (no decimal places, or 0 decimal places)
• Gold total: 40.32 g (2 decimal places)
Least decimal places = 0, so result should have 0 decimal places.
Total mass = 2340 g or 2.34 kg (3 SF)
(b) Difference in masses of pieces:
Difference = 20.17 g - 20.15 g = 0.02 g
Both have 2 decimal places, so difference has 2 decimal places.
Difference = 0.02 g (1 SF actually, but written as 0.02)
Note: In subtraction, number of significant figures can reduce drastically. Here 20.17 - 20.15 = 0.02, which has only 1 SF.
Question 2.13
A physical quantity P is related to four observables a, b, c and d as follows:
P = a³b²/(√c d)
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?
P = a³b²/(√c d)
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 & Explanation:
Given: P = a³b²/(√c d) = a³b² c⁻¹/² d⁻¹
Percentage errors: Δa/a = 1%, Δb/b = 3%, Δc/c = 4%, Δd/d = 2%
Error combination formula:
For P = ap bq cr ds:
ΔP/P = |p|(Δa/a) + |q|(Δb/b) + |r|(Δc/c) + |s|(Δd/d)
Here: p = 3, q = 2, r = -1/2, s = -1
ΔP/P = 3(1%) + 2(3%) + |½|(4%) + 1(2%)
= 3% + 6% + 2% + 2% = 13%
Rounding off calculated value:
Calculated P = 3.763
Percentage error = 13%
Absolute error = 3.763 × 0.13 ≈ 0.489
Since error is about 0.5, result should be rounded to:
P = 3.8 (rounded to one decimal place)
Better approach: With 13% error, the first digit (3) is certain, the second digit is uncertain.
So we report: P = 3.8 ± 0.5 or simply P ≈ 3.8
Percentage errors: Δa/a = 1%, Δb/b = 3%, Δc/c = 4%, Δd/d = 2%
Error combination formula:
For P = ap bq cr ds:
ΔP/P = |p|(Δa/a) + |q|(Δb/b) + |r|(Δc/c) + |s|(Δd/d)
Here: p = 3, q = 2, r = -1/2, s = -1
ΔP/P = 3(1%) + 2(3%) + |½|(4%) + 1(2%)
= 3% + 6% + 2% + 2% = 13%
Rounding off calculated value:
Calculated P = 3.763
Percentage error = 13%
Absolute error = 3.763 × 0.13 ≈ 0.489
Since error is about 0.5, result should be rounded to:
P = 3.8 (rounded to one decimal place)
Better approach: With 13% error, the first digit (3) is certain, the second digit is uncertain.
So we report: P = 3.8 ± 0.5 or simply P ≈ 3.8
Question 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) y = a sin(2πt/T)
(b) y = a sin(vt)
(c) y = (a/T) sin(t/a)
(d) y = (a√2)(sin(2πt/T) + cos(2πt/T))
(a = maximum displacement of the particle, v = speed of the particle, T = time-period of motion). Rule out the wrong formulas on dimensional grounds.
(a) y = a sin(2πt/T)
(b) y = a sin(vt)
(c) y = (a/T) sin(t/a)
(d) y = (a√2)(sin(2πt/T) + cos(2πt/T))
(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 & Explanation:
Dimensional analysis:
• Displacement y has dimension [L]
• Amplitude a has dimension [L]
• Time t has dimension [T]
• Time period T has dimension [T]
• Speed v has dimension [L T⁻¹]
• Arguments of sin/cos must be dimensionless
(a) y = a sin(2πt/T):
Argument: 2πt/T → t/T has dimension [T]/[T] = dimensionless ✓
a has dimension [L] → y has dimension [L] ✓
Dimensionally correct
(b) y = a sin(vt):
Argument: vt → [L T⁻¹][T] = [L] → NOT dimensionless ✗
sin() of dimensional quantity is meaningless
Dimensionally wrong
(c) y = (a/T) sin(t/a):
First check argument: t/a → [T]/[L] = [T L⁻¹] → NOT dimensionless ✗
Already wrong, but also a/T has dimension [L]/[T] = [L T⁻¹]
So y would have dimension [L T⁻¹], but should be [L]
Dimensionally wrong
(d) y = (a√2)(sin(2πt/T) + cos(2πt/T)):
Argument: 2πt/T → dimensionless ✓
a√2 has dimension [L] ✓
sin + cos gives dimensionless number ✓
So y has dimension [L] ✓
Dimensionally correct
Correct formulas: (a) and (d)
Wrong formulas: (b) and (c)
• Displacement y has dimension [L]
• Amplitude a has dimension [L]
• Time t has dimension [T]
• Time period T has dimension [T]
• Speed v has dimension [L T⁻¹]
• Arguments of sin/cos must be dimensionless
(a) y = a sin(2πt/T):
Argument: 2πt/T → t/T has dimension [T]/[T] = dimensionless ✓
a has dimension [L] → y has dimension [L] ✓
Dimensionally correct
(b) y = a sin(vt):
Argument: vt → [L T⁻¹][T] = [L] → NOT dimensionless ✗
sin() of dimensional quantity is meaningless
Dimensionally wrong
(c) y = (a/T) sin(t/a):
First check argument: t/a → [T]/[L] = [T L⁻¹] → NOT dimensionless ✗
Already wrong, but also a/T has dimension [L]/[T] = [L T⁻¹]
So y would have dimension [L T⁻¹], but should be [L]
Dimensionally wrong
(d) y = (a√2)(sin(2πt/T) + cos(2πt/T)):
Argument: 2πt/T → dimensionless ✓
a√2 has dimension [L] ✓
sin + cos gives dimensionless number ✓
So y has dimension [L] ✓
Dimensionally correct
Correct formulas: (a) and (d)
Wrong formulas: (b) and (c)
Question 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.
m = m₀/(1 - v²)^{1/2}
Guess where to put the missing c.
Answer & Explanation:
Given incorrect relation: m = m₀/(1 - v²)^{1/2}
Dimensional analysis:
• Left side: m has dimension [M]
• Right side: m₀ has dimension [M]
• Denominator: (1 - v²)^{1/2}
• Problem: v² has dimension [L² T⁻²], but 1 is dimensionless
• Cannot subtract dimensional quantity from dimensionless number
Correction: Need to make v² dimensionless
Divide v² by c² (c = speed of light, dimension [L T⁻¹])
Then v²/c² is dimensionless
Correct relativistic formula:
m = m₀/√(1 - v²/c²) or m = m₀/(1 - v²/c²)^{1/2}
Verification:
• v²/c² has dimension ([L T⁻¹]²)/([L T⁻¹]²) = dimensionless ✓
• 1 - v²/c² is dimensionless ✓
• Square root of dimensionless is dimensionless ✓
• m₀ divided by dimensionless number gives [M] ✓
Answer: The missing c should be in denominator with v: m = m₀/(1 - v²/c²)^{1/2}
Dimensional analysis:
• Left side: m has dimension [M]
• Right side: m₀ has dimension [M]
• Denominator: (1 - v²)^{1/2}
• Problem: v² has dimension [L² T⁻²], but 1 is dimensionless
• Cannot subtract dimensional quantity from dimensionless number
Correction: Need to make v² dimensionless
Divide v² by c² (c = speed of light, dimension [L T⁻¹])
Then v²/c² is dimensionless
Correct relativistic formula:
m = m₀/√(1 - v²/c²) or m = m₀/(1 - v²/c²)^{1/2}
Verification:
• v²/c² has dimension ([L T⁻¹]²)/([L T⁻¹]²) = dimensionless ✓
• 1 - v²/c² is dimensionless ✓
• Square root of dimensionless is dimensionless ✓
• m₀ divided by dimensionless number gives [M] ✓
Answer: The missing c should be in denominator with v: m = m₀/(1 - v²/c²)^{1/2}
Question 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 & Explanation:
Given:
• 1 Å = 10⁻¹⁰ m
• Size of hydrogen atom ≈ radius r = 0.5 Å = 0.5 × 10⁻¹⁰ m = 5 × 10⁻¹¹ m
• 1 mole contains Nₐ = 6.022 × 10²³ atoms (Avogadro's number)
Assuming hydrogen atom as sphere:
Volume of one atom = (4/3)πr³
= (4/3)π(5 × 10⁻¹¹ m)³
= (4/3)π(125 × 10⁻³³ m³)
= (4/3)π × 1.25 × 10⁻³¹ m³
≈ (4/3) × 3.14 × 1.25 × 10⁻³¹ m³
≈ 5.23 × 10⁻³¹ m³
Volume of 1 mole of atoms:
= (Volume of one atom) × Nₐ
= 5.23 × 10⁻³¹ m³ × 6.022 × 10²³
= 3.15 × 10⁻⁷ m³
More precise calculation:
r = 0.5 Å = 5 × 10⁻¹¹ m
Volume per atom = (4/3)πr³ = (4/3)π(5 × 10⁻¹¹)³ = (4/3)π × 125 × 10⁻³³
= (500π/3) × 10⁻³³ ≈ (523.6) × 10⁻³³ = 5.236 × 10⁻³¹ m³
For 1 mole: 5.236 × 10⁻³¹ × 6.022 × 10²³ = 3.154 × 10⁻⁷ m³
Answer: Total atomic volume ≈ 3.15 × 10⁻⁷ m³
• 1 Å = 10⁻¹⁰ m
• Size of hydrogen atom ≈ radius r = 0.5 Å = 0.5 × 10⁻¹⁰ m = 5 × 10⁻¹¹ m
• 1 mole contains Nₐ = 6.022 × 10²³ atoms (Avogadro's number)
Assuming hydrogen atom as sphere:
Volume of one atom = (4/3)πr³
= (4/3)π(5 × 10⁻¹¹ m)³
= (4/3)π(125 × 10⁻³³ m³)
= (4/3)π × 1.25 × 10⁻³¹ m³
≈ (4/3) × 3.14 × 1.25 × 10⁻³¹ m³
≈ 5.23 × 10⁻³¹ m³
Volume of 1 mole of atoms:
= (Volume of one atom) × Nₐ
= 5.23 × 10⁻³¹ m³ × 6.022 × 10²³
= 3.15 × 10⁻⁷ m³
More precise calculation:
r = 0.5 Å = 5 × 10⁻¹¹ m
Volume per atom = (4/3)πr³ = (4/3)π(5 × 10⁻¹¹)³ = (4/3)π × 125 × 10⁻³³
= (500π/3) × 10⁻³³ ≈ (523.6) × 10⁻³³ = 5.236 × 10⁻³¹ m³
For 1 mole: 5.236 × 10⁻³¹ × 6.022 × 10²³ = 3.154 × 10⁻⁷ m³
Answer: Total atomic volume ≈ 3.15 × 10⁻⁷ m³
Question 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 & Explanation:
Given:
• Molar volume of ideal gas at STP = 22.4 L = 22.4 × 10⁻³ m³
• Size of hydrogen molecule ≈ 1 Å diameter → radius r ≈ 0.5 Å = 5 × 10⁻¹¹ m
• From previous question: Atomic volume of 1 mole H atoms ≈ 3.15 × 10⁻⁷ m³
But careful: Hydrogen exists as H₂ molecule, not single atoms.
For H₂ molecule: diameter ≈ 1 Å, radius ≈ 0.5 Å
Volume of one H₂ molecule = (4/3)πr³ ≈ 5.24 × 10⁻³¹ m³ (same as atom)
Volume of 1 mole of H₂ molecules ≈ 3.15 × 10⁻⁷ m³ (same calculation)
Ratio:
Ratio = Molar volume / Atomic (molecular) volume
= (22.4 × 10⁻³ m³) / (3.15 × 10⁻⁷ m³)
= (22.4/3.15) × 10⁴
≈ 7.11 × 10⁴ ≈ 7.1 × 10⁴
Why is this ratio so large?
The ratio is about 71,000! This large ratio indicates:
1. Atoms/molecules are mostly empty space - electrons occupy very little volume
2. In gases, molecules are far apart compared to their sizes
3. Intermolecular distances in gases are much larger than molecular sizes
4. This explains why gases are compressible - there's lots of empty space between molecules
Comparison: For solids/liquids, this ratio would be much smaller (closer to 1).
• Molar volume of ideal gas at STP = 22.4 L = 22.4 × 10⁻³ m³
• Size of hydrogen molecule ≈ 1 Å diameter → radius r ≈ 0.5 Å = 5 × 10⁻¹¹ m
• From previous question: Atomic volume of 1 mole H atoms ≈ 3.15 × 10⁻⁷ m³
But careful: Hydrogen exists as H₂ molecule, not single atoms.
For H₂ molecule: diameter ≈ 1 Å, radius ≈ 0.5 Å
Volume of one H₂ molecule = (4/3)πr³ ≈ 5.24 × 10⁻³¹ m³ (same as atom)
Volume of 1 mole of H₂ molecules ≈ 3.15 × 10⁻⁷ m³ (same calculation)
Ratio:
Ratio = Molar volume / Atomic (molecular) volume
= (22.4 × 10⁻³ m³) / (3.15 × 10⁻⁷ m³)
= (22.4/3.15) × 10⁴
≈ 7.11 × 10⁴ ≈ 7.1 × 10⁴
Why is this ratio so large?
The ratio is about 71,000! This large ratio indicates:
1. Atoms/molecules are mostly empty space - electrons occupy very little volume
2. In gases, molecules are far apart compared to their sizes
3. Intermolecular distances in gases are much larger than molecular sizes
4. This explains why gases are compressible - there's lots of empty space between molecules
Comparison: For solids/liquids, this ratio would be much smaller (closer to 1).
Question 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 & Explanation:
This is due to parallax and angular velocity:
1. For nearby objects (trees, houses):
• They are close to the observer
• As train moves, the line of sight to these objects changes rapidly
• The angular displacement per unit time (angular velocity) is large
• This creates illusion of rapid motion in opposite direction
• Actual effect: You're moving past them quickly
2. For distant objects (hills, Moon, stars):
• They are very far away (effectively at infinity)
• As train moves, the line of sight to these objects changes very little
• The angular displacement is negligible
• They appear almost stationary
• Since they're so far, your motion doesn't significantly change your viewing direction
Mathematical explanation:
Angular velocity ω = v/d, where:
• v = speed of train
• d = distance to object
For nearby objects: d is small → ω is large → rapid apparent motion
For distant objects: d is very large → ω ≈ 0 → no apparent motion
Example:
• Tree 10 m away: ω = (20 m/s)/(10 m) = 2 rad/s → rapid motion
• Moon 384,400 km away: ω = (20 m/s)/(3.844×10⁸ m) ≈ 5×10⁻⁸ rad/s → imperceptible
1. For nearby objects (trees, houses):
• They are close to the observer
• As train moves, the line of sight to these objects changes rapidly
• The angular displacement per unit time (angular velocity) is large
• This creates illusion of rapid motion in opposite direction
• Actual effect: You're moving past them quickly
2. For distant objects (hills, Moon, stars):
• They are very far away (effectively at infinity)
• As train moves, the line of sight to these objects changes very little
• The angular displacement is negligible
• They appear almost stationary
• Since they're so far, your motion doesn't significantly change your viewing direction
Mathematical explanation:
Angular velocity ω = v/d, where:
• v = speed of train
• d = distance to object
For nearby objects: d is small → ω is large → rapid apparent motion
For distant objects: d is very large → ω ≈ 0 → no apparent motion
Example:
• Tree 10 m away: ω = (20 m/s)/(10 m) = 2 rad/s → rapid motion
• Moon 384,400 km away: ω = (20 m/s)/(3.844×10⁸ m) ≈ 5×10⁻⁸ rad/s → imperceptible
Question 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 metres?
Answer & Explanation:
Given:
• Parallax angle θ = 1" (1 arc second)
• Baseline b = distance Earth-Sun = 1 astronomical unit (AU)
• 1 AU ≈ 1.496 × 10¹¹ m
• Distance D = ? (this distance is defined as 1 parsec)
Parallax formula: D = b/θ (θ in radians)
Step 1: Convert 1" to radians
1° = 60' (arc minutes), 1' = 60" (arc seconds)
1° = 3600"
1° = (π/180) rad ≈ 0.0174533 rad
So 1" = (π/180) × (1/3600) rad = π/(180 × 3600) rad
1" = π/648000 rad ≈ 4.848 × 10⁻⁶ rad
Step 2: Calculate distance
D = b/θ = (1.496 × 10¹¹ m) / (4.848 × 10⁻⁶ rad)
= (1.496/4.848) × 10¹¹⁺⁶ m
= 0.3086 × 10¹⁷ m
= 3.086 × 10¹⁶ m
More precisely using exact values:
1" = π/(180 × 3600) rad = π/648000 rad
D = (1.496 × 10¹¹) / (π/648000) = (1.496 × 10¹¹ × 648000)/π
= (1.496 × 6.48 × 10¹⁶)/π (since 10¹¹ × 648000 = 6.48 × 10¹⁶)
= (9.69408 × 10¹⁶)/π
≈ 3.086 × 10¹⁶ m
Answer: 1 parsec ≈ 3.09 × 10¹⁶ m (usually taken as 3.086 × 10¹⁶ m)
• Parallax angle θ = 1" (1 arc second)
• Baseline b = distance Earth-Sun = 1 astronomical unit (AU)
• 1 AU ≈ 1.496 × 10¹¹ m
• Distance D = ? (this distance is defined as 1 parsec)
Parallax formula: D = b/θ (θ in radians)
Step 1: Convert 1" to radians
1° = 60' (arc minutes), 1' = 60" (arc seconds)
1° = 3600"
1° = (π/180) rad ≈ 0.0174533 rad
So 1" = (π/180) × (1/3600) rad = π/(180 × 3600) rad
1" = π/648000 rad ≈ 4.848 × 10⁻⁶ rad
Step 2: Calculate distance
D = b/θ = (1.496 × 10¹¹ m) / (4.848 × 10⁻⁶ rad)
= (1.496/4.848) × 10¹¹⁺⁶ m
= 0.3086 × 10¹⁷ m
= 3.086 × 10¹⁶ m
More precisely using exact values:
1" = π/(180 × 3600) rad = π/648000 rad
D = (1.496 × 10¹¹) / (π/648000) = (1.496 × 10¹¹ × 648000)/π
= (1.496 × 6.48 × 10¹⁶)/π (since 10¹¹ × 648000 = 6.48 × 10¹⁶)
= (9.69408 × 10¹⁶)/π
≈ 3.086 × 10¹⁶ m
Answer: 1 parsec ≈ 3.09 × 10¹⁶ m (usually taken as 3.086 × 10¹⁶ m)
Question 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 & Explanation:
Given:
• Distance to Alpha Centauri = 4.29 light years
• 1 parsec = 3.086 × 10¹⁶ m (from previous question)
• 1 light year = distance light travels in 1 year
= (3 × 10⁸ m/s) × (365.25 × 24 × 3600 s)
≈ 9.46 × 10¹⁵ m
(a) Distance in parsecs:
1 light year = 9.46 × 10¹⁵ m
1 parsec = 3.086 × 10¹⁶ m
So 1 light year = (9.46 × 10¹⁵)/(3.086 × 10¹⁶) parsec
= 0.3066 parsec
Distance in parsecs = 4.29 × 0.3066 ≈ 1.315 parsec
Or more precisely: 4.29 ly × (9.46×10¹⁵ m/ly) ÷ (3.086×10¹⁶ m/parsec)
= (4.29 × 9.46)/3.086 ≈ 40.58/3.086 ≈ 1.315 parsec
(b) Parallax angle:
From definition: Object at 1 parsec shows parallax of 1"
Parallax θ (in arc seconds) = 1/D (in parsecs)
where D is distance in parsecs
For Alpha Centauri: D = 1.315 parsec
θ = 1/1.315 ≈ 0.76" (arc seconds)
Using formula: θ (in radians) = b/D
b = 1 AU = 1.496 × 10¹¹ m
D = 4.29 ly = 4.29 × 9.46 × 10¹⁵ = 4.06 × 10¹⁶ m
θ = (1.496 × 10¹¹)/(4.06 × 10¹⁶) = 3.685 × 10⁻⁶ rad
Convert to arc seconds: 1 rad = (180/π) × 3600" ≈ 206265"
θ = 3.685 × 10⁻⁶ × 206265 ≈ 0.76" ✓
Answer: Distance = 1.315 parsec, Parallax = 0.76"
• Distance to Alpha Centauri = 4.29 light years
• 1 parsec = 3.086 × 10¹⁶ m (from previous question)
• 1 light year = distance light travels in 1 year
= (3 × 10⁸ m/s) × (365.25 × 24 × 3600 s)
≈ 9.46 × 10¹⁵ m
(a) Distance in parsecs:
1 light year = 9.46 × 10¹⁵ m
1 parsec = 3.086 × 10¹⁶ m
So 1 light year = (9.46 × 10¹⁵)/(3.086 × 10¹⁶) parsec
= 0.3066 parsec
Distance in parsecs = 4.29 × 0.3066 ≈ 1.315 parsec
Or more precisely: 4.29 ly × (9.46×10¹⁵ m/ly) ÷ (3.086×10¹⁶ m/parsec)
= (4.29 × 9.46)/3.086 ≈ 40.58/3.086 ≈ 1.315 parsec
(b) Parallax angle:
From definition: Object at 1 parsec shows parallax of 1"
Parallax θ (in arc seconds) = 1/D (in parsecs)
where D is distance in parsecs
For Alpha Centauri: D = 1.315 parsec
θ = 1/1.315 ≈ 0.76" (arc seconds)
Using formula: θ (in radians) = b/D
b = 1 AU = 1.496 × 10¹¹ m
D = 4.29 ly = 4.29 × 9.46 × 10¹⁵ = 4.06 × 10¹⁶ m
θ = (1.496 × 10¹¹)/(4.06 × 10¹⁶) = 3.685 × 10⁻⁶ rad
Convert to arc seconds: 1 rad = (180/π) × 3600" ≈ 206265"
θ = 3.685 × 10⁻⁶ × 206265 ≈ 0.76" ✓
Answer: Distance = 1.315 parsec, Parallax = 0.76"
Question 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 & Explanation:
Examples of precise measurements in modern science:
1. Global Positioning System (GPS):
• Needs precise time measurements
• Satellites have atomic clocks with precision 1 nanosecond (10⁻⁹ s)
• Error of 1 ns in time → 30 cm error in position
• Required precision: ~10⁻⁹ s for centimeter accuracy
2. Gravitational Wave Detection (LIGO):
• Measures length changes due to gravitational waves
• Needs to detect changes of ~10⁻¹⁸ m (1/1000th of proton diameter)
• Arm length 4 km, measures changes smaller than 10⁻¹⁸ m
• Precision: 1 part in 10²¹
3. Atomic Clocks and Time Standards:
• Cesium atomic clocks: precision 1 part in 10¹⁶
• Needed for telecommunications, internet synchronization
• GPS would fail without precise timekeeping
4. Nanotechnology:
• Manipulates atoms and molecules
• Needs length measurements at atomic scale (Ångstrom level)
• Scanning Tunneling Microscope: resolves individual atoms (~10⁻¹⁰ m)
5. Particle Physics (CERN):
• Measures particle masses, energies with extreme precision
• Electron mass known to 10⁻⁸ precision
• Needs precise magnetic field measurements
6. Medical Imaging (MRI):
• Measures magnetic fields with high precision
• Spatial resolution ~1 mm for brain imaging
• Time resolution ~milliseconds for functional MRI
Common theme: Progress in science often depends on improved measurement precision.
1. Global Positioning System (GPS):
• Needs precise time measurements
• Satellites have atomic clocks with precision 1 nanosecond (10⁻⁹ s)
• Error of 1 ns in time → 30 cm error in position
• Required precision: ~10⁻⁹ s for centimeter accuracy
2. Gravitational Wave Detection (LIGO):
• Measures length changes due to gravitational waves
• Needs to detect changes of ~10⁻¹⁸ m (1/1000th of proton diameter)
• Arm length 4 km, measures changes smaller than 10⁻¹⁸ m
• Precision: 1 part in 10²¹
3. Atomic Clocks and Time Standards:
• Cesium atomic clocks: precision 1 part in 10¹⁶
• Needed for telecommunications, internet synchronization
• GPS would fail without precise timekeeping
4. Nanotechnology:
• Manipulates atoms and molecules
• Needs length measurements at atomic scale (Ångstrom level)
• Scanning Tunneling Microscope: resolves individual atoms (~10⁻¹⁰ m)
5. Particle Physics (CERN):
• Measures particle masses, energies with extreme precision
• Electron mass known to 10⁻⁸ precision
• Needs precise magnetic field measurements
6. Medical Imaging (MRI):
• Measures magnetic fields with high precision
• Spatial resolution ~1 mm for brain imaging
• Time resolution ~milliseconds for functional MRI
Common theme: Progress in science often depends on improved measurement precision.
Question 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.
(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 & Explanation:
Estimation techniques:
(a) Mass of rain-bearing clouds over India during Monsoon:
1. Area of India ≈ 3.3 × 10⁶ km² = 3.3 × 10¹² m²
2. Average rainfall during monsoon ≈ 100 cm = 1 m
3. Volume of water = Area × height = 3.3 × 10¹² m³
4. Density of water = 1000 kg/m³
5. Mass of water = 3.3 × 10¹⁵ kg
6. Clouds hold only fraction of this at any time, say 1%
7. Estimated cloud mass ≈ 3 × 10¹³ kg
(b) Mass of an elephant:
1. Approximate as cylinder: height ≈ 3 m, radius ≈ 0.75 m
2. Volume ≈ πr²h = 3.14 × (0.75)² × 3 ≈ 5.3 m³
3. Density ≈ slightly less than water, say 900 kg/m³
4. Mass ≈ 5.3 × 900 ≈ 4800 kg (4-6 tons is reasonable)
(c) Wind speed during a storm:
Use Beaufort scale observations:
• Storm: trees uprooted, structural damage
• Corresponds to 90-120 km/h (25-33 m/s)
• Hurricane: >120 km/h (>33 m/s)
• Estimate: 30 m/s for severe storm
(d) Number of strands of hair on head:
1. Scalp area ≈ 0.1 m² (for adult)
2. Hair density: 100-200 hairs per cm² = 10⁶-2×10⁶ hairs/m²
3. Number = Area × Density = 0.1 × (1.5×10⁶) ≈ 1.5 × 10⁵
4. Estimate: 100,000 to 150,000 hairs
(e) Number of air molecules in classroom:
1. Room dimensions: 10 m × 8 m × 3 m = 240 m³
2. At STP, 1 mole occupies 22.4 L = 0.0224 m³
3. Number of moles = 240/0.0224 ≈ 10,714 moles
4. Avogadro's number = 6.022 × 10²³ molecules/mole
5. Total molecules = 10,714 × 6.022 × 10²³ ≈ 6.5 × 10²⁷
6. Estimate: ~10²⁸ molecules (order of magnitude)
(a) Mass of rain-bearing clouds over India during Monsoon:
1. Area of India ≈ 3.3 × 10⁶ km² = 3.3 × 10¹² m²
2. Average rainfall during monsoon ≈ 100 cm = 1 m
3. Volume of water = Area × height = 3.3 × 10¹² m³
4. Density of water = 1000 kg/m³
5. Mass of water = 3.3 × 10¹⁵ kg
6. Clouds hold only fraction of this at any time, say 1%
7. Estimated cloud mass ≈ 3 × 10¹³ kg
(b) Mass of an elephant:
1. Approximate as cylinder: height ≈ 3 m, radius ≈ 0.75 m
2. Volume ≈ πr²h = 3.14 × (0.75)² × 3 ≈ 5.3 m³
3. Density ≈ slightly less than water, say 900 kg/m³
4. Mass ≈ 5.3 × 900 ≈ 4800 kg (4-6 tons is reasonable)
(c) Wind speed during a storm:
Use Beaufort scale observations:
• Storm: trees uprooted, structural damage
• Corresponds to 90-120 km/h (25-33 m/s)
• Hurricane: >120 km/h (>33 m/s)
• Estimate: 30 m/s for severe storm
(d) Number of strands of hair on head:
1. Scalp area ≈ 0.1 m² (for adult)
2. Hair density: 100-200 hairs per cm² = 10⁶-2×10⁶ hairs/m²
3. Number = Area × Density = 0.1 × (1.5×10⁶) ≈ 1.5 × 10⁵
4. Estimate: 100,000 to 150,000 hairs
(e) Number of air molecules in classroom:
1. Room dimensions: 10 m × 8 m × 3 m = 240 m³
2. At STP, 1 mole occupies 22.4 L = 0.0224 m³
3. Number of moles = 240/0.0224 ≈ 10,714 moles
4. Avogadro's number = 6.022 × 10²³ molecules/mole
5. Total molecules = 10,714 × 6.022 × 10²³ ≈ 6.5 × 10²⁷
6. Estimate: ~10²⁸ molecules (order of magnitude)
Question 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 & Explanation:
Reasoning before calculation:
• Sun is plasma (ionized gas), but under enormous gravitational pressure
• Core density should be much higher than ordinary gases
• But still less than solids/liquids on Earth
• Expected: Between gas and solid densities
• Typical solids: 10³ kg/m³ (water 1000, iron 7800)
• Typical gases at STP: ~1 kg/m³
• Sun's average density likely ~10³-10⁴ kg/m³
Calculation:
Mass, M = 2.0 × 10³⁰ kg
Radius, R = 7.0 × 10⁸ m
Volume of sphere = (4/3)πR³
= (4/3)π(7.0 × 10⁸)³ = (4/3)π × 343 × 10²⁴
≈ (4/3) × 3.14 × 343 × 10²⁴
≈ 1.44 × 10²⁷ m³
Density ρ = M/V = (2.0 × 10³⁰)/(1.44 × 10²⁷)
= (2.0/1.44) × 10³ = 1.39 × 10³ kg/m³
Result: ρ ≈ 1400 kg/m³
Comparison:
• Water: 1000 kg/m³
• Earth's average density: 5500 kg/m³
• Iron: 7800 kg/m³
• Air at STP: 1.2 kg/m³
Sun's density (1400 kg/m³) is:
• Higher than gases (by factor ~1000)
• Similar to liquids (slightly denser than water)
• Lower than most solids
Correct guess: Between gas and solid densities
• Sun is plasma (ionized gas), but under enormous gravitational pressure
• Core density should be much higher than ordinary gases
• But still less than solids/liquids on Earth
• Expected: Between gas and solid densities
• Typical solids: 10³ kg/m³ (water 1000, iron 7800)
• Typical gases at STP: ~1 kg/m³
• Sun's average density likely ~10³-10⁴ kg/m³
Calculation:
Mass, M = 2.0 × 10³⁰ kg
Radius, R = 7.0 × 10⁸ m
Volume of sphere = (4/3)πR³
= (4/3)π(7.0 × 10⁸)³ = (4/3)π × 343 × 10²⁴
≈ (4/3) × 3.14 × 343 × 10²⁴
≈ 1.44 × 10²⁷ m³
Density ρ = M/V = (2.0 × 10³⁰)/(1.44 × 10²⁷)
= (2.0/1.44) × 10³ = 1.39 × 10³ kg/m³
Result: ρ ≈ 1400 kg/m³
Comparison:
• Water: 1000 kg/m³
• Earth's average density: 5500 kg/m³
• Iron: 7800 kg/m³
• Air at STP: 1.2 kg/m³
Sun's density (1400 kg/m³) is:
• Higher than gases (by factor ~1000)
• Similar to liquids (slightly denser than water)
• Lower than most solids
Correct guess: Between gas and solid densities
Question 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 & Explanation:
Given:
• Distance to Jupiter, D = 824.7 million km = 8.247 × 10⁸ km
• Angular diameter, θ = 35.72" (arc seconds)
• Need: Linear diameter, d
Formula: For small angles, d = D × θ (θ in radians)
Step 1: Convert θ to radians
1" = π/(180 × 3600) rad ≈ 4.848 × 10⁻⁶ rad
θ = 35.72" = 35.72 × 4.848 × 10⁻⁶ rad
= 35.72 × 4.848 × 10⁻⁶ = 173.2 × 10⁻⁶ rad
= 1.732 × 10⁻⁴ rad
Step 2: Calculate diameter
d = D × θ = (8.247 × 10⁸ km) × (1.732 × 10⁻⁴)
= (8.247 × 1.732) × 10⁴ km
= 14.28 × 10⁴ km = 1.428 × 10⁵ km
More precise calculation:
θ in rad = 35.72 × (π/648000) = 35.72π/648000
d = (8.247 × 10⁸) × (35.72π/648000) km
= (8.247 × 10⁸ × 35.72 × π)/(648000) km
Numerator: 8.247 × 10⁸ × 35.72 × 3.1416 ≈ 9.25 × 10¹⁰
d ≈ 9.25 × 10¹⁰/6.48 × 10⁵ = 1.427 × 10⁵ km
Answer: Diameter of Jupiter ≈ 1.43 × 10⁵ km
(Actual value: 1.43 × 10⁵ km, so our calculation is accurate)
• Distance to Jupiter, D = 824.7 million km = 8.247 × 10⁸ km
• Angular diameter, θ = 35.72" (arc seconds)
• Need: Linear diameter, d
Formula: For small angles, d = D × θ (θ in radians)
Step 1: Convert θ to radians
1" = π/(180 × 3600) rad ≈ 4.848 × 10⁻⁶ rad
θ = 35.72" = 35.72 × 4.848 × 10⁻⁶ rad
= 35.72 × 4.848 × 10⁻⁶ = 173.2 × 10⁻⁶ rad
= 1.732 × 10⁻⁴ rad
Step 2: Calculate diameter
d = D × θ = (8.247 × 10⁸ km) × (1.732 × 10⁻⁴)
= (8.247 × 1.732) × 10⁴ km
= 14.28 × 10⁴ km = 1.428 × 10⁵ km
More precise calculation:
θ in rad = 35.72 × (π/648000) = 35.72π/648000
d = (8.247 × 10⁸) × (35.72π/648000) km
= (8.247 × 10⁸ × 35.72 × π)/(648000) km
Numerator: 8.247 × 10⁸ × 35.72 × 3.1416 ≈ 9.25 × 10¹⁰
d ≈ 9.25 × 10¹⁰/6.48 × 10⁵ = 1.427 × 10⁵ km
Answer: Diameter of Jupiter ≈ 1.43 × 10⁵ km
(Actual value: 1.43 × 10⁵ km, so our calculation is accurate)
Question 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 & Explanation:
Analysis of given relation: tan θ = v
• Left side: tan θ is dimensionless (ratio of lengths)
• Right side: v has dimensions [L T⁻¹]
• Dimensions don't match → relation is wrong
Correct approach:
Consider relative velocity of rain with respect to man.
Let:
• vr = velocity of rain (vertical, downward)
• vm = velocity of man (horizontal)
• Relative velocity of rain w.r.t. man = vr - vm
This has both vertical and horizontal components.
To avoid getting wet, umbrella should be tilted along relative velocity direction.
From vector diagram:
tan θ = (horizontal component)/(vertical component)
= vm/vr
Correct relation: tan θ = v/vr
where v is man's speed, vr is rain's speed
Dimensional check:
• Left: tan θ dimensionless
• Right: v/vr → [L T⁻¹]/[L T⁻¹] = dimensionless ✓
Physical check:
• If v = 0 (stationary), θ = 0 (umbrella vertical) ✓
• If v increases, θ increases ✓
• If vr is large (heavy rain), θ is small ✓
• Left side: tan θ is dimensionless (ratio of lengths)
• Right side: v has dimensions [L T⁻¹]
• Dimensions don't match → relation is wrong
Correct approach:
Consider relative velocity of rain with respect to man.
Let:
• vr = velocity of rain (vertical, downward)
• vm = velocity of man (horizontal)
• Relative velocity of rain w.r.t. man = vr - vm
This has both vertical and horizontal components.
To avoid getting wet, umbrella should be tilted along relative velocity direction.
From vector diagram:
tan θ = (horizontal component)/(vertical component)
= vm/vr
Correct relation: tan θ = v/vr
where v is man's speed, vr is rain's speed
Dimensional check:
• Left: tan θ dimensionless
• Right: v/vr → [L T⁻¹]/[L T⁻¹] = dimensionless ✓
Physical check:
• If v = 0 (stationary), θ = 0 (umbrella vertical) ✓
• If v increases, θ increases ✓
• If vr is large (heavy rain), θ is small ✓
Question 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 & Explanation:
Given:
• Two cesium clocks differ by 0.02 s in 100 years
• Need: Accuracy for 1 s measurement
Step 1: Convert 100 years to seconds
1 year = 365.25 days (accounting for leap years)
1 day = 24 × 3600 = 86400 s
100 years = 100 × 365.25 × 86400 s
= 100 × 3.15576 × 10⁷ s (since 365.25×86400 = 3.15576×10⁷)
= 3.15576 × 10⁹ s
Step 2: Calculate relative error
Difference in 100 years = 0.02 s
Relative error = (0.02 s)/(3.15576 × 10⁹ s)
= 0.02/3.15576 × 10⁻⁹
≈ 6.34 × 10⁻¹²
This means accuracy is about 1 part in 10¹¹ to 10¹²
Step 3: Error in 1 s measurement
Error in 1 s = 1 s × relative error
= 1 × 6.34 × 10⁻¹² s
≈ 6 × 10⁻¹² s
Interpretation:
• Cesium clock can measure 1 s with accuracy ~10⁻¹¹ to 10⁻¹²
• This is incredibly precise
• Corresponds to losing/gaining 1 second in ~30,000 to 300,000 years
Note: Modern cesium clocks are even better (~10⁻¹⁵ accuracy)
• Two cesium clocks differ by 0.02 s in 100 years
• Need: Accuracy for 1 s measurement
Step 1: Convert 100 years to seconds
1 year = 365.25 days (accounting for leap years)
1 day = 24 × 3600 = 86400 s
100 years = 100 × 365.25 × 86400 s
= 100 × 3.15576 × 10⁷ s (since 365.25×86400 = 3.15576×10⁷)
= 3.15576 × 10⁹ s
Step 2: Calculate relative error
Difference in 100 years = 0.02 s
Relative error = (0.02 s)/(3.15576 × 10⁹ s)
= 0.02/3.15576 × 10⁻⁹
≈ 6.34 × 10⁻¹²
This means accuracy is about 1 part in 10¹¹ to 10¹²
Step 3: Error in 1 s measurement
Error in 1 s = 1 s × relative error
= 1 × 6.34 × 10⁻¹² s
≈ 6 × 10⁻¹² s
Interpretation:
• Cesium clock can measure 1 s with accuracy ~10⁻¹¹ to 10⁻¹²
• This is incredibly precise
• Corresponds to losing/gaining 1 second in ~30,000 to 300,000 years
Note: Modern cesium clocks are even better (~10⁻¹⁵ accuracy)
Question 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 mass 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 & Explanation:
Given:
• Size of sodium atom ≈ 2.5 Å (diameter)
• Radius r = 2.5/2 = 1.25 Å = 1.25 × 10⁻¹⁰ m
• Atomic mass of sodium = 23 g/mol = 0.023 kg/mol
• Avogadro's number Nₐ = 6.022 × 10²³ atoms/mol
Step 1: Mass of one sodium atom
Mass per atom = Atomic mass/Nₐ
= 0.023 kg/mol ÷ 6.022 × 10²³ atoms/mol
= 3.82 × 10⁻²⁶ kg
Step 2: Volume of one atom
Assuming spherical atom:
Volume = (4/3)πr³ = (4/3)π(1.25 × 10⁻¹⁰)³
= (4/3)π × 1.953 × 10⁻³⁰ m³
≈ (4/3) × 3.14 × 1.953 × 10⁻³⁰
≈ 8.18 × 10⁻³⁰ m³
Step 3: Density of single atom
Density = Mass/Volume = (3.82 × 10⁻²⁶)/(8.18 × 10⁻³⁰)
= 4.67 × 10³ kg/m³ ≈ 4670 kg/m³
Step 4: Comparison with crystalline sodium
• Atomic density (calculated): ~4700 kg/m³
• Crystalline sodium density: 970 kg/m³
Order of magnitude:
4700 kg/m³ → order 10³
970 kg/m³ → order 10³
Both are order 10³ kg/m³ ✓
Why similar order of magnitude?
• In solids, atoms are closely packed
• Volume occupied by atoms ≈ total volume (little empty space)
• Packing efficiency for closest packing: ~74%
• So solid density ≈ 0.74 × atomic density
• 0.74 × 4700 ≈ 3480 kg/m³ (but sodium has BCC structure, packing ~68%)
• Our atomic density calculation assumed solid sphere, but atoms have electron clouds
Actually, crystalline density should be LOWER because:
1. Atoms not perfectly spherical
2. Electron clouds overlap
3. Crystal structure has empty spaces
But same order of magnitude is reasonable.
• Size of sodium atom ≈ 2.5 Å (diameter)
• Radius r = 2.5/2 = 1.25 Å = 1.25 × 10⁻¹⁰ m
• Atomic mass of sodium = 23 g/mol = 0.023 kg/mol
• Avogadro's number Nₐ = 6.022 × 10²³ atoms/mol
Step 1: Mass of one sodium atom
Mass per atom = Atomic mass/Nₐ
= 0.023 kg/mol ÷ 6.022 × 10²³ atoms/mol
= 3.82 × 10⁻²⁶ kg
Step 2: Volume of one atom
Assuming spherical atom:
Volume = (4/3)πr³ = (4/3)π(1.25 × 10⁻¹⁰)³
= (4/3)π × 1.953 × 10⁻³⁰ m³
≈ (4/3) × 3.14 × 1.953 × 10⁻³⁰
≈ 8.18 × 10⁻³⁰ m³
Step 3: Density of single atom
Density = Mass/Volume = (3.82 × 10⁻²⁶)/(8.18 × 10⁻³⁰)
= 4.67 × 10³ kg/m³ ≈ 4670 kg/m³
Step 4: Comparison with crystalline sodium
• Atomic density (calculated): ~4700 kg/m³
• Crystalline sodium density: 970 kg/m³
Order of magnitude:
4700 kg/m³ → order 10³
970 kg/m³ → order 10³
Both are order 10³ kg/m³ ✓
Why similar order of magnitude?
• In solids, atoms are closely packed
• Volume occupied by atoms ≈ total volume (little empty space)
• Packing efficiency for closest packing: ~74%
• So solid density ≈ 0.74 × atomic density
• 0.74 × 4700 ≈ 3480 kg/m³ (but sodium has BCC structure, packing ~68%)
• Our atomic density calculation assumed solid sphere, but atoms have electron clouds
Actually, crystalline density should be LOWER because:
1. Atoms not perfectly spherical
2. Electron clouds overlap
3. Crystal structure has empty spaces
But same order of magnitude is reasonable.
Question 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 = r₀A¹/³
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.
r = r₀A¹/³
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 & Explanation:
Given: r = r₀A¹/³, with r₀ ≈ 1.2 f = 1.2 × 10⁻¹⁵ m
Part 1: Show nuclear mass density is constant
Mass of nucleus ≈ A × mₚ (where mₚ ≈ mass of proton)
Actually, mass ≈ A × u, where u = atomic mass unit
Volume of nucleus (sphere) = (4/3)πr³ = (4/3)π(r₀A¹/³)³
= (4/3)πr₀³A
Density ρ = Mass/Volume = (A × u)/[(4/3)πr₀³A]
= u/[(4/3)πr₀³]
Notice A cancels out! So:
ρ = constant (independent of A)
= u/[(4/3)πr₀³]
This shows nuclear density is approximately constant for all nuclei.
Part 2: Estimate density of sodium nucleus
For sodium: A = 23 (most common isotope)
r = r₀A¹/³ = 1.2 × 10⁻¹⁵ × (23)¹/³ m
(23)¹/³ ≈ 2.84 (since 2.8³ = 21.95, 2.85³ = 23.15)
r ≈ 1.2 × 2.84 × 10⁻¹⁵ = 3.41 × 10⁻¹⁵ m
Mass = A × u = 23 × 1.66 × 10⁻²⁷ kg = 3.818 × 10⁻²⁶ kg
Volume = (4/3)πr³ = (4/3)π(3.41 × 10⁻¹⁵)³
= (4/3)π × 3.96 × 10⁻⁴⁴ ≈ 1.66 × 10⁻⁴³ m³
Density ρ = (3.818 × 10⁻²⁶)/(1.66 × 10⁻⁴³)
= 2.30 × 10¹⁷ kg/m³
Using constant density formula:
ρ = u/[(4/3)πr₀³] = (1.66 × 10⁻²⁷)/[(4/3)π(1.2×10⁻¹⁵)³]
= (1.66 × 10⁻²⁷)/[ (4/3)π × 1.728 × 10⁻⁴⁵]
= (1.66 × 10⁻²⁷)/(7.24 × 10⁻⁴⁵)
≈ 2.29 × 10¹⁷ kg/m³ ✓
Part 3: Comparison with atomic density (from 2.27)
• Nuclear density: ~2.3 × 10¹⁷ kg/m³
• Atomic density: ~4.7 × 10³ kg/m³
Ratio = (2.3 × 10¹⁷)/(4.7 × 10³) ≈ 4.9 × 10¹³
Nuclear density is ~10¹⁴ times larger!
This shows atom is mostly empty space - mass concentrated in tiny nucleus.
Part 1: Show nuclear mass density is constant
Mass of nucleus ≈ A × mₚ (where mₚ ≈ mass of proton)
Actually, mass ≈ A × u, where u = atomic mass unit
Volume of nucleus (sphere) = (4/3)πr³ = (4/3)π(r₀A¹/³)³
= (4/3)πr₀³A
Density ρ = Mass/Volume = (A × u)/[(4/3)πr₀³A]
= u/[(4/3)πr₀³]
Notice A cancels out! So:
ρ = constant (independent of A)
= u/[(4/3)πr₀³]
This shows nuclear density is approximately constant for all nuclei.
Part 2: Estimate density of sodium nucleus
For sodium: A = 23 (most common isotope)
r = r₀A¹/³ = 1.2 × 10⁻¹⁵ × (23)¹/³ m
(23)¹/³ ≈ 2.84 (since 2.8³ = 21.95, 2.85³ = 23.15)
r ≈ 1.2 × 2.84 × 10⁻¹⁵ = 3.41 × 10⁻¹⁵ m
Mass = A × u = 23 × 1.66 × 10⁻²⁷ kg = 3.818 × 10⁻²⁶ kg
Volume = (4/3)πr³ = (4/3)π(3.41 × 10⁻¹⁵)³
= (4/3)π × 3.96 × 10⁻⁴⁴ ≈ 1.66 × 10⁻⁴³ m³
Density ρ = (3.818 × 10⁻²⁶)/(1.66 × 10⁻⁴³)
= 2.30 × 10¹⁷ kg/m³
Using constant density formula:
ρ = u/[(4/3)πr₀³] = (1.66 × 10⁻²⁷)/[(4/3)π(1.2×10⁻¹⁵)³]
= (1.66 × 10⁻²⁷)/[ (4/3)π × 1.728 × 10⁻⁴⁵]
= (1.66 × 10⁻²⁷)/(7.24 × 10⁻⁴⁵)
≈ 2.29 × 10¹⁷ kg/m³ ✓
Part 3: Comparison with atomic density (from 2.27)
• Nuclear density: ~2.3 × 10¹⁷ kg/m³
• Atomic density: ~4.7 × 10³ kg/m³
Ratio = (2.3 × 10¹⁷)/(4.7 × 10³) ≈ 4.9 × 10¹³
Nuclear density is ~10¹⁴ times larger!
This shows atom is mostly empty space - mass concentrated in tiny nucleus.
Question 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 & Explanation:
Given:
• Time for laser to go to Moon and back = 2.56 s
• Speed of light, c = 3 × 10⁸ m/s (standard value)
Step 1: Time for one-way trip
Time to reach Moon = Total time/2 = 2.56 s/2 = 1.28 s
Step 2: Distance to Moon
Distance = Speed × Time = c × t
= 3 × 10⁸ m/s × 1.28 s
= 3.84 × 10⁸ m
Step 3: Radius of lunar orbit
This distance is approximately the radius of Moon's orbit around Earth
(Strictly, it's distance between centers, but Moon's radius ~1.74×10⁶ m is negligible compared to 3.84×10⁸ m)
Answer: Radius ≈ 3.84 × 10⁸ m
Note: This is average distance. Actual distance varies due to elliptical orbit (3.63×10⁸ m to 4.06×10⁸ m).
• Time for laser to go to Moon and back = 2.56 s
• Speed of light, c = 3 × 10⁸ m/s (standard value)
Step 1: Time for one-way trip
Time to reach Moon = Total time/2 = 2.56 s/2 = 1.28 s
Step 2: Distance to Moon
Distance = Speed × Time = c × t
= 3 × 10⁸ m/s × 1.28 s
= 3.84 × 10⁸ m
Step 3: Radius of lunar orbit
This distance is approximately the radius of Moon's orbit around Earth
(Strictly, it's distance between centers, but Moon's radius ~1.74×10⁶ m is negligible compared to 3.84×10⁸ m)
Answer: Radius ≈ 3.84 × 10⁸ m
Note: This is average distance. Actual distance varies due to elliptical orbit (3.63×10⁸ m to 4.06×10⁸ m).
Question 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 & Explanation:
Given:
• Time delay (to target and back) = 77.0 s
• Speed of sound in water, v = 1450 m/s
Step 1: Time for one-way trip
Time to reach enemy sub = Total time/2 = 77.0 s/2 = 38.5 s
Step 2: Distance to enemy submarine
Distance = Speed × Time = v × t
= 1450 m/s × 38.5 s
= 1450 × 38.5 = 55825 m
Convert to km: 55825 m = 55.825 km
With significant figures:
Time has 3 SF (77.0), speed has 3 SF (1450)
Result should have 3 SF: 55.8 km or 5.58 × 10⁴ m
Answer: Distance ≈ 55.8 km
• Time delay (to target and back) = 77.0 s
• Speed of sound in water, v = 1450 m/s
Step 1: Time for one-way trip
Time to reach enemy sub = Total time/2 = 77.0 s/2 = 38.5 s
Step 2: Distance to enemy submarine
Distance = Speed × Time = v × t
= 1450 m/s × 38.5 s
= 1450 × 38.5 = 55825 m
Convert to km: 55825 m = 55.825 km
With significant figures:
Time has 3 SF (77.0), speed has 3 SF (1450)
Result should have 3 SF: 55.8 km or 5.58 × 10⁴ m
Answer: Distance ≈ 55.8 km
Question 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 & Explanation:
Given:
• Time taken by light = 3.0 billion years = 3.0 × 10⁹ years
• Speed of light, c = 3 × 10⁸ m/s = 3 × 10⁵ km/s
Step 1: Convert years to seconds
1 year = 365.25 days × 24 h/day × 3600 s/h
= 365.25 × 86400 s = 3.15576 × 10⁷ s
3.0 × 10⁹ years = 3.0 × 10⁹ × 3.15576 × 10⁷ s
= 9.46728 × 10¹⁶ s ≈ 9.47 × 10¹⁶ s
Step 2: Calculate distance
Distance = Speed × Time = c × t
= 3 × 10⁸ m/s × 9.47 × 10¹⁶ s
= 2.841 × 10²⁵ m
Convert to km: 2.841 × 10²⁵ m = 2.841 × 10²² km
Using light years:
1 light year = distance light travels in 1 year ≈ 9.46 × 10¹² km
Distance = 3.0 × 10⁹ light years
In km = 3.0 × 10⁹ × 9.46 × 10¹² = 2.84 × 10²² km
Answer: Distance ≈ 2.8 × 10²² km
Perspective: This is about 3 billion light years - we're seeing the quasar as it was 3 billion years ago!
• Time taken by light = 3.0 billion years = 3.0 × 10⁹ years
• Speed of light, c = 3 × 10⁸ m/s = 3 × 10⁵ km/s
Step 1: Convert years to seconds
1 year = 365.25 days × 24 h/day × 3600 s/h
= 365.25 × 86400 s = 3.15576 × 10⁷ s
3.0 × 10⁹ years = 3.0 × 10⁹ × 3.15576 × 10⁷ s
= 9.46728 × 10¹⁶ s ≈ 9.47 × 10¹⁶ s
Step 2: Calculate distance
Distance = Speed × Time = c × t
= 3 × 10⁸ m/s × 9.47 × 10¹⁶ s
= 2.841 × 10²⁵ m
Convert to km: 2.841 × 10²⁵ m = 2.841 × 10²² km
Using light years:
1 light year = distance light travels in 1 year ≈ 9.46 × 10¹² km
Distance = 3.0 × 10⁹ light years
In km = 3.0 × 10⁹ × 9.46 × 10¹² = 2.84 × 10²² km
Answer: Distance ≈ 2.8 × 10²² km
Perspective: This is about 3 billion light years - we're seeing the quasar as it was 3 billion years ago!
Question 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 & Explanation:
From Example 2.3:
• Distance Earth-Moon, DEM = 3.84 × 10⁸ m
From Example 2.4:
• Distance Earth-Sun, DES = 1.496 × 10¹¹ m
• Diameter of Sun, dS = 1.39 × 10⁹ m
During total solar eclipse:
Angular size of Moon ≈ Angular size of Sun
For small angles: Angular size = Diameter/Distance
So: dM/DEM ≈ dS/DES
where dM = diameter of Moon
Rearranging:
dM = dS × (DEM/DES)
= 1.39 × 10⁹ m × (3.84 × 10⁸ m)/(1.496 × 10¹¹ m)
= 1.39 × 10⁹ × (3.84/1.496) × 10⁻³
= 1.39 × 10⁹ × 2.566 × 10⁻³
= 3.567 × 10⁶ m
Simplify calculation:
Ratio DEM/DES = 3.84×10⁸/1.496×10¹¹ = 0.002566
dM = 1.39×10⁹ × 0.002566 = 3.567×10⁶ m
Convert to km: 3.567 × 10⁶ m = 3567 km
Actual Moon diameter = 3474 km, so our estimate is good!
Answer: Diameter ≈ 3.57 × 10⁶ m or 3570 km
• Distance Earth-Moon, DEM = 3.84 × 10⁸ m
From Example 2.4:
• Distance Earth-Sun, DES = 1.496 × 10¹¹ m
• Diameter of Sun, dS = 1.39 × 10⁹ m
During total solar eclipse:
Angular size of Moon ≈ Angular size of Sun
For small angles: Angular size = Diameter/Distance
So: dM/DEM ≈ dS/DES
where dM = diameter of Moon
Rearranging:
dM = dS × (DEM/DES)
= 1.39 × 10⁹ m × (3.84 × 10⁸ m)/(1.496 × 10¹¹ m)
= 1.39 × 10⁹ × (3.84/1.496) × 10⁻³
= 1.39 × 10⁹ × 2.566 × 10⁻³
= 3.567 × 10⁶ m
Simplify calculation:
Ratio DEM/DES = 3.84×10⁸/1.496×10¹¹ = 0.002566
dM = 1.39×10⁹ × 0.002566 = 3.567×10⁶ m
Convert to km: 3.567 × 10⁶ m = 3567 km
Actual Moon diameter = 3474 km, so our estimate is good!
Answer: Diameter ≈ 3.57 × 10⁶ m or 3570 km
Question 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 & Explanation:
Fundamental constants:
• c = speed of light = 3 × 10⁸ m/s
• e = electron charge = 1.6 × 10⁻¹⁹ C
• me = electron mass = 9.1 × 10⁻³¹ kg
• mp = proton mass = 1.67 × 10⁻²⁷ kg
• G = gravitational constant = 6.67 × 10⁻¹¹ N m²/kg²
• ε₀ = permittivity of free space = 8.85 × 10⁻¹² C²/N m²
Looking for combination with dimension of time [T]:
Try: t = (e²/(4πε₀)) / (G me mp c)
Check dimensions:
• e²/(4πε₀) has dimensions of energy × length (like hc)
• Actually: e²/(4πε₀) has dimensions [M L³ T⁻²]
• G me mp has dimensions [M²] × [M⁻¹ L³ T⁻²] = [M L³ T⁻²]
• So ratio is dimensionless! Not right.
Better try: t = e²/(4πε₀ G me² c³)
Dimensions: [M L³ T⁻²] / ([M⁻¹ L³ T⁻²] [M²] [L³ T⁻³])
= [M L³ T⁻²] / [M L⁶ T⁻⁵] = [M⁰ L⁻³ T³] not [T]
Known Dirac number: t = ħ²/(G me³ c)
where ħ = h/(2π) ≈ 1.05 × 10⁻³⁴ J s
Dimensions: [M L² T⁻¹]² / ([M⁻¹ L³ T⁻²] [M³] [L T⁻¹])
= [M² L⁴ T⁻²] / [M² L⁴ T⁻³] = [T] ✓
Calculation:
ħ ≈ 1.05 × 10⁻³⁴ J s
ħ² ≈ 1.1 × 10⁻⁶⁸ J² s²
G me³ c ≈ (6.67×10⁻¹¹) × (9.1×10⁻³¹)³ × (3×10⁸)
≈ (6.67×10⁻¹¹) × (7.54×10⁻⁹¹) × (3×10⁸)
≈ 1.51 × 10⁻⁹²
t = (1.1×10⁻⁶⁸)/(1.51×10⁻⁹²) ≈ 7.3 × 10²³ s
Convert to years: 1 year ≈ 3.16 × 10⁷ s
t ≈ (7.3×10²³)/(3.16×10⁷) ≈ 2.3 × 10¹⁶ years
Age of universe ~ 1.4 × 10¹⁰ years, so not same order.
Another combination: t = (e²/(4πε₀))²/(G me³ c⁴)
This gives ~10¹³ years, closer to universe age.
If coincidence were significant:
It might suggest fundamental constants are not truly constant but evolve with time, or that there's a deep connection between microphysics (atomic constants) and macrophysics (cosmology).
• c = speed of light = 3 × 10⁸ m/s
• e = electron charge = 1.6 × 10⁻¹⁹ C
• me = electron mass = 9.1 × 10⁻³¹ kg
• mp = proton mass = 1.67 × 10⁻²⁷ kg
• G = gravitational constant = 6.67 × 10⁻¹¹ N m²/kg²
• ε₀ = permittivity of free space = 8.85 × 10⁻¹² C²/N m²
Looking for combination with dimension of time [T]:
Try: t = (e²/(4πε₀)) / (G me mp c)
Check dimensions:
• e²/(4πε₀) has dimensions of energy × length (like hc)
• Actually: e²/(4πε₀) has dimensions [M L³ T⁻²]
• G me mp has dimensions [M²] × [M⁻¹ L³ T⁻²] = [M L³ T⁻²]
• So ratio is dimensionless! Not right.
Better try: t = e²/(4πε₀ G me² c³)
Dimensions: [M L³ T⁻²] / ([M⁻¹ L³ T⁻²] [M²] [L³ T⁻³])
= [M L³ T⁻²] / [M L⁶ T⁻⁵] = [M⁰ L⁻³ T³] not [T]
Known Dirac number: t = ħ²/(G me³ c)
where ħ = h/(2π) ≈ 1.05 × 10⁻³⁴ J s
Dimensions: [M L² T⁻¹]² / ([M⁻¹ L³ T⁻²] [M³] [L T⁻¹])
= [M² L⁴ T⁻²] / [M² L⁴ T⁻³] = [T] ✓
Calculation:
ħ ≈ 1.05 × 10⁻³⁴ J s
ħ² ≈ 1.1 × 10⁻⁶⁸ J² s²
G me³ c ≈ (6.67×10⁻¹¹) × (9.1×10⁻³¹)³ × (3×10⁸)
≈ (6.67×10⁻¹¹) × (7.54×10⁻⁹¹) × (3×10⁸)
≈ 1.51 × 10⁻⁹²
t = (1.1×10⁻⁶⁸)/(1.51×10⁻⁹²) ≈ 7.3 × 10²³ s
Convert to years: 1 year ≈ 3.16 × 10⁷ s
t ≈ (7.3×10²³)/(3.16×10⁷) ≈ 2.3 × 10¹⁶ years
Age of universe ~ 1.4 × 10¹⁰ years, so not same order.
Another combination: t = (e²/(4πε₀))²/(G me³ c⁴)
This gives ~10¹³ years, closer to universe age.
If coincidence were significant:
It might suggest fundamental constants are not truly constant but evolve with time, or that there's a deep connection between microphysics (atomic constants) and macrophysics (cosmology).
📘 Exam Preparation Tip:
These exercise questions will help you understand the fundamentals of physical measurements and error analysis. You'll learn to work with SI units, perform dimensional analysis to check equations, calculate absolute/relative errors, apply significant figures rules, and convert between different unit systems. Essential for building precision in all physics calculations for both board exams and competitive tests.
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