ARMCQs DIGITAL STUDY NOTES
Chapter 5: States of Matter
Physical States of Matter
What is matter?
Matter is anything that has mass and occupies space. Its particles can be arranged in different ways. These arrangements help explain its different physical states.
Understand it simply
The same substance can have different states. Ice, liquid water and water vapour are all H₂O, but their particles are arranged and move differently.
Solids, liquids and gases are the three familiar states. Matter can also form plasma and Bose–Einstein condensates.
Solid • Liquid • Gas
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When a solid becomes a liquid, what mainly changes in this particle model?
Choose what you expect, then test it below. You can explore without answering first.
The model contains 30 particles. Start with Solid.
Press Play movement, then choose Liquid and Gas. Compare spacing and movement.Solid particles vibrate close to fixed positions.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
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Property | Solid | Liquid | Gas |
|---|---|---|---|
Shape | Fixed | Takes container shape | Fills container |
Volume | Fixed | Almost fixed | No fixed volume |
Particle spacing | Usually close | Usually close | Far apart |
Particle movement | Mostly vibrate in place | Slide past neighbours | Move freely and randomly |
Compressibility | Very small | Very small | High |
Diffusion | Usually very slow | Slower than gases | Generally fast |
Why are their properties different?
Particles move and attract one another. Temperature and pressure affect their arrangement. These factors help decide the state. Kinetic energy is energy of motion. At one temperature, some particles move faster than others.
A particle is not always a molecule. Depending on the substance, it may be an atom, a molecule or an ion.
Kinetic Molecular Theory of Gases
Main ideas for an ideal gas
A gas has many tiny particles. There are large spaces between them.
The particles keep moving in random directions. Between collisions, they move in straight lines.
Particles hit one another and the container walls. In an ideal gas, these collisions are elastic: the total kinetic energy stays the same during each collision.
The ideal-gas model treats particles as very small compared with the container. It ignores attractions between them except during collisions.
The average kinetic energy of straight-line particle motion depends only on temperature in kelvin. Higher kelvin temperature means higher average kinetic energy.
Why does a gas exert pressure?
Moving particles hit the walls. Each hit transfers momentum and produces a force. The force on each unit of wall area gives gas pressure.
Why Gases Exert Pressure
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At fixed volume, what happens to ideal-gas pressure when 300 K becomes 600 K?
Choose what you expect, then test it below. You can explore without answering first.
Start: 300 K, relative pressure 1.00 ×. Gas amount and volume stay fixed.
Press Play movement. Raise Gas temperature to 600 K. Compare the pressure and speed readings.Relative to 300 K. Heating a fixed amount of ideal gas at fixed volume raises pressure. Straight paths and wall rebounds illustrate collisions; particle sizes and speeds are schematic.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
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Real gases
Real particles take up space and attract one another. The ideal-gas model works best at low pressure and high temperature, when the gas is not close to becoming liquid.
Diffusion and Effusion of Gases
Diffusion
Diffusion is the net spreading of particles from higher concentration to lower concentration due to random motion, until the mixture becomes more uniform.
Understand it simply
Particles spread because they keep moving randomly. Over time, a concentrated patch becomes more evenly mixed.
Examples: perfume spreading across a room, smoke mixing with air and the smell of flowers.
Diffusion Of Gases
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As particles mix, what happens to their total number?
Choose what you expect, then test it below. You can explore without answering first.
Mixing progress starts at 0%. Two colours help you follow the particles.
Press Play mixing or move Mixing progress from 0% to 100%. Follow both colours.The same particles become more evenly distributed. The progress control is an illustration, not a measured diffusion time.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
View complete static diagram
Effusion
Effusion is the escape of gas through a tiny opening into a lower-pressure region, ideally with the opening smaller than the molecular mean free path.
A gas may escape through a tiny hole in a balloon or tyre.
Difference
Diffusion | Effusion |
|---|---|
Mixing/spreading within a space | Escape through a tiny hole |
No tiny hole required | A tiny hole is essential |
Depends on concentration and transport conditions | Depends strongly on molecular mass and pressure |
Graham's law (equal temperature and comparable conditions)
Rate of effusion ∝ 1 / √(molar mass). Thus, rate₁ / rate₂ = √(M₂ / M₁). This simple relation is most accurate for ideal gases effusing through small openings.
Example: Hydrogen gas (M = 2) effuses four times as fast as oxygen gas (M = 32), since √(32/2) = √16 = 4.
Graham’s simple law works best for effusion through very small openings. Diffusion in air also depends on collisions and mixing, so this law alone may not predict its rate.
Mean free path
The average distance a gas molecule travels between successive collisions.
Gas Pressure, Compressibility, Mobility and Density
Pressure
Pressure = force acting at right angles to a surface / area, or P = F/A. Its SI unit is pascal (Pa), where 1 Pa = 1 N/m².
Standard pressure unit | Equivalent |
|---|---|
1 atm | 101 325 Pa |
1 atm | 760 mmHg = 760 torr |
1 atm | about 101.3 kPa |
A barometer measures atmospheric pressure.
A manometer compares gas pressure with a known pressure, often the pressure of the air.
Heating gas in a rigid container usually raises its pressure. The particles hit the walls harder and transfer more momentum.
Compressibility
Large gaps make a gas easy to squeeze into less space. Compression brings the same particles closer. At the same temperature, pressure increases.
Gas Compression
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What happens to pressure when you halve the gas volume?
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Start: 4 L and 1 atm. Keep gas amount and temperature fixed.
Move Change volume from 4 L to 2 L. Compare pressure before and after.Ideal-gas illustration. Particle number stays fixed. The graph and piston show the same relationship.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
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Mobility
Gas particles move freely, which allows gases to flow, expand and mix easily.
Density
Density is mass divided by volume: ρ = m/V. Gas density is usually much lower than the density of a liquid or solid.
At the same pressure, heating a fixed amount of gas increases its volume. Its density falls because the same mass occupies more space. Cooling has the opposite effect.
Gas density depends on temperature and pressure. Check both conditions before comparing values.
Gas | Density around 0 °C, 1 atm (kg/m³) |
|---|---|
H₂ | 0.090 |
He | 0.179 |
N₂ | 1.25 |
O₂ | 1.43 |
CO₂ | 1.98 |
Cl₂ | 3.17 |
Boyle's Law — Pressure and Volume
Statement
For a fixed amount of gas at constant temperature, volume is inversely proportional to absolute pressure.
V ∝ 1/P → PV = constant → P₁V₁ = P₂V₂.
Understand it simply
If pressure doubles at the same temperature, gas volume becomes half. If pressure becomes half, volume doubles.
Boyle’s Law • P × V = Constant
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What happens to pressure when you halve the gas volume?
Choose what you expect, then test it below. You can explore without answering first.
Start: 4 L and 1 atm. Keep gas amount and temperature fixed.
Move Change volume from 4 L to 2 L. Compare pressure before and after.Ideal-gas illustration. Particle number stays fixed. The graph and piston show the same relationship.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
View complete static diagram
Pressure (atm) | Volume (L) | P × V |
|---|---|---|
1 | 4 | 4 |
2 | 2 | 4 |
4 | 1 | 4 |
How to solve
Write P₁, V₁, P₂ and V₂ with units.
Convert pressures to the same unit and volumes to the same unit.
Use P₁V₁ = P₂V₂, rearrange and substitute.
Check whether the answer makes physical sense.
Solved example 1: volume after reducing pressure
Given: P₁ = 3 atm; V₁ = 5 L; P₂ = 2 atm; V₂ = ?
Formula: V₂ = P₁V₁ / P₂
Step: V₂ = (3 × 5) / 2 = 15/2
Step: V₂ = 7.5 L
Answer: 7.5 L. Pressure decreased, so volume increased.
Solved example 2: pressure after halving volume
Given: P₁ = 650 mmHg; V₁ = 700 cm³; V₂ = 350 cm³; P₂ = ?
Formula: P₂ = P₁V₁ / V₂
Step: P₂ = (650 × 700) / 350
Step: 700/350 = 2; therefore P₂ = 650 × 2
Answer: 1300 mmHg. Halving volume doubles pressure.
Charles's Law — Volume and Temperature
Statement
For a fixed amount of gas at constant pressure, its volume is directly proportional to its absolute temperature.
V ∝ T → V/T = constant → V₁/T₁ = V₂/T₂. Always use temperature in kelvin.
Kelvin and Celsius
T(K) = t(°C) + 273.15. For school-level mental calculations, +273 is a common approximation.
Absolute zero is 0 K, or −273.15 °C. Extending the ideal-gas graph reaches zero volume there. A real gas changes into liquid or solid before it can reach this predicted state.
Charles’s Law • V / T = Constant
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At fixed pressure, what happens to volume when kelvin temperature doubles?
Choose what you expect, then test it below. You can explore without answering first.
Start: 300 K and 2 L. Keep gas amount and pressure fixed.
Move Change temperature from 300 K to 600 K. Watch the piston and graph.Ideal-gas illustration. Particle number stays fixed. The graph and piston show the same relationship.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
View complete static diagram
Understand it simply
At constant pressure, 300 K to 600 K doubles the volume. But 30 °C to 60 °C does not double the kelvin temperature.
How to solve
Convert each Celsius temperature to kelvin before applying the formula.
Identify V₁, V₂, T₁ and T₂.
Rearrange V₁/T₁ = V₂/T₂ and substitute.
If the required answer is °C, convert back at the end.
Solved example 3: heating a gas
Given: V₁ = 600 mL; T₁ = 27 °C ≈ 300 K; T₂ = 77 °C ≈ 350 K; V₂ = ?
Formula: V₂ = V₁T₂ / T₁
Step: V₂ = 600 × 350 / 300
Step: 600/300 = 2; 2 × 350 = 700
Answer: 700 mL (using the usual school-level 273 K approximation).
Solved example 4: temperature when volume doubles
Given: V₁ = 350 cm³; V₂ = 700 cm³; T₁ = 40 °C ≈ 313 K; T₂ = ?
Formula: T₂ = T₁V₂ / V₁
Step: T₂ = 313 × (700/350) = 313 × 2
Step: T₂ = 626 K; t₂ ≈ 626 − 273
Answer: 626 K, or approximately 353 °C.
Gas Laws: Concept Check
Boyle's law | Charles's law |
|---|---|
Relates pressure and volume | Relates volume and absolute temperature |
Constant temperature | Constant pressure |
P₁V₁ = P₂V₂ | V₁/T₁ = V₂/T₂ |
Inverse relationship | Direct relationship |
Graph P against V: curved hyperbola | Graph V against T(K): straight line |
What must remain fixed?
For both laws, keep the amount of gas fixed. For Boyle’s law, also keep temperature fixed. For Charles’s law, keep pressure fixed.
What if a gas is allowed to expand?
Expansion alone does not tell us whether gas temperature rises or falls. It depends on how the gas expands and whether heat enters or leaves. Charles’s law applies when pressure stays fixed.
Why Celsius cannot be substituted directly
Gas-law ratios need kelvin temperature. Celsius starts from a different zero. Convert Celsius to kelvin before putting temperatures into the formula.
Liquid State: Structure and Properties
What is a liquid?
A liquid has nearly fixed volume but no fixed shape. It flows and takes the shape of the lower part of its container.
Liquid particles are close together. They can slide past one another.
Liquids are hard to squeeze into less space because their particles are already close.
Attractions hold liquid particles together. The particles are still free to change places.
Under similar conditions, particles usually spread more slowly through liquids than through gases.
Why liquids flow
A liquid flows because its particles can change places. It keeps nearly the same volume and usually has a surface. A gas spreads to fill all the space available.
Evaporation and Cooling
Definition
Evaporation is the change of liquid into vapour from its surface, including at temperatures below its boiling point. It requires energy (endothermic process).
Understand it simply
Some molecules escape from the liquid surface. This can happen without boiling the whole liquid.
Evaporation
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Liquid surface. Evaporation occurs at the surface. Some energetic molecules escape into the space above the liquid.
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Why evaporation cools
Faster, higher-energy molecules are more likely to escape. The liquid left behind can have lower average kinetic energy and become cooler. Heat then flows in from the surroundings.
Examples: sweating cools the skin; wet clothes dry in air.
Factors affecting evaporation
Higher temperature usually makes evaporation faster.
A larger exposed surface lets more molecules escape each second.
Moving air carries vapour away. More liquid can then evaporate.
Drier air usually allows faster evaporation. Humidity tells us how much water vapour is in the air.
Under similar conditions, weaker attractions let particles escape more easily.
Evaporation versus boiling
Evaporation happens at the surface and can occur below the boiling point. Boiling makes vapour bubbles throughout the liquid. It begins when vapour pressure matches the pressure outside.
Vapour Pressure and Dynamic Equilibrium
Definition
Equilibrium vapour pressure is the pressure exerted by a liquid's vapour in a closed system when evaporation and condensation occur at equal rates at a fixed temperature.
Understand it simply
In a closed container, liquid particles leave and return. At equilibrium, both happen at the same rate.
How equilibrium is reached
At first, some liquid particles escape into the space above the liquid.
Vapour builds up. More vapour particles then return to the liquid. This return is condensation.
Eventually, particles leave and return at equal rates. Both processes continue. This is dynamic equilibrium.
Dynamic Vapour Equilibrium
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Early stage. At first, more molecules evaporate than condense.
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Factors affecting vapour pressure
Higher temperature gives a higher equilibrium vapour pressure.
At the same temperature, stronger attractions usually give a lower vapour pressure.
Molecular size also affects attractions. Polarity alone cannot tell us how easily a liquid evaporates.
At 100 °C, water's equilibrium vapour pressure is 760 mmHg (1 atm), its normal boiling point. At 0 °C the saturation pressure over liquid water is about 4.6 mmHg.
At a fixed temperature, the equilibrium vapour pressure stays the same while some liquid remains. Adding more of that liquid does not raise the equilibrium vapour pressure.
Boiling and Freezing Points
Boiling point
The boiling point is the temperature at which vapour pressure becomes equal to external pressure. Vapour bubbles can then grow throughout the liquid.
Higher outside pressure raises the boiling point. This is why water boils at a higher temperature in a pressure cooker.
Lower outside pressure lowers the boiling point. On high mountains, water boils below 100 °C.
Among similar liquids, stronger attractions usually give a higher boiling point.
At standard atmospheric pressure (1 atm), water boils near 100 °C; ethanol near 78 °C; bromine near 59 °C; diethyl ether near 35 °C; acetic acid near 118 °C; mercury near 357 °C.
Freezing point
The freezing point is the temperature where a liquid and its solid can coexist in equilibrium at a specified pressure. A pure substance has the same equilibrium freezing and melting point at that pressure.
Phase Changes
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Solid ↔ liquid. Melting changes solid to liquid. Freezing is the reverse change.
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Factors
Changing pressure has a large effect on boiling point. Its effect on ordinary freezing points is usually much smaller.
Some dissolved impurities lower a solvent’s freezing point. Salt added to ice water is an example.
Particle arrangement and attractions help determine melting and freezing points.
Examples of freezing points: water 0 °C; benzene 5.5 °C; acetic acid 16.6 °C; ethanol −114 °C; bromine −7.2 °C; mercury −38.8 °C.
At the freezing point, solid and liquid can remain together without an overall change from one into the other. This balance is called phase equilibrium.
Diffusion, Mobility and Density of Liquids
Diffusion
Diffusion is the net spreading of particles from a region of greater concentration to a region of lower concentration due to random motion. A drop of ink gradually spreads through still water.
Diffusion In Liquids
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As particles mix, what happens to their total number?
Choose what you expect, then test it below. You can explore without answering first.
Mixing progress starts at 0%. Two colours help you follow the particles.
Press Play mixing or move Mixing progress from 0% to 100%. Follow both colours.The same particles become more evenly distributed. The progress control is an illustration, not a measured diffusion time.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
View complete static diagram
Factors affecting diffusion
Temperature: higher temperature usually speeds up diffusion.
Viscosity describes resistance to flow. Particles usually move more slowly through a more viscous liquid.
Under similar conditions, smaller particles can spread faster. Particle shape also matters.
A concentration difference gives an overall spread from the more concentrated region towards the less concentrated region.
Mobility
Mobility is how easily particles can move. Molecules in a warmer or less viscous liquid are often more mobile.
Density
Density (ρ) = mass (m) / volume (V). Liquids are generally denser than gases and much less compressible.
Most liquids expand when heated. Their density therefore falls. Water is unusual between 0 and 4 °C: it is densest near 4 °C.
Approximate water densities: 0 °C = 0.99984 g/cm³; 30 °C = 0.99565 g/cm³; 60 °C = 0.9832 g/cm³; 90 °C = 0.9653 g/cm³.
Under usual conditions, pressure changes a liquid’s density only slightly.
Solid State: Melting, Rigidity and Density
Physical properties
Solids have definite shape and volume.
Particles vibrate near fixed positions. They do not stop moving.
Most solids are hard to compress. They do not flow like liquids.
Pure crystalline solids often have a sharp melting point.
Melting point
The melting point is the temperature at which solid and liquid coexist in equilibrium at a fixed pressure. Added heat changes particle arrangement rather than increasing temperature during the phase transition of a pure material.
Ice melts near 0 °C at atmospheric pressure; sodium chloride near 801 °C.
Rigidity
Particles in a solid cannot easily change neighbours. The solid therefore resists a change in shape. Its particles still vibrate.
Density
Density = m/V. Many solids are denser than corresponding liquids, but ice is less dense than liquid water.
Approximate solid densities in g/cm³: aluminium 2.70; iron 7.87; gold 19.3; sodium chloride 2.16; sucrose 1.59.
Mercury is liquid at room temperature. Its melting point is −38.8 °C.
Crystalline and Amorphous Solids
Crystalline solids
Particles are arranged in a regular, repeating three-dimensional pattern (long-range order). Pure crystals commonly have a sharp melting point. Some split along particular flat surfaces called cleavage planes.
Examples include sodium chloride, diamond, quartz and ice.
Amorphous solids
Particles have no long-range periodic order. Many amorphous substances soften over a range of temperatures rather than melting sharply.
Ordinary glass and many plastics are examples. Some polymers contain both ordered and disordered regions.
Crystalline Vs Amorphous
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What distinguishes the crystalline view from the amorphous view?
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Both views represent a solid. Compare the particle arrangement.
Switch between Crystalline and Amorphous. Look for a pattern that repeats across the model.Compare a repeating pattern with a disordered arrangement. Both represent solids.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
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Key differences
A crystal has a repeating structure. It often melts at a sharp temperature. Some properties depend on direction. This is called anisotropy.
An amorphous solid lacks a long-range repeating pattern. It often softens over a range of temperatures. Its properties are usually the same in different directions. This is called isotropy.
Some crystals split along particular flat surfaces, called cleavage planes. Amorphous solids do not have regular cleavage planes.
Crystals are not all made of molecules. NaCl contains ions. Diamond contains covalently bonded carbon atoms.
Allotropy of Elements
Definition
Allotropy is the existence of an element in two or more different structural forms in the same physical state. Those different forms are called allotropes.
Understand it simply
The element stays the same, but its atoms join or arrange differently. A different structure gives different properties.
Carbon allotropes
In diamond, each carbon bonds to 4 others in a three-dimensional network. Diamond is very hard. Pure diamond does not conduct electricity.
In graphite, carbon atoms form layers of hexagonal rings. Some electrons move along the layers, so graphite conducts electricity.
Graphene is one layer of bonded carbon atoms in a hexagonal pattern. It is very thin, strong and electrically conductive.
In fullerenes, carbon atoms form closed cages. C₆₀ is one example.
Carbon Allotropes
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Diamond. Each carbon bonds to four others in a tetrahedral network. Strong covalent bonding in three dimensions helps make diamond very hard.
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Other examples
O₂ and O₃ are allotropes of oxygen. Sulfur and phosphorus also have different forms.
Allotropes contain the same element. Their different structures give them different properties.
Plasma and Bose–Einstein Condensate
Plasma state
Plasma contains free-moving charged particles, including positive ions and electrons. The particles affect one another and respond to electric and magnetic fields. Plasma is often called the fourth state of matter.
Examples: lightning, plasma globes, the Sun, fluorescent tubes and neon signs.
Adding enough energy to a gas can remove electrons and form plasma. Not every plasma is extremely hot.
Fusion researchers study ways to control very hot plasma.
Bose–Einstein condensate (BEC)
A Bose–Einstein condensate (BEC) can form when a suitable gas is cooled to extremely low temperatures near absolute zero. Many particles then share the same lowest-energy quantum state. Bosons are the kind of particles that can share the same quantum state in this way. A quantum state describes a particle’s allowed energy and other features of its motion.
Bose and Einstein developed the ideas in 1924–1925. Cornell, Wieman and their team made the first dilute-gas BEC in 1995. Ketterle also carried out important early experiments.
BEC depends on particle wave behaviour at very low temperatures. It is not ordinary condensation from gas to liquid.
Plasma And Bose–Einstein Condensate
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Plasma. Plasma contains mobile charged particles, including ions and electrons. Examples include stars and lightning.
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Absolute zero is 0 K, or −273.15 °C. It does not mean that every kind of motion stops. Some quantum motion, called zero-point motion, can remain.
Phase Changes: Quick Comparison
Melting and freezing
Melting: solid → liquid and absorbs energy. Freezing: liquid → solid and releases energy.
Evaporation and condensation
Vaporization: liquid → gas and absorbs energy. Condensation: gas → liquid and releases energy.
Sublimation and deposition
Sublimation: solid → gas without first becoming liquid. Deposition: gas → solid.
Ionization and recombination
Ionization forms charged particles in a gas. During recombination, electrons can rejoin ions.
At fixed pressure, a pure substance stays at nearly the same temperature while melting or boiling. Energy changes the state during this time.
A simple energy ladder can help compare familiar changes of state. It does not fully describe plasma or BEC.
Solved Textbook Short Questions
1. What is allotropy? Give examples.
Allotropy is the existence of one element in different structures in the same physical state. Examples: diamond and graphite (carbon); oxygen and ozone.
2. Explain effusion with examples.
Effusion is the escape of a gas through a very small opening into a lower-pressure space. Gas escaping through a sufficiently tiny opening into a lower-pressure space is an example.
3. Define boiling, melting and freezing points.
Boiling point: temperature where liquid vapour pressure equals external pressure. Melting point: temperature where solid and liquid coexist in equilibrium. Freezing point: temperature where liquid solidifies in equilibrium with solid.
4. How do temperature and pressure affect liquid density?
Heating generally expands a liquid and lowers its density; higher pressure slightly raises density. Water has maximum density near 4 °C.
5. Explain plasma with everyday examples.
Plasma is a partly or strongly ionized gas with mobile electrons and ions. Examples include lightning, fluorescent lights, neon signs and plasma globes.
6. Why are BEC atoms extremely cold?
Scientists cool a suitable gas until many of its particles can share the same lowest-energy state. Their wave behaviour then becomes important and a BEC can form. Their motion does not completely stop.
7. Use kinetic theory to compare states.
Solid: particles vibrate near fixed positions. Liquid: nearby particles move past one another. Gas: particles are far apart, move randomly and spread to fill the container.
Important self-test: why do gases diffuse quickly?
Gas particles move constantly and have relatively large spaces between them, leading to rapid mixing.
Important self-test: why does gas density rise on cooling?
For a fixed amount of gas at constant pressure, cooling reduces its volume, so density m/V rises.
Important self-test: why is diffusion in a liquid slower?
Liquid particles remain close to one another and interact strongly, making long-distance movement slower than gas mixing in common conditions.
Important self-test: why does evaporation cool?
More energetic molecules escape first, reducing the average energy of the remaining liquid; energy is absorbed from its surroundings.
Important self-test: why does a pressure cooker cook faster?
Higher pressure raises water's boiling point, allowing food to be heated above 100 °C.
Important self-test: what is dynamic vapour equilibrium?
In a closed container at fixed temperature, evaporation and condensation continue at equal rates.
Important self-test: what is absolute zero?
Absolute zero is 0 K or −273.15 °C, the lowest temperature on the kelvin scale. Some quantum motion can remain even at this temperature.
Solved Textbook Detailed Questions
1. Explain evaporation and its factors.
Evaporation is surface vaporization below the boiling point. It requires energy, often causing cooling. Its rate generally rises with temperature, exposed surface area and airflow and falls with humidity. Liquids with weaker intermolecular attractions are usually more volatile under similar conditions.
2. State and explain Boyle's law.
For fixed gas amount and temperature, pressure and volume vary inversely: PV = constant, so P₁V₁ = P₂V₂. Example: 1 atm × 4 L = 2 atm × 2 L. A pressure increase makes volume smaller.
3. Compare crystalline and amorphous solids.
Crystalline solids have long-range repeating order, often sharp melting points and directional properties. Amorphous solids lack long-range order and commonly soften over a temperature range. Examples: NaCl crystal versus ordinary glass.
4. State and explain Charles's law.
At constant pressure for a fixed quantity of gas, V ∝ T(K), so V₁/T₁ = V₂/T₂. Example: 300 K and 2 L become 600 K and 4 L at constant pressure.
5. Explain diffusion in liquids and its factors.
In a liquid, particles move randomly. Overall, more particles move from a region of higher concentration to one of lower concentration. The change in concentration over a distance is called a concentration gradient.
Diffusion is usually faster at higher temperature and slower in more viscous liquids. Viscosity is resistance to flow. Particle size and shape also affect diffusion.
6. Explain factors affecting boiling point.
A liquid boils when its vapour pressure reaches external pressure. Higher external pressure raises boiling point; lower pressure lowers it. Stronger intermolecular attractions generally cause a higher boiling point for similar molecules; composition can also alter it.
7. Define vapour pressure and explain closed-system equilibrium.
Equilibrium vapour pressure is the pressure of vapour in contact with its liquid when evaporation equals condensation at a fixed temperature. This saturated dynamic equilibrium is most readily established and maintained in a closed container; vapour still exists above an open liquid.
Comparison: ideal gas versus real gas.
An ideal gas is a model that ignores particle volume and attractions between particles. Real gas particles have size and attract one another. Real gases behave more like ideal gases at low pressure and high temperature.
Solved Exercise Numericals — Every Step
How to solve gas-law calculations
Write down all given quantities with units.
Identify the constant condition: Boyle = constant temperature; Charles = constant pressure.
Convert Celsius into kelvin when temperature occurs in a gas-law equation.
Substitute values, simplify, write final answer and check whether the change makes sense.
Question 1(a): Convert 100 °C to kelvin.
Step 1: T(K) = t(°C) + 273.15.
Step 2: T = 100 + 273.15 = 373.15 K.
Answer: 373.15 K (≈373 K).
Question 1(b): Convert 150 °C to kelvin.
Step 1: T(K) = t(°C) + 273.15.
Step 2: T = 150 + 273.15 = 423.15 K.
Answer: 423.15 K (≈423 K).
Question 1(c): Convert 780 K into Celsius.
Step 1: t(°C) = T(K) − 273.15.
Step 2: t = 780 − 273.15 = 506.85 °C.
Answer: 506.85 °C (≈507 °C).
Question 1(d): Convert 170 K into Celsius.
Step 1: t(°C) = T(K) − 273.15.
Step 2: t = 170 − 273.15 = −103.15 °C.
Answer: −103.15 °C (≈−103 °C).
Question 2: Gas expands from 90.5 to 120 cm³ at constant pressure. Initial temperature is 33 °C.
Given: V₁ = 90.5 cm³; V₂ = 120 cm³; T₁ = 33 + 273.15 = 306.15 K; T₂ = ?
Step 1: Charles's law is V₁/T₁ = V₂/T₂.
Step 2: T₂ = T₁ × V₂/V₁ = 306.15 × 120/90.5.
Step 3: T₂ ≈ 405.94 K.
Step 4: t₂ = 405.94 − 273.15 ≈ 132.8 °C.
Answer: approximately 406 K or 133 °C. More volume at constant pressure means a higher absolute temperature.
Question 3: 78 mL of gas heated from 35 °C to 80 °C at constant pressure.
Given: V₁ = 78 mL; T₁ = 35 + 273.15 = 308.15 K; T₂ = 80 + 273.15 = 353.15 K.
Step 1: V₁/T₁ = V₂/T₂, so V₂ = V₁ × T₂/T₁.
Step 2: V₂ = 78 × 353.15/308.15 ≈ 89.39 mL.
Answer: about 89.4 mL. Heating at constant pressure increases gas volume.
Question 4: 40.0 dm³ gas at 1 atm compressed to 3 atm at the same temperature.
Given: P₁ = 1 atm; V₁ = 40.0 dm³; P₂ = 3 atm; V₂ = ?
Step 1: Boyle's law, P₁V₁ = P₂V₂.
Step 2: V₂ = (P₁V₁)/P₂ = (1 × 40)/3 = 13.33 dm³.
Answer: approximately 13.3 dm³. Tripling pressure reduces volume to one third.
Question 5: 800 cm³ gas at 750 mmHg compressed to 250 cm³.
Given: P₁ = 750 mmHg; V₁ = 800 cm³; V₂ = 250 cm³; P₂ = ?
Step 1: P₁V₁ = P₂V₂; P₂ = P₁V₁/V₂.
Step 2: P₂ = (750 × 800)/250 = 750 × 3.2 = 2400 mmHg.
Answer: 2400 mmHg (about 3.16 atm).
Question 6: Gas at 8 atm and 15 L, pressure reduced to 6 atm.
Given: P₁ = 8 atm; V₁ = 15 L; P₂ = 6 atm; V₂ = ?
Step 1: V₂ = P₁V₁/P₂.
Step 2: V₂ = (8 × 15)/6 = 120/6 = 20 L.
Answer: 20 L. Pressure decreases, therefore volume increases.
Numerical accuracy note
Using +273 instead of +273.15 gives very slightly different results, which are acceptable for Class 9 approximations. For formal scientific calculations, use 273.15.