Q.Explain why
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Kinetic Theory Explanation
Imagine you're sitting in a quiet room. The air around you feels still, but it isn't. Every second, billions of tiny particles — molecules of nitrogen and oxygen — are zipping past you at hundreds of metres per second. You don't feel them because they're too small, and they're moving in every direction at once. But if you put your hand near a hot stove, you suddenly feel heat. Why?
The answer is the kinetic theory of matter. It's a way of explaining what we observe at the human scale (temperature, pressure, heat) by thinking about what's happening at the molecular scale.
The core idea
The kinetic theory says three simple things:
- All matter is made of tiny particles (atoms or molecules) that are in constant, random motion.
- The particles collide with each other and with the walls of their container — these collisions are perfectly elastic (no energy is lost).
- The average kinetic energy of these particles is directly proportional to the temperature of the substance.
That's it. Everything else — pressure, diffusion, the way a gas expands when heated — follows from these three statements.
Building intuition
Think of a single gas molecule bouncing around inside a box. It hits a wall, bounces off, and keeps going. Each time it hits the wall, it exerts a tiny force. Now multiply that by billions of molecules hitting every square centimetre of wall every second. That constant, collective force is what we measure as pressure.
Now heat the box. The molecules move faster — their average kinetic energy increases. They hit the walls harder and more often. Pressure goes up. If the walls can move (like a piston), the gas expands until the pressure inside equals the pressure outside.
This is why a bicycle tyre feels hot after you pump it: you're doing work on the air, compressing it, which increases the average kinetic energy of the molecules — and that's exactly what temperature is.
Temperature is not the total kinetic energy of all molecules — it's the average kinetic energy per molecule. A large cold object can have more total energy than a small hot one, but its molecules move slower on average.
The precise statement
For an ideal gas (a gas where intermolecular forces are negligible and collisions are perfectly elastic), the kinetic theory gives us a direct mathematical link:
Average kinetic energy per molecule=23kBT
where kB is Boltzmann's constant (1.38×10−23J/K) and T is the absolute temperature in Kelvin.
This means that at the same temperature, all gas molecules — regardless of their mass — have the same average kinetic energy. A light hydrogen molecule moves faster than a heavy oxygen molecule at the same temperature, but their average kinetic energies are equal.
From this, we can derive the ideal gas law:
PV=31Nmv2=NkBT
where P is pressure, V is volume, N is the number of molecules, m is the mass of one molecule, and v2 is the mean square speed.
PV=nRT
This is the familiar ideal gas law. The kinetic theory shows it's not just an empirical rule — it follows directly from the motion of molecules.
What the theory explains
The kinetic theory isn't just abstract. It explains everyday phenomena:
- Evaporation cools you: The fastest molecules escape from a liquid surface, leaving behind slower ones. The average kinetic energy drops — so the temperature drops.
- Diffusion: Molecules spread out because they're constantly moving and colliding, gradually mixing with neighbouring molecules.
- Brownian motion: Pollen grains jitter under a microscope because they're being bombarded unevenly by invisible water molecules. …
Concept: Thermal Radiation Properties – The Earth's atmosphere acts as a greenhouse blanket, while the Moon lacks one; temperature with altitude depends on how the atmosphere absorbs and re-radiates energy.
(a) The Moon has no atmosphere because its escape velocity is too low and its surface temperature too high. Gas molecules achieve thermal speeds that exceed the Moon's escape velocity (~2.4 km/s), so they simply leak away into space over time. Without sufficient gravity to hold an atmosphere, none exists. …
Both phenomena are explained by the kinetic theory of gases and the nature of thermal radiation.
- The Moon lacks an atmosphere because its escape velocity is too low to retain gas molecules against thermal motion.
- Temperature falls with altitude in the troposphere because the atmosphere is heated from below by the Earth's surface, not directly by sunlight.
The Core Idea: Two Different Mechanisms
These two questions might seem unrelated, but they both hinge on how gases behave under gravity and how heat is transferred. One is about whether a planet can hold onto its air, the other about how that air is warmed.
Let's take them one at a time.
(a) Why there is no atmosphere on the Moon
1. The escape velocity problem. Every celestial body has an escape velocity — the minimum speed an object needs to break free from its gravitational pull. For the Moon, this is only about 2.38 km/s. For Earth, it's 11.2 km/s. That's a huge difference.
2. Gas molecules are always moving. According to the kinetic theory of gases, the average speed of a gas molecule depends on temperature and molecular mass:
vrms=m3kT
where k is Boltzmann's constant, T is temperature, and m is the molecule's mass. Lighter molecules (like hydrogen, helium) move faster; heavier ones (like oxygen, nitrogen) move slower.
3. The critical ratio. A planet can retain a gas only if the escape velocity is at least 6 times the root-mean-square speed of that gas molecule. This is the Jeans escape criterion. On the Moon, even at its moderate daytime temperature (∼400 K), the rms speed of nitrogen molecules is about 0.6 km/s — and 6×0.6=3.6 km/s, which is greater than the Moon's escape velocity of 2.38 km/s.
A common mistake is to think the Moon has no atmosphere because it has no magnetic field. While that affects how solar wind strips away ions, the primary reason is simply gravity being too weak to hold gas molecules in the first place. Even without solar wind, any primordial atmosphere would have boiled away over geological time.
4. The result. Any gas that might have existed on the Moon — whether from volcanic outgassing or comet impacts — would have had molecules moving fast enough to simply drift off into space. The Moon is too small and too light to hold an atmosphere.
(b) Why temperature falls with altitude
1. The common misconception. Many students think "higher up means closer to the Sun, so it should be hotter." That's wrong. The Sun's radiation travels through the atmosphere almost without heating it directly — the air is mostly transparent to visible light.
2. The real heating mechanism. The Earth's surface absorbs sunlight and warms up. That warm surface then emits infrared radiation (thermal radiation). The atmosphere is opaque to much of this infrared radiation (thanks to greenhouse gases like CO₂ and water vapour), so it absorbs this energy and gets heated from below.
Think of the atmosphere as a blanket. The ground is the hot water bottle, and the air is the blanket. The part of the blanket closest to the bottle is warmest; the outer edge is coolest. That's exactly what happens in the troposphere — the lowest 10–15 km of the atmosphere. …
Alternate framing — think in terms of the high-speed tail, not the average. (a) It isn't the average thermal speed that determines escape, but the small fraction of molecules in the high-speed tail of the Maxwell–Boltzmann distribution that momentarily exceed escape velocity; on the Moon that tail overlaps substantially with vesc, so loss happens continuously over geological time even though the rms speed itself stays below vesc. On Earth vesc is so much larger than typical thermal speeds that even the tail almost never reaches it, except for light gases like hydrogen and helium — which is why Earth's atmosphere is nearly free of them too. …
Showing the 12 most recent of 15 on this concept.
- TG EAPCET 2026Set eng-2026-05-09-FN1 markMCQQ.Two brass spheres approaching each other with the same speed collide head-on elastically. After collision, if one of the spheres of radius R comes to rest, then the radius of the other sphere is (A) 32R (B) 33R (C) 32R (D) 33R
›Reveal solutionSolution
In a head-on elastic collision, both momentum and kinetic energy are conserved. Using the fact that one sphere comes to rest after the collision, the mass ratio is determined, and since mass is proportional to the cube of the radius, the other sphere's radius is found to be 33R.
Concept and Intuition
When two objects collide elastically, both momentum and kinetic energy are perfectly conserved. Here, the two brass spheres have the same material density, so their masses are proportional to the cube of their radii. They approach each other with equal speed, and after the collision one sphere (radius R) stops completely. This special outcome forces a specific mass ratio. By solving the conservation equations, we can find the unknown radius.
- Set up variables and conservation of momentum Let the sphere of radius R have mass m1=ρ⋅34πR3, and the other sphere of unknown radius r have mass m2=ρ⋅34πr3. Both approach with speed v in opposite directions. Take the direction of m1 as positive. Then initial velocities: u1=+v, u2=−v. After collision, m1 comes to rest: v1=0. Let v2 be the velocity of m2. Conservation of momentum:
m1v+m2(−v)=m1(0)+m2v2
(m1−m2)v=m2v2⇒v2=m2m1−m2v.
- Apply conservation of kinetic energy Initial kinetic energy:
21m1v2+21m2v2=21(m1+m2)v2.
Final kinetic energy:
21m1(0)2+21m2v22=21m2v22.
Equate:
21(m1+m2)v2=21m2v22.
Substitute v2 from step 1:
(m1+m2)v2=m2(m2m1−m2v)2=m2(m1−m2)2v2.
Cancel v2 (nonzero):
m1+m2=m2(m1−m2)2.
- Solve for the mass ratio Multiply both sides by m2:
m2(m1+m2)=(m1−m2)2.
Expand:
m1m2+m22=m12−2m1m2+m22.
Cancel m22:
m1m2=m12−2m1m2⇒3m1m2=m12.
If m1=0, divide by m1:
3m2=m1⇒m2m1=3. …
- TG EAPCET 2025Set ap-2025-04-29-AN1 markMCQQ.During adiabatic compression of an ideal gas at an initial pressure P, the final density of the gas becomes n times its initial value. The final pressure of the gas is (γ is the ratio of the specific heats of the gas at constant pressure and constant volume) (A) n(1−γ)P (B) n(γ−1)P (C) n−γP (D) nγP
›Reveal solutionSolution
During an adiabatic compression, the relationship between pressure and density is P∝ργ. Given that the final density is n times the initial density, the final pressure becomes nγ times the initial pressure. The final pressure is nγP.
When an ideal gas undergoes an adiabatic process, it means there is no heat exchange with the surroundings. This specific condition leads to a particular relationship between the pressure (P) and volume (V) of the gas, which is PVγ=constant. To solve this problem, we need to connect this relationship with the given information about the change in density.
The key insight is to express the volume of the gas in terms of its density. For a fixed mass of gas (m), volume (V) and density (ρ) are inversely related: V=m/ρ. Since the mass of the gas does not change during compression, we can substitute this expression for volume into the adiabatic equation to find a relationship between pressure and density.
- State the adiabatic process equation: For an adiabatic process, the product of pressure and volume raised to the power of γ (the ratio of specific heats) remains constant. If P1 and V1 are the initial pressure and volume, and P2 and V2 are the final pressure and volume, then:
P1V1γ=P2V2γ
- Relate volume to density: The density ρ of a gas is defined as its mass m per unit volume V, i.e., ρ=m/V. Therefore, the volume can be expressed as V=m/ρ. Since the mass of the gas remains constant throughout the compression, we can write:
V1=ρ1mandV2=ρ2m
where $\rho_1$ and $\rho_2$ are the initial and final densities, respectively.3. Substitute volume in terms of density into the adiabatic equation:
Substitute the expressions for V1 and V2 from Step 2 into the adiabatic equation from Step 1:
P1(ρ1m)γ=P2(ρ2m)γ
P1ρ1γmγ=P2ρ2γmγ
Since $m^\gamma$ is a non-zero constant on both sides, it cancels out: … - TG EAPCET 2024Set eng-2024-05-09-AN1 markMCQQ.If the temperature of a gas is increased from 27∘C to 159∘C, the increase in the rms speed of the gas molecules is (A) 142% (B) 71% (C) 80% (D) 20%
›Reveal solutionSolution
The rms speed scales with the square root of absolute temperature; converting to Kelvin and taking the ratio gives a 20% increase, so the correct option is (D).
The key idea is that the root-mean-square speed of gas molecules is given by vrms=m3kT, where T is the absolute temperature (in Kelvin). This means vrms∝T. A common pitfall is to use Celsius temperatures directly, but the relationship only holds for Kelvin. The percentage increase in speed is not the same as the percentage increase in Celsius temperature.
- Convert temperatures to Kelvin. Absolute zero is −273∘C, so:
T1=27+273=300K,T2=159+273=432K.
- Write the ratio of rms speeds. Since vrms∝T,
v1v2=T1T2=300432=1.44=1.2.
- Find the percentage increase. …
- TG EAPCET 2023Set eng-2023-05-14-AN1 markMCQQ.If the temperature of a gas is increased from 27∘C to 159∘C, then the percentage increase in the rms speed of the gas molecules is (A) 5 (B) 10 (C) 15 (D) 20
›Reveal solutionSolution
rms speed ∝T (absolute temperature). Raising T from 300K to 432K multiplies the speed by 1.44=1.2, a 20% increase.
Solution
The rms speed of gas molecules is
vrms=M3RT ∝ T,
with T in kelvin.
Convert the temperatures:
T1=27∘C=300K,T2=159∘C=432K.
Ratio of speeds:
v1v2=T1T2=300432=1.44=1.2. …
- TG EAPCET 2023Set eng-2023-05-14-FN1 markMCQQ.Heavy water is used as moderator in nuclear reactor because (A) It controls the energy released in the reactor (B) It absorbs neutrons and stops chain reaction (C) It cools the reactor faster (D) It slows down the fast moving neutrons
›Reveal solutionSolution
Heavy water slows down fast neutrons via elastic collisions without absorbing them, making it an ideal moderator. The correct option is (D).
Concept and Intuition
In a nuclear reactor, the fuel (e.g., uranium-235) fissions most efficiently when struck by slow (thermal) neutrons. The neutrons released from fission are very fast — about 2 MeV of kinetic energy. A moderator is a material placed in the reactor to reduce the speed of these fast neutrons to thermal energies (around 0.025 eV) through repeated collisions, without absorbing them. Heavy water (D₂O) is excellent at this because its deuterium nucleus has nearly the same mass as a neutron, allowing maximum energy transfer per collision, and it has a very low neutron absorption cross-section.
Step-by-Step Reasoning
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Identify the role of a moderator
A moderator’s job is to slow down fast neutrons so they can cause further fission. It does not control the overall energy release (that’s the job of control rods), nor does it absorb neutrons to stop the chain reaction (that would be a poison or control rod), nor is its primary purpose cooling (that’s the coolant). So options (A), (B), and (C) are incorrect by definition.
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Why heavy water slows neutrons effectively
When a neutron collides elastically with a nucleus, the energy lost per collision is greatest when the target nucleus has a mass close to the neutron’s. Deuterium (²H) has a mass of about 2 u, while a neutron is about 1 u. This near-match means each collision can transfer a large fraction of the neutron’s kinetic energy. Ordinary water (H₂O) has hydrogen (mass 1 u), which is even better for slowing, but hydrogen absorbs neutrons too readily (forming deuterium), which would reduce the neutron population. Heavy water’s deuterium absorbs neutrons far less.
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Eliminate the distractors
- (A) “Controls the energy released” — This is done by control rods (e.g., boron or cadmium) that absorb excess neutrons. The moderator merely sustains the chain reaction by slowing neutrons.
- (B) “Absorbs neutrons and stops chain reaction” — Heavy water is chosen precisely because it does not absorb many neutrons. Absorbing would stop the reaction, which is undesirable. …
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- TG EAPCET 2022Set ap-2022-07-31-FN1 markMCQQ.Match the columns for the first law of thermodynamics Column - I A) Adiabatic processes B) Constant - volume processes C) Isothermal processes D) Constant - pressure processes Column - II I) W=0, ΔEint=Q II) Q=W; ΔEint=0 III) Q=0; ΔEint=−W IV) W=0; ΔEint=Q (W – work done, Q - heat absorbed, ΔEint - change of internal energy) The correct match is (A) A B C D III II IV I (B) A B C D III IV II I (C) A B C D IV I III II (D) A B C D I III IV II
›Reveal solutionSolution
The first law of thermodynamics, ΔEint=Q−W, is applied to four special processes. Matching each process to its characteristic conditions gives the sequence A→III, B→IV, C→II, D→I, which corresponds to option (B).
The first law of thermodynamics is the energy‑conservation statement for thermodynamic systems:
ΔEint=Q−W,
where Q is heat added to the system, W is work done by the system, and ΔEint is the change in internal energy.
Each special process imposes a constraint (e.g., constant volume, no heat exchange), which simplifies the first law in a characteristic way. The trick is to remember the definition of each process and then substitute into the first law.
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Adiabatic processes (A)
Definition: No heat exchange with the surroundings → Q=0.
First law becomes ΔEint=−W.
Work is generally nonzero (e.g., compression or expansion).
So A matches III: Q=0; ΔEint=−W.
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Constant‑volume processes (B)
Definition: Volume does not change → W=∫PdV=0.
First law becomes ΔEint=Q.
Heat can flow in or out, changing internal energy directly.
So B matches IV: W=0; ΔEint=Q.
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Isothermal processes (C)
Definition: Temperature is constant → for an ideal gas, ΔEint=0 (internal energy depends only on temperature).
First law gives 0=Q−W → Q=W.
Work is generally nonzero (e.g., isothermal expansion).
So C matches II: Q=W; ΔEint=0.
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Constant‑pressure processes (D)
Definition: Pressure is constant; work done is W=PΔV, which is generally nonzero.
Heat Q is also nonzero, and internal energy changes because temperature changes. …
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- TG EAPCET 2022Set eng-2022-07-19-AN1 markMCQQ.An ideal gas at pressure P0 undergoes an isothermal expansion until its volume is 8.0 times its initial volume. The gas is slowly and adiabatically compressed back to its original volume. If the adiabatic constant of the gas is γ=4/3, then the ratio of the average kinetic energy per molecule in this final state to that in the initial state is (A) 1.44 (B) 1.68 (C) 2.0 (D) 1.2
›Reveal solutionSolution
An ideal gas undergoes isothermal expansion followed by adiabatic compression. The average kinetic energy per molecule is directly proportional to the absolute temperature. The isothermal process keeps the temperature constant, while the adiabatic compression increases the temperature. The final temperature is twice the initial temperature, so the ratio of average kinetic energy per molecule in the final state to the initial state is 2.0.
The average kinetic energy per molecule of an ideal gas is directly proportional to its absolute temperature. This is a fundamental concept in the kinetic theory of gases. Therefore, to find the ratio of the average kinetic energy per molecule in the final state to that in the initial state, we need to determine the ratio of the final absolute temperature to the initial absolute temperature.
We will analyze the process in two stages:
- Isothermal Expansion: The temperature remains constant.
- Adiabatic Compression: The temperature changes according to the adiabatic relation.
Let's denote the initial state as state 1, the intermediate state (after isothermal expansion) as state 2, and the final state (after adiabatic compression) as state 3.
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Initial State (State 1):
Let the initial pressure, volume, and temperature be P1=P0, V1=V0, and T1=T0, respectively.
The average kinetic energy per molecule in this state is KE1∝T0.
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Isothermal Expansion (State 1 to State 2):
In an isothermal process, the temperature of the gas remains constant.
ImportantFor an isothermal process, T=constant.
The gas expands until its volume is 8.0 times its initial volume.
So, V2=8.0V0.
Since the process is isothermal, the temperature at state 2 is the same as at state 1:
T2=T1=T0.
The average kinetic energy per molecule in this state is KE2∝T0.
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Adiabatic Compression (State 2 to State 3):
The gas is slowly and adiabatically compressed back to its original volume.
ImportantFor an adiabatic process, PVγ=constant or TVγ−1=constant.
The compression starts from state 2 (V2=8V0, T2=T0) and ends at state 3, where the volume is the original volume, V3=V0.
We use the adiabatic relation involving temperature and volume:
[!FORMULA]
TVγ−1=constant
Applying this between state 2 and state 3:
T2V2γ−1=T3V3γ−1
Substitute the known values:
T0(8V0)γ−1=T3(V0)γ−1
To find T3, rearrange the equation:
T3=T0(V08V0)γ−1
T3=T0(8)γ−1
We are given the adiabatic constant γ=4/3.
Calculate γ−1: …
- TG EAPCET 2022Set eng-2022-07-20-AN1 markMCQQ.Statement I : A device in which heat measurement can be made is called calorimeter. Statement II : Skating is possible on snow due to the formation of water below the skates. Water is formed due to the increase of temperature and ice melts. Statement III: Two bodies at different temperature are mixed in a calorimeter. Total internal energy of the two bodies remains conserved. Which of the following is correct? (A) Statements I, II and III are true (B) Statement I is true, but statements II and III are false (C) Both statements I and II are true, but statement III is false (D) Both statements I, III are true, but statement II is false
›Reveal solutionSolution
We need to evaluate three statements about calorimetry and phase transitions. Statement I (calorimeter definition) is true, Statement II (skating mechanism) is false because it misidentifies the cause of ice melting, and Statement III (energy conservation in calorimetry) is true. The correct option is (D).
Let me analyze each statement carefully to understand the physics involved.
Statement I: Definition of a Calorimeter
A calorimeter is indeed a device designed to measure heat transfer. The name comes from "calor" (heat) and "meter" (to measure). This is a straightforward definition and is TRUE.
Statement II: The Physics of Ice Skating
This statement claims that skating is possible because increased temperature melts the ice. Let's examine this critically:
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The traditional explanation (which this statement reflects) suggested that pressure from the skate blade lowers the melting point of ice, causing it to melt and form a lubricating water layer.
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Modern understanding shows this is incorrect for typical skating conditions. The pressure-melting effect is negligible at normal skating temperatures (around -5°C to 0°C). The pressure from a skate can only lower the melting point by about 0.5°C, which is insufficient.
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The actual mechanism involves frictional heating and a pre-existing quasi-liquid layer that exists on ice surfaces even below 0°C due to surface molecular mobility.
The statement says water forms "due to the increase of temperature" without mentioning the actual mechanism (friction), and implies this is primarily a pressure effect. This is FALSE or at best misleading.
Watch outThe pressure-melting explanation for ice skating is a common misconception found in many textbooks, but modern research has shown it's not the primary mechanism at typical skating temperatures.
Statement III: Energy Conservation in Calorimetry
When two bodies at different temperatures are mixed in an isolated calorimeter:
- The system is thermally isolated from the surroundings (that's the purpose of a calorimeter). …
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- TG EAPCET 2022Set ap-2022-07-31-AN1 markMCQQ.A hole is drilled at the center of a metallic plate. If the metal plate is heated, then the size of the hole will be (A) Expanding (B) Contracting (C) Remains same (D) Not predicted
›Reveal solutionSolution
When a metal plate is heated uniformly, every linear dimension — including the diameter of a hole — expands according to the same coefficient of linear expansion. The hole expands.
The key idea is that thermal expansion is a property of the material itself, not of the shape. When you heat a uniform metal plate, the atoms vibrate more and the average distance between them increases. This happens everywhere in the plate — in the solid region and along the boundary of the hole. The hole is not a separate object; it is simply the absence of metal. The metal around the hole expands outward, making the hole larger.
A common mistake is to think the hole "fills in" as the metal expands inward. That would only happen if the plate were heated from the outside inward, but here the heating is uniform. Every point on the rim of the hole moves away from the center because the material between that point and the center expands.
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Think of the hole as being defined by a circle of metal atoms. If you mark a circle on the plate and then heat it, the circumference of that circle increases. Since circumference = πd, the diameter d must also increase.
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Use the linear expansion formula. For a small temperature change ΔT, the change in any linear dimension L is ΔL=αLΔT, where α is the coefficient of linear expansion. This applies to the diameter of the hole just as it applies to the outer diameter of the plate. …
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- TG EAPCET 2022Set ap-2022-07-31-AN1 markMCQQ.A gaseous mixture consists of molecules of type A, B and C with masses MA>MB>MC. The correct relation between their average kinetic energy is (A) KA>KB>KC (B) KA<KB<KC (C) KA=KB=KC (D) KA=KB<KC
›Reveal solutionSolution
The average kinetic energy of gas molecules in a mixture depends only on the absolute temperature of the mixture, not on the individual masses of the molecules. Since all components of a gaseous mixture are at the same temperature, their average kinetic energies are equal. The correct option is (C).
The core concept here comes from the kinetic theory of gases, which describes the macroscopic properties of gases in terms of the microscopic behavior of their molecules. A fundamental postulate of this theory is that the absolute temperature of an ideal gas is a direct measure of the average translational kinetic energy of its molecules.
When different gases are mixed together, they quickly reach thermal equilibrium. This means that all components of the mixture will be at the same temperature. If the temperature is the same for all types of molecules in the mixture, then their average kinetic energies must also be the same, regardless of their individual masses.
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Understanding Average Kinetic Energy: For an ideal gas, the average translational kinetic energy per molecule is directly proportional to the absolute temperature of the gas. This is a key result from the kinetic theory.
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The Formula: The average translational kinetic energy (Kavg) of a single molecule in an ideal gas is given by:
Kavg=23kBT
where kB is the Boltzmann constant (a universal constant) and T is the absolute temperature of the gas in Kelvin.
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Applying to the Mixture: In the given problem, we have a gaseous mixture consisting of molecules of type A, B, and C. Since they are all part of the same mixture, they are in thermal equilibrium with each other. This implies that all three types of molecules (A, B, and C) are at the same absolute temperature, T.
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Comparing Kinetic Energies:
- For molecule type A, the average kinetic energy is KA=23kBT.
- For molecule type B, the average kinetic energy is KB=23kBT. …
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- TG EAPCET 2021Set ap-2021-08-09-FN1 markMCQQ.An ideal gas at temperature T & pressure P fills the chamber A which is separated from chamber B which has vacuum. The two chambers are thermally insulated. When plug is removed the gas fills both the chambers. Both A & B have same volume. What will be the pressure & temperature of the gas after it comes to equilibrium.? (A) P,T (B) P/2,T (C) P/2,T/2 (D) P,T/2
›Reveal solutionSolution
The gas undergoes free expansion into a vacuum, which is an irreversible adiabatic process. For an ideal gas, internal energy depends only on temperature, so temperature remains constant; pressure halves because volume doubles. The correct option is (B).
The key concept here is free expansion (also called Joule expansion). When a gas expands into a vacuum, it does no work (no opposing pressure) and, because the container is thermally insulated, no heat is exchanged. The first law of thermodynamics says ΔU=Q−W. Here Q=0 and W=0, so ΔU=0. For an ideal gas, internal energy U depends only on temperature, so constant U means constant T.
Now, let’s walk through the reasoning step by step.
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Identify the process.
The gas is initially in chamber A at pressure P and temperature T. Chamber B is evacuated. When the plug is removed, the gas rushes into B. This is free expansion — the gas expands against zero external pressure, so no work is done (W=0). The walls are thermally insulated, so no heat flows (Q=0).
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Apply the first law.
ΔU=Q−W=0−0=0. The internal energy of the ideal gas does not change.
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Relate internal energy to temperature.
For an ideal gas, U=nCVT, where n is the number of moles and CV is the molar heat capacity at constant volume. Since ΔU=0, we have nCVΔT=0, so ΔT=0. Thus the final temperature remains T.
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Find the final pressure. …
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- TG EAPCET 2021Set ap-2021-08-09-FN1 markMCQQ.The rms speed of H2 molecules is C at 27∘C. The molecules break into atoms. What should be the new temperature such that atoms have same speed as molecules (Assume the mass of H2 molecules is twice the mass of H- atom) (A) 600 K (B) 150 K (C) 100 K (D) 300 K
›Reveal solutionSolution
The key idea is that rms speed depends on temperature and mass: vrms=3kT/m. For the same speed, the product mT must be constant. Since an H atom has half the mass of H₂, the temperature must be halved from 300 K to 150 K. The correct option is (B).
Concept and Intuition
The root-mean-square speed of gas molecules is given by vrms=m3kT, where k is Boltzmann’s constant, T is absolute temperature, and m is the mass of one molecule. If we want the atoms (each of mass matom) to have the same rms speed as the original molecules (each of mass mmolecule=2matom), then the temperature must adjust to compensate for the mass change. Since vrms is proportional to T/m, keeping vrms constant means T/m must stay constant — so T must scale with m.
Step-by-step solution
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Convert given temperature to Kelvin
The problem states 27∘C.
Tinitial=27+273=300 K.
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Write the rms speed for H₂ molecules
Let m be the mass of an H atom. Then the mass of an H₂ molecule is 2m.
The rms speed of H₂ at 300 K is
vrms, H₂=2m3k⋅300.
- Write the rms speed for H atoms at unknown temperature T Each H atom has mass m.
vrms, H=m3kT.
- Set the speeds equal We require vrms, H=vrms, H₂, so m3kT=2m3k⋅300. …
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