Q.It is found experimentally that 13.6 eV energy is required to separate a hydrogen atom into a proton and an electron. Compute the orbital radius and the velocity of the electron in a hydrogen atom.
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🔒 Start your 14-day free trial to unlock the full solution →Concept understanding — Bohr Model Quantization
Why does an electron not spiral into the nucleus?
Imagine you're pushing a child on a swing. If you push at random moments, the swing jerks and slows down. But if you push exactly in rhythm with the swing's natural motion, each push adds energy smoothly and the swing goes higher and higher. The swing "prefers" to move at specific frequencies — its natural modes.
An electron orbiting a nucleus is similar, but with a crucial twist from the quantum world. Classical physics says an accelerating charge (like an electron going in a circle) must continuously radiate energy. If that were true, the electron would lose energy, spiral into the nucleus, and atoms would collapse in a flash of light. But atoms are stable. So something is fundamentally different.
The radical idea: allowed orbits only
Niels Bohr proposed in 1913 that the electron cannot occupy just any orbit. It can only exist in certain stationary states — orbits where it does not radiate energy. These are like the swing's natural frequencies, but for an electron.
The key condition that picks out these special orbits is called quantization of angular momentum.
L=n2πh,n=1,2,3,…
Here L is the orbital angular momentum of the electron, h is Planck's constant, and n is a positive integer called the principal quantum number.
What this means physically
Angular momentum for a circular orbit is L=mvr, where m is the electron mass, v its speed, and r the orbit radius. So the quantization condition becomes:
mvr=n2πh
This is not a formula you derive — it is a postulate, a rule that nature follows. Bohr had no deeper explanation for why this rule works; he simply noticed it gave the right answers for hydrogen's spectrum.
The quantity 2πh appears so often that it has its own symbol: ℏ (h-bar). So the condition is often written as L=nℏ.
What it predicts
Combining this quantization with Newton's law for circular motion (centripetal force = Coulomb attraction) gives:
- Radius of the nth orbit: rn=n2a0, where a0=0.529A˚ is the Bohr radius (the smallest orbit, n=1).
- Energy of the nth orbit: En=−n213.6eV
The negative sign means the electron is bound to the nucleus. As n increases, the orbit gets larger and the energy becomes less negative (closer to zero).
The key insight for exams
Bohr quantization is not a derivation — it is a condition you apply. When you see a problem about hydrogen-like atoms (one electron), you:
- Write mvr=nℏ
- Write the force balance: rmv2=r2kZe2 (for nuclear charge Ze)
- Solve for r and v in terms of n …
Why this formula?
Why Angular Momentum is Quantised in the Bohr Model
The Bohr model's most famous result — that angular momentum comes only in integer multiples of 2πh — is not an arbitrary assumption. It follows directly from a single, elegant idea: the electron's wave must close on itself.
The core problem Bohr faced
By 1913, physicists knew two things that seemed contradictory:
- Rutherford's nuclear model showed electrons orbiting the nucleus.
- Maxwell's equations predicted that any accelerating charge (like an orbiting electron) must radiate energy, spiral inward, and collapse in about 10−11 seconds.
Atoms are stable. Something was missing.
Bohr's breakthrough was to combine the newly discovered quantum idea (Planck's constant h) with classical mechanics, but only for allowed orbits. The key constraint came from thinking of the electron not as a tiny planet, but as a standing wave.
The de Broglie wavelength argument (the cleanest derivation)
A few years after Bohr, de Broglie proposed that every moving particle has a wavelength:
λ=ph=mvh
For an electron in a circular orbit of radius r, the circumference is 2πr. For the wave to be stable — not cancelling itself out — the circumference must contain an integer number of wavelengths:
2πr=nλ,n=1,2,3,…
Substitute λ=h/(mv):
2πr=n⋅mvh
Rearrange:
mvr=n⋅2πh
That's it. The left side mvr is the angular momentum L. So:
L=nℏ,where ℏ=2πh
This is not a separate postulate — it is a consequence of requiring the electron wave to be a standing wave. If the wave doesn't close on itself, it interferes destructively and the orbit cannot exist.
Why this fixes the energy levels
Once angular momentum is quantised, the rest follows from classical physics. For a circular orbit, the centripetal force is provided by the Coulomb attraction:
rmv2=4πϵ01r2e2
Combine this with mvr=nℏ and solve for r and E:
rn=me24πϵ0ℏ2⋅n2=a0n2
En=−8ϵ02h2me4⋅n21=−n213.6 eV …
The key idea is that the 13.6 eV binding energy equals the magnitude of the total energy E of the electron in the ground state of hydrogen. For a circular orbit, the total energy is half the potential energy: E=−2rke2.
Step 1: Convert the binding energy to joules.
13.6 eV=13.6×1.6×10−19=2.176×10−18 J
Since E=−13.6 eV, we have ∣E∣=2rke2.
Step 2: Solve for the orbital radius r.
r=2∣E∣ke2=2×2.176×10−18(9×109)(1.6×10−19)2
r=4.352×10−189×2.56×10−29=4.352×10−182.304×10−28=5.29×10−11 m
Step 3: Find the velocity using mv2/r=ke2/r2, so v=mrke2. …
The problem uses the experimentally measured ionization energy (13.6 eV) to deduce the electron's orbital radius and velocity in the Bohr model. The key is equating the ionization energy to the total energy of the electron in the ground state, then using Bohr's quantization condition. The orbital radius comes out to 5.29×10−11 m and the velocity to 2.19×106 m/s.
The 13.6 eV given is not just any number — it is the ionization energy, the minimum energy needed to completely remove the electron from the proton's influence. In the Bohr model, this equals the negative of the total energy of the electron in the n=1 orbit. So the electron's total energy in the ground state is −13.6 eV.
Why does this help? Because in the Bohr model, the total energy, orbital radius, and velocity are all linked by simple relations. If we know one, we can find the others. The trick is to work in SI units consistently — convert eV to joules, then use Coulomb's law and Newton's second law alongside Bohr's angular momentum quantization.
Let's go step by step.
1. Convert the given energy to joules
The ionization energy is 13.6 eV. Since 1 eV=1.602×10−19 J:
Eion=13.6×1.602×10−19=2.179×10−18 J
This is the magnitude of the total energy ∣E∣ of the electron in the ground state. In the Bohr model, the total energy is negative (bound state), so:
E=−2.179×10−18 J
A common mistake is to forget the negative sign. The total energy of a bound electron is negative; the ionization energy is the positive amount needed to bring it to zero energy. So E=−13.6 eV, not +13.6 eV.
2. Recall the Bohr model relations for hydrogen
For an electron in a circular orbit around a proton, two equations hold:
- Newton's second law (Coulomb force provides centripetal acceleration):
4πε01r2e2=rmv2
- Bohr's quantization of angular momentum (for the ground state, n=1):
mvr=2πh
Here m=9.109×10−31 kg (electron mass), e=1.602×10−19 C, ε0=8.854×10−12 F/m, and h=6.626×10−34 J⋅s.
The total energy of the electron in the n-th Bohr orbit is:
En=−8ε02h2me4⋅n21
For n=1, this gives E1=−13.6 eV — which is exactly our starting point.
3. Use the total energy to find the radius
The total energy is the sum of kinetic and potential energies:
E=21mv2−4πε01re2
From the centripetal equation, we have rmv2=4πε01r2e2, which gives:
mv2=4πε01re2
So the kinetic energy K=21mv2=21⋅4πε01re2.
The potential energy U=−4πε01re2.
Therefore:
E=K+U=21⋅4πε01re2−4πε01re2=−21⋅4πε01re2
This is a neat result: the total energy is exactly half the potential energy (and the negative of the kinetic energy). Rearranging for r:
r=−21⋅4πε01Ee2
Since E is negative, r comes out positive. Plug in the numbers:
r=−21⋅4π(8.854×10−12)1⋅−2.179×10−18(1.602×10−19)2
First compute 4πε01=8.988×109 N⋅m2/C2. Then:
r=21×8.988×109×2.179×10−182.566×10−38 …
Method: Bohr Model for Hydrogen Atom
This problem uses the Bohr model of the hydrogen atom, which combines classical circular motion with quantised angular momentum. The key idea is that the electron orbits the proton in a circle, held by electrostatic attraction, but only certain orbits are allowed — those where the angular momentum is an integer multiple of 2πh.
Step 1: Write the energy condition
The total energy of the electron in the n=1 orbit (ground state) is given as 13.6 eV. This is the ionisation energy — the energy needed to remove the electron completely. In the Bohr model, the total energy is:
E=−2rke2
where k=4πϵ01=9×109 N m2/C2, e=1.6×10−19 C, and r is the orbital radius. The negative sign means the electron is bound.
Since ∣E∣=13.6 eV, we have:
2rke2=13.6 eV
Convert 13.6 eV to joules: 13.6×1.6×10−19=2.176×10−18 J.
Step 2: Solve for the orbital radius r
From the energy equation:
r=2Eke2
Substitute values:
r=2×2.176×10−18(9×109)(1.6×10−19)2
r=4.352×10−189×109×2.56×10−38
r=4.352×10−182.304×10−28
r=5.29×10−11 m
This is the Bohr radius (a0), a fundamental constant in atomic physics.
Step 3: Find the velocity v
The centripetal force is provided by the electrostatic attraction:
rmv2=r2ke2
Cancel one r:
mv2=rke2
So: …
Common Mistakes in Rutherford/Bohr Radius & Velocity Problems
This question is a classic — it tests whether you truly understand the link between energy, radius, and velocity in the Bohr model. Most students jump straight to formulas without connecting the given energy to the right physical quantity.
Mistake 1: Confusing the given 13.6 eV with kinetic energy
The most frequent error: students see 13.6 eV and immediately plug it into Ek=21mv2 to find velocity. But 13.6 eV is the total energy (or the ionization energy), not the kinetic energy.
Why this happens: The problem says "energy required to separate" — that's the binding energy, which equals the magnitude of the total energy of the electron in the ground state. In the Bohr model:
Etotal=−n213.6 eV
For n=1, Etotal=−13.6 eV. The kinetic energy is +13.6 eV, and the potential energy is −27.2 eV.
Never equate the given ionization energy directly to 21mv2. The kinetic energy is positive and equal in magnitude to the total energy, but the total energy itself is negative.
How to avoid: Always write down the three energy relations side by side before substituting numbers:
- Etotal=−2rke2 (or −13.6/n2 eV)
- Ek=2rke2=+13.6 eV (for n=1)
- Ep=−rke2=−27.2 eV
Mistake 2: Using the wrong value of e (electronic charge)
Students often use e=1.6×10−19 C but forget to square it when it appears as e2 in formulas. Or they mix up e with the charge on the nucleus (Ze), but here Z=1.
How to avoid: Write the formula with e2 explicitly, then substitute e=1.6×10−19 C and square it immediately. Keep units consistent — use SI units throughout.
Mistake 3: Forgetting to convert eV to joules
The given energy is in electronvolts, but the Coulomb constant k=9×109 and other quantities are in SI units. If you plug 13.6 directly without converting to joules, your radius will be off by a factor of 1019.
1 eV=1.6×10−19 J, so 13.6 eV=13.6×1.6×10−19=2.176×10−18 J.
How to avoid: Before starting any calculation, convert all energies to joules. Write the conversion step explicitly.
Mistake 4: Using the wrong formula for orbital radius
Some students try to derive radius from F=rmv2 alone, forgetting they need a second equation (either energy quantization or angular momentum quantization). Without Bohr's postulate, you cannot get a unique radius.
The correct approach: Use the total energy relation:
Etotal=−2rke2
Since ∣Etotal∣=13.6 eV=2.176×10−18 J, we have:
2rke2=2.176×10−18
Solve for r:
r=2×2.176×10−18ke2
r=2∣Etotal∣ke2
Mistake 5: Computing velocity from the wrong energy
After finding r, students sometimes use Ek=21mv2 but plug in the total energy value (negative) instead of the kinetic energy magnitude. …
- COMEDK 2026Set 2026-A1 markMCQQ.What is the frequency of the electron in the first orbit of hydrogen atom of orbital radius 0.5×10−10 m, if its orbital velocity in that orbit is 2.2×106 ms−1. (A) 3.49×1015 Hz (B) 3.49×1013 Hz (C) 6.98×1015 Hz (D) 6.98×1013 Hz
›Reveal solutionSolution
The frequency of an electron in a circular orbit is the number of revolutions per second, found by dividing the orbital speed by the circumference of the orbit. Using the given values, the frequency is approximately 7.0×1015Hz, which matches option (C).
The key idea here is that the electron in the first orbit of hydrogen moves in a circular path. Its frequency is simply how many times it goes around the circle per second — that is, the orbital speed divided by the circumference of the orbit. This is a direct application of the relation between speed, radius, and frequency for uniform circular motion.
- Recall the relationship between speed, radius, and frequency For an object moving in a circle of radius r with constant speed v, the time for one complete revolution (the period T) is the distance around the circle divided by the speed:
T=v2πr
The frequency f is the reciprocal of the period:
f=T1=2πrv
- Plug in the given values
We are told:
- Orbital radius r=0.5×10−10m
- Orbital velocity v=2.2×106m/s So:
f=2π×(0.5×10−10)2.2×106
- Simplify step by step First, compute the denominator:
2π×0.5×10−10=π×10−10
(since 2×0.5=1).
So:
f=π×10−102.2×106=π2.2×1016
- Evaluate numerically Using π≈3.1416:
3.14162.2≈0.7003
Thus:
f≈0.7003×1016=7.003×1015Hz
- Match with the options …
- COMEDK 2025Set 2025-A1 markMCQQ.What is the frequency ' ν ' of the electron in Bohr's first orbit of radius ' r ' of the hydrogen atom? (A) v=4πε0hre2 (B) v=2πε0hr2e2 (C) v=4πε0hr2e2 (D) v=2πε0hre2
›Reveal solutionSolution
Using the first-orbit speed v=2ε0he2 and ν=2πrv gives ν=4πε0hre2 — option (A).
For the electron in Bohr's first orbit, the orbital speed follows from combining the Coulomb–centripetal balance with angular-momentum quantization (mvr=2πh):
v=2ε0he2. …
- COMEDK 2025Set 2025-A1 markMCQQ.What is the kinetic energy of the electron in the nth level, moving in a plane under the influence of a magnetic field ' B '? [ m -mass of electron; h - Planck's constant; e- electronic charge] (A) 4πnmheB (B) 4πmnheB (C) 2πmnheB (D) 2πnmheB
›Reveal solutionSolution
The kinetic energy of an electron in the nth Landau level under a magnetic field B is quantized; using the Bohr quantization of angular momentum in a circular orbit, the result is 4πmnheB, which corresponds to option (B).
Concept & Intuition
When an electron moves perpendicular to a uniform magnetic field, it experiences a centripetal Lorentz force and follows a circular path. In quantum mechanics, the angular momentum of such an orbit is quantized in units of ℏ=h/(2π). This is analogous to Bohr’s quantization for atomic orbits, but here the centripetal force is magnetic rather than electrostatic. The kinetic energy is purely the energy of circular motion, and we can find it by combining the force balance with the quantization condition.
Step-by-step reasoning
- Force balance for circular motion For an electron of mass m and charge e moving with speed v in a circle of radius r perpendicular to a uniform magnetic field B, the magnetic (Lorentz) force provides the centripetal force:
evB=rmv2
Cancelling one v gives:
eB=rmv⇒v=meBr
- Quantization of angular momentum Bohr’s postulate for a stationary orbit states that the angular momentum is an integer multiple of ℏ=h/(2π):
mvr=nℏ=2πnh
Substitute v from step 1 into this:
m(meBr)r=eBr2=2πnh
Hence the radius is:
r2=2πeBnh
- Kinetic energy expression Kinetic energy is K=21mv2. Using v=eBr/m from step 1:
- COMEDK 2025Set 2025-E1 markMCQQ.Which of the following is correct in the case of the Bohr model of atoms? A. Predicts continuous emission spectra for all atoms B. Assumes that the angular momentum of electrons is quantised C. Predicts same emission spectrum for singly ionised neon atom and hydrogen atom D. Predicts same emission spectrum for singly ionised neon atom and singly ionised helium atom (A) C (B) B (C) A (D) D
›Reveal solutionSolution
The Bohr model is built on the quantisation of angular momentum, which leads to discrete energy levels and line spectra. The correct statement is that it assumes angular momentum is quantised — option (B).
The Bohr model of the atom was a revolutionary step in explaining why atoms emit only specific frequencies of light. The key insight is that classical physics would allow an electron to spiral into the nucleus, emitting a continuous spectrum. Bohr fixed this by imposing a quantisation condition: the electron’s angular momentum can only take certain discrete values. This single assumption leads to fixed orbits, discrete energy levels, and thus a line spectrum — not a continuous one.
Let’s examine each option carefully.
-
Option A: “Predicts continuous emission spectra for all atoms”
This is false. The Bohr model explicitly predicts discrete (line) spectra, not continuous. A continuous spectrum would come from a free electron radiating energy as it spirals in — exactly what Bohr’s quantisation prevents. So A is wrong.
-
Option B: “Assumes that the angular momentum of electrons is quantised”
This is the core postulate of the Bohr model. Bohr stated that the electron’s angular momentum L must be an integer multiple of ℏ=h/(2π):
L=nℏ,n=1,2,3,…
This quantisation is what gives rise to stable orbits and discrete energy levels. So B is correct.
- Option C: “Predicts same emission spectrum for singly ionised neon atom and hydrogen atom” Singly ionised neon (Ne⁺) has 9 electrons, while hydrogen has 1. The Bohr model works well only for one-electron systems (like H, He⁺, Li²⁺). For Ne⁺, the remaining electrons screen the nucleus and interact with each other, so the simple Bohr formula fails. Even if we considered a one-electron ion, the nuclear charge Z differs: for H, Z=1; for Ne⁺, Z=10. The energy levels scale as Z2, so the spectra are completely different. Thus C is false. …
-
- COMEDK 2025Set 2025-M1 markMCQQ.According to Bohr's theory of hydrogen atom, the speed of the electron, its energy and radius of its orbit vary with the principal quantum number n, respectively as (A) n1,n2,n21 (B) n1,n21,n2 (C) n,n21,n2 (D) n21,n1,n2
›Reveal solutionSolution
In Bohr’s model, the electron’s speed varies as 1/n, its energy as 1/n2, and the orbital radius as n2. The correct matching is option (B).
The key idea is that Bohr’s model quantizes angular momentum:
mvr=n2πh
and the Coulomb force provides the centripetal force:
r2ke2=rmv2
From these two equations, we can solve for v, r, and the total energy E in terms of n. The dependencies are not arbitrary — they follow directly from combining these relations.
- Find how radius r depends on n. From the angular momentum condition: v=2πmrnh. Substitute into the force equation:
r2ke2=m⋅r1(2πmrnh)2
Simplify:
r2ke2=4π2mr3n2h2
Multiply both sides by r3:
ke2r=4π2mn2h2
So
r=4π2mke2n2h2∝n2
Thus radius ∝n2.
- Find how speed v depends on n. From angular momentum: v=2πmrnh. Since r∝n2, we get
v∝n2n=n1
So speed ∝1/n.
- Find how total energy E depends on n. Total energy = kinetic + potential:
E=21mv2−rke2
Using the force equation r2ke2=rmv2, we have mv2=rke2.
Then kinetic energy = 21mv2=2rke2.
So
E=2rke2−rke2=−2rke2 …
- COMEDK 2024Set 2024-A1 markMCQQ.In a hydrogen atom, if electron is replaced by a particle which is 40 times heavier but has the same charge, then, the ratio of the radius of the first excited state of a normal hydrogen atom to the ground state of the above atom is (A) 40 : 1 (B) 1 : 160 (C) 1 : 40 (D) 160 : 1
›Reveal solutionSolution
The key idea is that the Bohr radius scales inversely with the reduced mass of the electron-nucleus system. Replacing the electron with a particle 40 times heavier reduces the radius by a factor of 40. The first excited state of normal hydrogen (n=2) has radius 4 times the ground state. The ratio asked is (normal H, n=2) : (heavy particle, n=1) = 4 : (1/40) = 160 : 1. So the answer is (D).
The problem is about how the size of an atom changes when the orbiting particle’s mass changes. In the Bohr model, the radius of an orbit depends on the reduced mass of the two-body system (nucleus + orbiting particle). Most students forget that the electron’s mass appears in the denominator of the radius formula — so a heavier particle actually orbits closer to the nucleus. Let’s walk through it carefully.
- Recall the Bohr radius formula for a hydrogen-like atom For a nucleus of charge +Ze and an orbiting particle of mass m and charge −e, the radius of the n-th orbit is:
rn=πme2Zn2h2ε0
But this formula assumes the nucleus is infinitely heavy. In reality, the electron and nucleus both orbit their common centre of mass, so we must use the reduced mass μ:
μ=m+MmM
where m is the orbiting particle’s mass and M is the nucleus mass. For hydrogen, M≈1836me, so μ≈me. The correct radius is:
rn=πμe2Zn2h2ε0
So the radius is inversely proportional to the reduced mass.
- What changes in the problem?
- Normal hydrogen: orbiting particle is an electron of mass me, nucleus is a proton of mass mp. Reduced mass μH≈me (since mp≫me).
- Modified atom: orbiting particle has mass 40me (same charge −e), nucleus is still a proton. The new reduced mass is:
μ′=40me+mp(40me)mp
Since $m_p \approx 1836 m_e$, the denominator is dominated by $m_p$, so:μ′≈mp40memp=40me
More precisely, $\mu'$ is very close to $40 m_e$ because the proton is still much heavier than the new particle. So the reduced mass increases by a factor of about 40.3. Effect on the ground state radius
For the modified atom in its ground state (n=1):
r1′∝μ′1≈40me1 …
- COMEDK 2024Set 2024-E1 markMCQQ.An electron has a mass of 9.1×10−31 kg. It revolves round the nucleus in a circular orbit of radius 0.529×10−10 m at a speed of 2.2×106 ms−1. The magnitude of its angular momentum is (A) 1.06×10−34Kgm2 s−1 (B) 1.06×10−24Kgm2 s−1 (C) 2.06×10−34Kgm2 s−1 (D) 2.06×10−24Kgm2 s−1
›Reveal solutionSolution
Angular momentum for a point mass in circular motion is L=mvr. Substituting the given values yields L≈1.06×10−34kgm2/s, which matches option (A).
The concept here is angular momentum of a particle in circular motion. For a point mass moving in a circle, the magnitude of its orbital angular momentum about the center is simply the product of its linear momentum (mv) and the radius (r), because the velocity is perpendicular to the radius vector. This is a direct application of L=mvr, not requiring integration or calculus.
- Identify the formula: For a particle of mass m moving with speed v in a circle of radius r, the angular momentum about the center is
L=mvr.
This works because the angle between the velocity and the radius is 90∘, so sin90∘=1.
- Plug in the given values:
m=9.1×10−31kg,v=2.2×106m/s,r=0.529×10−10m.
- Multiply step by step (keeping track of powers of 10): First, multiply the coefficients:
9.1×2.2=20.02,then20.02×0.529≈10.59.
(More precisely: 20.02×0.5=10.01, plus 20.02×0.029≈0.5806, sum ≈10.5906.)
- Combine the powers of ten:
10−31×106×10−10=10−31+6−10=10−35.
So the product is approximately
10.59×10−35=1.059×10−34.
- Round to three significant figures (since all inputs have two or three significant figures): L≈1.06×10−34kgm2/s. …
- KCET 2021Set B-21 markMCQQ.Energy of an electron in the second orbit of hydrogen atom is E2. The energy of electron in the third orbit of He+ will be (A) 169E2 (B) 916E2 (C) 163E2 (D) 316E2
›Reveal solutionSolution
Apply En∝Z2/n2 to both cases and take the ratio — the answer is 916E2.
Step 1 — The Bohr energy formula for a hydrogen-like species
For any one-electron (hydrogen-like) atom or ion with nuclear charge Z:
En=−13.6n2Z2 eV
The Z2 arises because a larger nuclear charge binds the electron more tightly (the Coulomb attraction scales with Z, and the orbit radius shrinks as 1/Z); the 1/n2 is the usual orbit-quantisation result. He+ has one electron and Z=2, so the formula applies to it.
Step 2 — Hydrogen, second orbit
Z=1, n=2:
E2=−13.6×2212=−413.6=−3.4 eV
Step 3 — He+, third orbit
Z=2, n=3:
E3(He+)=−13.6×3222=−13.6×94=−6.04 eV
Step 4 — Express it in terms of E2 (take the ratio)
E2(H)E3(He+)=−13.6×41−13.6×94=94×14=916
∴E3(He+)=916E2
Numerically: 916×(−3.4)=−6.04 eV. ✓ Consistent. …
- KCET 2018Set A-11 markMCQQ.The period of revolution of an electron in the ground state of hydrogen atom is T. The period of revolution of the electron in the first excited state is (A) 2T (B) 4T (C) 6T (D) 8T
›Reveal solutionSolution
Period Tn=vn2πrn with rn∝n2 and vn∝1/n gives Tn∝n3; for n=2 that is 8× the ground-state period.
Step 1 — Bohr's radius and speed.
For hydrogen,
rn=πme2n2h2ε0∝n2,vn=2ε0hne2∝n1
(The n2 growth of the orbit and the 1/n slowing of the electron both come from the quantisation condition mvr=2πnh combined with the Coulomb force providing the centripetal force.)
Step 2 — Period of revolution.
Tn=speedcircumference=vn2πrn∝1/nn2=n3
So Tn∝n3 — the electron in a higher orbit takes dramatically longer to go round, because the orbit is much bigger and it moves more slowly.
Step 3 — Apply to the given states. …
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