Q.The wavelength of a photon needed to remove a proton from a nucleus which is bound to the nucleus with 1 MeV energy is nearly
Concept understanding — Photon Energy
Photon Energy: The Energy Carried by Light
Light does not carry its energy in a continuous stream. It comes in discrete packets — like individual drops instead of a steady hose. Each packet is called a photon: the smallest possible unit of light of a given frequency. You cannot have half a photon; it is all or nothing.
The Intuition: Colour Determines Energy
Red light and blue light are both light, but they behave differently — blue light causes sunburn and drives chemical reactions more readily than red. The reason is that the colour (frequency) of light directly fixes how much energy each photon carries, and blue photons carry more energy than red photons.
The Planck–Einstein Relation
The energy E of a single photon is directly proportional to its frequency f, and inversely proportional to its wavelength λ:
E=hf=λhc
Where:
- E = energy of one photon (joules, J)
- f = frequency (hertz, Hz)
- λ = wavelength (metres, m)
- c = speed of light in vacuum (3.00×108 m/s)
- h = Planck's constant (6.626×10−34 J·s)
Planck's constant h is extremely tiny, so an individual photon carries a very small amount of energy — which is why we never feel single photons striking our skin.
What This Tells You
- Higher frequency = higher energy. Gamma rays have extremely energetic photons; radio waves have very low-energy photons.
- Shorter wavelength = higher energy. Ultraviolet photons are more energetic than visible-light photons; infrared photons are less.
- Energy is quantised. Light energy comes in fixed packets — you can have 1, 2, or 1000 photons, but never 0.5. This was Max Planck's revolutionary idea of 1900.
This is why UV light causes sunburn (UV photons carry enough energy to damage DNA, while visible photons do not), why X-ray photons are energetic enough to pass through soft tissue but get absorbed by bone, and why a photon needs enough energy to actually break a bond or drive a photochemical/biological reaction, rather than merely wavelength-dependent intensity.
A Concrete Example
Question: Which has more energy — a photon of red light (λ=700 nm) or a photon of blue light (λ=450 nm)?
Since E=λhc, energy is inversely proportional to wavelength, so the shorter-wavelength blue photon carries more energy:
- Red: Ered=700×10−9(6.626×10−34)(3.00×108)≈2.84×10−19 J
- Blue: Eblue=450×10−9(6.626×10−34)(3.00×108)≈4.42×10−19 J
The blue photon carries about 1.5 times the energy of the red photon.
A common mistake is to think brighter light means more energetic photons. Brightness is the number of photons per second, not the energy per photon. A bright red light has many low-energy photons; a dim blue light has fewer but higher-energy ones.
The Big Picture
Photon energy is the bridge between the wave nature of light (frequency, wavelength) and its particle nature (energy packets) — one of the foundational ideas of quantum mechanics: at the smallest scales, energy is not continuous but comes in discrete, indivisible units.
Photon energy, given by the Planck-Einstein relation E = hf, is one of the most fundamental formulas in the NCERT Class 12 Physics Dual Nature of Radiation and Matter chapter, and "photon energy formula and calculation" is a heavily searched query among students preparing for CBSE boards, JEE Main, and NEET. Because this idea links directly to the photoelectric effect and atomic spectra, it also anchors several "modern physics important questions" compiled for competitive-exam revision.
Why this formula?
Why Photon Energy is E=hf — The Reasoning Behind the Formula
The formula E=hf is not something you memorise and plug numbers into. It comes from a deep shift in how physicists understood light.
The problem that forced the formula
By the late 1800s, classical physics said light was a wave — continuous, carrying energy in proportion to its intensity (brightness). But blackbody radiation and the photoelectric effect showed something bizarre: when you shine light on a metal, electrons are ejected only if the light's frequency is above a certain threshold, no matter how bright the light is. Below that frequency, even the brightest lamp won't kick out a single electron. Classically this made no sense — a wave's energy depends on amplitude, not frequency.
Einstein's radical idea (1905)
Einstein proposed that light comes in discrete packets — photons — each carrying a fixed energy that depends only on its frequency, with Planck's constant h as the proportionality:
A single photon's energy is E=hf, where f is the frequency of the light.
This directly explains the photoelectric effect: an electron needs a minimum energy (the work function ϕ) to escape. If a photon's energy hf<ϕ, no electron is ejected — regardless of how many photons you send, because each photon interacts with one electron individually.
E=hf is not derived from deeper principles — it is a postulate justified by the experiments it explains, and it unified optics with quantum mechanics.
The equivalent forms
Since c=fλ for light in vacuum, the same idea in terms of wavelength is:
E=λhc
Use this when you're given λ instead of f. A photon also carries momentum (despite having no mass):
p=cE=λh
This follows from special relativity: E2=(pc)2+(mc2)2, and for a photon m=0, so E=pc, hence p=h/λ.
- h=6.626×10−34 J⋅s (Planck's constant)
- c=3.0×108 m/s (speed of light)
- For atomic-scale problems use electronvolts: 1 eV=1.602×10−19 J
A common exam trap
E=hf means higher frequency = more energy per photon — true. But a brighter light does not mean higher photon energy. Intensity is the number of photons per second per area; each photon still carries hf.
Do not confuse intensity (number of photons) with frequency (energy per photon). They are independent.
Final answer: E=hf
The key idea is that the photon must supply at least the binding energy of the proton — here 1 MeV.
Reasoning:
- The minimum photon energy required is E=1 MeV=106 eV.
- Use the photon energy-wavelength relation:
E=λhc⇒λ=Ehc.
- A useful shortcut: hc≈1240 eV⋅nm. So
λ=106 eV1240 eV⋅nm=1.24×10−3 nm.
This matches option (B).
The wavelength is nearly 1.2×10−3 nm, which corresponds to option (B).
The photon must supply exactly the binding energy of the proton (1 MeV). Using E=hc/λ, the wavelength comes out to about 1.24×10−3 nm, which matches option (B).
The core idea here is that removing a proton from a nucleus requires overcoming the nuclear binding force. That binding energy is given as 1 MeV — the minimum energy a photon must carry to eject the proton. Since a photon’s energy is inversely proportional to its wavelength, we can directly compute the wavelength.
A common pitfall is forgetting to convert units properly or mixing up the energy-wavelength relation for photons. Let’s walk through it cleanly.
- Recall the photon energy-wavelength relation For any photon, E=λhc, where h is Planck’s constant and c is the speed of light. The product hc is a very useful constant:
hc=1240 eV⋅nm
(This is exact enough for all exam purposes — it comes from h=4.135667×10−15 eV⋅s and c=2.998×108 m/s, giving hc≈1240 eV⋅nm.)
- Set the photon energy equal to the binding energy The photon must have E=1 MeV=106 eV. So:
λhc=106 eV
- Solve for λ
λ=106 eVhc=106 eV1240 eV⋅nm=1.24×10−3 nm
- Match with the options The value 1.24×10−3 nm is extremely close to 1.2×10−3 nm — the slight difference is due to rounding hc to 1240 instead of 1239.84. In multiple-choice exams, this is the intended match.
A very common mistake is to use E=hf and then forget that c=fλ, or to mix up units (e.g., using hc=1240 eV⋅nm but then treating the energy in MeV without converting to eV). Always convert MeV to eV first: 1 MeV=106 eV.
Memorising hc=1240 eV⋅nm saves enormous time. For any photon energy in eV, the wavelength in nm is simply 1240/E. For MeV energies, just shift the decimal: 1240/106=1.24×10−3.
The correct option is (B) 1.2×10−3 nm.
Method: Converting a Threshold/Binding Energy into a Photon Wavelength
Use this whenever a question gives you a minimum energy a photon must supply (a binding energy, an ionisation energy, a work function) and asks for the corresponding photon wavelength.
Steps
Step 1: Identify the minimum photon energy required
The photon must carry at least the stated binding/threshold energy — treat that value as E directly. Convert it to electron-volts if it isn't already (e.g. 1 MeV=106 eV); electron-volts pair naturally with the shortcut in Step 3.
Step 2: Start from the photon energy–wavelength relation
E=λhc⇒λ=Ehc
Step 3: Use the hc≈1240 eV⋅nm shortcut
For any photon energy expressed in eV, the wavelength in nanometres is simply
λ(nm)=E(eV)1240
This avoids carrying h and c separately through the algebra and is accurate enough for exam purposes.
Step 4: Apply to this problem and sanity-check the order of magnitude
Divide 1240 by the energy in eV, watching the powers of ten carefully — a binding energy in the MeV range (nuclear scale) should give a wavelength many orders of magnitude shorter than a typical atomic-scale binding energy (eV range, giving hundreds of nm). If your answer doesn't fall in the expected range for the physical scale of the problem, re-check the unit conversion in Step 1 rather than the formula.
- GSEB Higher Secondary Certificate (HSC) Examination 2026Set ANNUAL1 markMCQQ.Monochromatic light of frequency 6.0 x 10^14 Hz is produced by a laser. The power emitted is 2.0 x 10^-3 W. How many photons per second on an average, are emitted by the source?(a) 0.5 x 10^15(b) 0.5 x 10^17(c) 5 x 10^17(d) 5 x 10^15
›Reveal solutionSolution
The number of photons emitted per second is the total power divided by the energy carried by a single photon, E = h nu.
Given: nu = 6.0 x 10^14 Hz, P = 2.0 x 10^-3 W, h = 6.63 x 10^-34 J s.
Energy per photon: E = h nu = 6.63 x 10^-34 x 6.0 x 10^14 = 3.98 x 10^-19 J
Photons per second: n = P/E = (2.0 x 10^-3)/(3.98 x 10^-19) = 5.0 x 10^15 photons/s.
✓Final answer(d) 5 x 10^15.
- GSEB Higher Secondary Certificate (HSC) Examination 2025Set ANNUAL1 markMCQQ.Monochromatic light of frequency 6 x 10^14 Hz is produced by a laser. The power emitted is 2 x 10^-3 W. How many photons per second on an average are emitted by the source? [h = 6.63 x 10^-34 Js](a) 3.98 x 10^19(b) 1.99 x 10^15(c) 3 x 10^15(d) 5 x 10^15
›Reveal solutionSolution
Each photon carries energy E = hν; dividing the total power by this per-photon energy gives the photon emission rate.
E = hν = (6.63 × 10⁻³⁴)(6 × 10¹⁴) = 3.978 × 10⁻¹⁹ J.
n = P/E = (2 × 10⁻³)/(3.978 × 10⁻¹⁹) ≈ 5.03 × 10¹⁵ ≈ 5 × 10¹⁵ photons/s.
✓Final answer(d) 5 × 10¹⁵ photons/s.
- GSEB Higher Secondary Certificate (HSC) Examination 2025Set ANNUAL1 markMCQQ.A difference of 2.3 eV separates two energy levels in an atom. What is the frequency of radiation emitted when the atom makes a transition from the upper level to the lower level? [h = 6.63 x 10^-34 Js](a) 1.2 x 10^14 Hz(b) 5.6 x 10^14 Hz(c) 3.8 x 10^14 Hz(d) 1.6 x 10^6 Hz
›Reveal solutionSolution
The frequency of emitted radiation during an atomic transition follows Bohr's frequency condition: hν = ΔE.
ΔE = 2.3 eV = 2.3 × 1.6 × 10⁻¹⁹ = 3.68 × 10⁻¹⁹ J.
ν = ΔE/h = 3.68 × 10⁻¹⁹ / 6.63 × 10⁻³⁴ ≈ 5.55 × 10¹⁴ Hz ≈ 5.6 × 10¹⁴ Hz.
✓Final answer(b) 5.6 × 10¹⁴ Hz.
- GSEB Higher Secondary Certificate (HSC) Examination 2024Set ANNUAL1 markMCQQ.The momentum of a photon of light of frequency f is ___.(a) hc/f(b) h/cf(c) hf/c(d) hcf
›Reveal solutionSolution
A photon of energy E = hf carries momentum p = E/c.
p = E/c = hf/c.
✓Final answer(c) hf/c.
- GSEB Higher Secondary Certificate (HSC) Examination 2023Set ANNUAL1 markMCQQ.Monochromatic light of frequency 6 x 10^14 Hz is produced by laser. The power emitted is 2 x 10^-3 W. The energy of the photon in this light beam is ___ eV. [h = 6.63 x 10^-34 Js, 1 eV = 1.6 x 10^-19 J](a) 3.0(b) 3.5(c) 4.0(d) 2.5
›Reveal solutionSolution
Photon energy E = h*nu = 3.98 x 10^-19 J; dividing by 1.6 x 10^-19 J/eV gives about 2.5 eV.
Energy of a photon: E = h*nu = (6.63 x 10^-34)(6 x 10^14) = 3.978 x 10^-19 J.
Convert to eV: E = (3.978 x 10^-19)/(1.6 x 10^-19) = 2.49 eV approximately 2.5 eV.
(The beam power 2 x 10^-3 W is extra data - it fixes the number of photons per second, not the energy of one photon.)
✓Final answer(d) 2.5 eV.
- GUJCET 2022Set 171 markMCQQ.A difference of 5.4 eV separates two energy levels in an atom. What is the frequency of radiation emitted when the atom make a transition from the upper level to the lower level? [1 eV = 1.6×10−19 J, h=6.625×10−34 J.s.] (A) 1.304×1015 Hz (B) 5.6×1015 Hz (C) 5.6×1014 Hz (D) 1.304×1014 Hz
›Reveal solutionSolution
Photon frequency f=ΔE/h.
Steps.
- ΔE=5.4 eV=5.4×1.6×10−19=8.64×10−19 J.
- f=6.625×10−348.64×10−19=1.304×1015 Hz.
✓Final answer(A) 1.304×1015 Hz
ANSWER: (A)
- GUJCET 2022Set 171 markMCQQ.What is the shortest wavelength present in the Paschen series of spectral lines? (A) 320 nm (B) 720 nm (C) 840 nm (D) 820 nm
›Reveal solutionSolution
Shortest wavelength = series limit, 1/λ=RH/9.
Concept. The shortest wavelength of a hydrogen series comes from the transition n=∞→nf. For Paschen, nf=3.
Steps.
- λ1=RH(321−0)=91.097×107=1.219×106 m−1.
- λ=8.2×10−7 m=820 nm.
✓Final answer(D) 820 nm
ANSWER: (D)
- GSEB Higher Secondary Certificate (HSC) Examination 2020Set ANNUAL1 markMCQQ.Monochromatic light of frequency 6x10^14 Hz is produced by laser. Each photon has an energy = ____ J.(a) 6x10^14(b) 4x10^-19(c) 4x10^-20(d) 6x10^-14
›Reveal solutionSolution
Photon energy E = hf; substituting f = 6×10¹⁴ Hz gives about 4×10⁻¹⁹ J.
E=hf=(6.63×10−34)×(6×1014)=3.978×10−19 J≈4×10−19 J.
✓Final answer(b) 4×10^-19 J.
- GSEB Higher Secondary Certificate (HSC) Examination 2019Set ANNUAL1 markMCQQ.Which of the following physical quantity has the dimension of planck constant (h)?(a) Angular momentum(b) Force(c) Energy(d) Power
›Reveal solutionSolution
Planck's constant has dimensions of Energy × Time =[ML2T−2][T]=[ML2T−1], which is also the dimension of angular momentum.
Angular momentum =mvr has dimension [M][LT−1][L]=[ML2T−1], matching h. Force, energy, and power all have different dimensions ([MLT−2], [ML2T−2], [ML2T−3] respectively).
✓Final answer(a) Angular momentum.
- GSEB Higher Secondary Certificate (HSC) Examination 2018Set ANNUAL1 markMCQQ.Energy of photon is E = hf and its momentum is P = h/lambda, where lambda is the wavelength of photon. With this assumption speed of light wave is ___.(a) P/E(b) E/P(c) EP(d) (E/P)^2
›Reveal solutionSolution
Speed of light = f x lambda; using f = E/h and lambda = h/P gives speed = E/P.
The speed of a light wave is v = f lambda.
From E = h f: f = E/h.
From P = h/lambda: lambda = h/P.
Therefore v = f lambda = (E/h)(h/P) = E/P.
(This is the familiar relation E = P c for a photon, since v = c.)
✓Final answer(b) E/P.
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