Q.The terminology of different parts of the electromagnetic spectrum is given in the text. Use the formula E=hν (for energy of a quantum of radiation: photon) and obtain the photon energy in units of eV for different parts of the electromagnetic spectrum. In what way are the different scales of photon energies that you obtain related to the sources of electromagnetic radiation?
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Photon Energy Calculation
The Core Idea
Light is not a smooth, continuous flow of energy — it comes in tiny indivisible packets called photons. Each photon carries a fixed amount of energy that depends only on the light's frequency (its colour), not on how bright the beam is. A brighter beam simply contains more photons; each individual photon still carries the same energy.
The Master Formula
E=hf=λhc
where
- E = energy of one photon (joule, J),
- h=6.63×10−34 J s is Planck's constant,
- f = frequency of the light (hertz, Hz),
- c=3×108 m/s is the speed of light, and
- λ = wavelength (metre, m).
The two forms are connected by the wave relation c=fλ. Use E=hf when you are given the frequency and E=hc/λ when you are given the wavelength.
Because E=hc/λ, energy is inversely proportional to wavelength: short-wavelength radiation (X-rays, UV) has high-energy photons; long-wavelength radiation (radio, microwave) has low-energy photons.
Working in Electron-Volts
Photon energies are tiny in joules, so we often use the electron-volt:
1 eV=1.6×10−19 J
A handy shortcut for visible/UV light expresses the energy directly from the wavelength in nanometres:
E(eV)≈λ (nm)1240
(The number 1240 is just hc expressed in eV·nm.)
Worked Example 1 — from frequency
Find the energy of a photon of frequency f=5.0×1014 Hz (green light).
E=hf=(6.63×10−34)(5.5×1014)=3.6×10−19 J
Converting to eV:
E=1.6×10−193.3×10−19≈2.1 eV
Worked Example 2 — from wavelength
Find the energy of a photon of wavelength λ=620 nm (red light).
E=λhc=620×10−9(6.63×10−34)(3×108)=3.2×10−19 J≈2.0 eV
Or with the shortcut: E≈1240/620=2.0 eV — same answer, much faster.
Total Energy of a Beam
A single photon's energy is tiny, but a real beam contains enormous numbers of them. If a source emits N photons per second (or a pulse contains N photons), the total energy is simply
Etotal=N×hf
So the number of photons carrying a given power P is …
Why this formula?
Photon Energy Calculation
Light of frequency ν (or wavelength λ) is carried in indivisible packets called photons. Calculating a photon's energy is one of the most common numerical tasks in modern physics, and it rests on a single relation.
A photon's energy depends only on its frequency (colour), not on how bright the beam is: E=hν=λhc.
The Working Formula
E=hν=λhc
where h=6.63×10−34 J⋅s (Planck's constant), c=3×108 m/s, ν is frequency (Hz) and λ is wavelength (m). The two forms are linked by the wave relation c=νλ, so ν=c/λ.
Two Handy Shortcuts
- Product hc: hc=6.63×10−34×3×108≈1.99×10−25 J⋅m.
- Energy in electron-volts (divide joules by 1.6×10−19):
E(eV)=λ(nm)1240 …
E=hν=hc/λ, and hc≈1240 eV*nm, so E(eV)=1240/λ(nm).
Using one representative wavelength per band: radio (~1 m) ≈1.24×10−6 eV; microwave (~1 cm) ≈1.24×10−4 eV; infrared (~10 μm) ≈0.124 eV; visible (400-700 nm) ≈1.8-3.1 eV; ultraviolet (~100 nm) ≈12.4 eV; X-ray (~0.1 nm) ≈1.24×104 eV; gamma ray (~1 pm) ≈1.24×106 eV. …
Photon energy is E=hν=hc/λ. Using representative wavelengths for each band (radio ~1 m, microwave ~1 cm, infrared ~10 μm, visible 400-700 nm, UV ~100 nm, X-ray ~0.1 nm, gamma ray ~1 pm), photon energies range from about 10−6 eV (radio) to over 106 eV (gamma rays) -- this huge range directly reflects the different physical processes (from oscillating currents to nuclear transitions) that generate each band.
The formula
E=hν=λhc
with h=6.63×10−34 J*s, c=3×108 m/s. Converting to electronvolts (1 eV =1.6×10−19 J) gives the handy shortcut
E(eV)=λ(nm)1240
Photon energy across the spectrum (one representative wavelength per band)
| Region | Representative λ | E (eV) | Typical source |
|---|---|---|---|
| Radio | 1 m | 1.24×10−6 | Oscillating currents in antennas |
| Microwave | 1 cm | 1.24×10−4 | Molecular rotation, oscillators |
| Infrared | 10 μm | 0.124 | Molecular vibration, thermal emission |
| Visible | 400-700 nm | 1.8-3.1 | Electronic transitions in atoms/molecules |
| Ultraviolet | 100 nm | 12.4 | Atomic ionisation, hot sources |
| X-ray | 0.1 nm | 1.24×104 | Inner-shell transitions, bremsstrahlung |
| Gamma ray | 1 pm | 1.24×106 | Nuclear transitions, particle annihilation |
Sample calculations: radio E=1240/(1×109)=1.24×10−6 eV; gamma ray E=1240/(0.001)=1.24×106 eV.
How photon energy relates to the source
Each energy scale matches the energy scale of the physical process that produces it:
- Radio/microwave (μeV-meV): energies of oscillating currents in circuits/antennas or molecular rotations -- very small, so these come from low-energy motions.
- Infrared (~0.1 eV): matches the spacing of molecular vibrational energy levels and thermal (blackbody) emission from warm objects. …
Method: Direct Photon Energy Calculation Using E=hν
Concept: The energy of a single photon is directly proportional to its frequency. The constant of proportionality is Planck's constant h.
Steps
- Recall the formula The energy of one photon is:
E=hν
where:
- E = energy (in joules, J)
- h=6.626×10−34 J⋅s (Planck's constant)
- ν = frequency of radiation (in Hz, or s−1)
- Convert energy from joules to electronvolts (eV) Since 1 eV = 1.602×10−19 J, the energy in eV is:
EeV=1.602×10−19hν
- Use the relation between frequency and wavelength If wavelength λ (in metres) is given instead of frequency:
ν=λc
where c=3.00×108 m/s (speed of light).
Then:
E=λhc
and in eV:
EeV=λ×1.602×10−19hc
- Plug in values for each spectral region For example, for visible light (say λ≈500 nm = 5.00×10−7 m):
EeV=(5.00×10−7)(1.602×10−19)(6.626×10−34)(3.00×108)≈2.48 eV
- Interpret the scale
- Radio waves → very low energy (micro-eV to meV)
- Microwaves → low energy (meV range)
- Infrared → moderate energy (meV to eV)
- Visible light → ~1.5–3 eV
- Ultraviolet → higher energy (3–100 eV) …
Here are the common mistakes students make when solving photon energy problems (like the one from the NCERT Electromagnetic Spectrum chapter), along with how to avoid each.
1. Forgetting to Convert Frequency to Hz (or Wavelength to Meters)
The Mistake:
Students plug in frequency given in MHz, GHz, or wavelength in nm, Å, or cm directly into E=hν or E=λhc without converting to Hz (s⁻¹) or meters (m).
Why it’s wrong:
Planck’s constant h=6.63×10−34J s and c=3×108m/s are in SI units. Using non-SI units gives a completely wrong numerical value.
How to avoid:
- Always write the given value with its unit.
- Convert:
- 1MHz=106Hz
- 1nm=10−9m
- 1A˚=10−10m
- Check: If your answer is off by a factor of 109 or 1015, you likely missed a conversion.
2. Using the Wrong Formula for Energy
The Mistake:
Using E=hν when wavelength is given, or using E=λhc when frequency is given — but then forgetting to use c correctly or mixing up ν and λ.
Why it’s wrong:
The two formulas are equivalent only if you use the correct relation c=νλ. Mixing them without substitution gives nonsense.
How to avoid:
- If frequency is given → use E=hν
- If wavelength is given → use E=λhc
- Never plug a wavelength into E=hν — you’ll get energy in Joules that is off by a factor of 108.
3. Incorrect Conversion from Joules to eV
The Mistake:
Using 1eV=1.6×10−19J but dividing instead of multiplying (or vice versa).
Why it’s wrong:
1 eV is a smaller unit than 1 J. So a number in Joules should be divided by 1.6×10−19 to get eV. Doing the opposite gives a ridiculously tiny number.
How to avoid:
- Remember: 1 eV = 1.6×10−19 J
- To convert J → eV: divide by 1.6×10−19
- Quick sanity check: Visible light photons are ~2–3 eV. If your answer is 10−19 eV or 1020 eV, you’ve swapped.
4. Forgetting to Use h and c with Correct Units
The Mistake:
Using h=6.63×10−34J s but then using c=3×108m/s and wavelength in cm — or using h in eV·s without converting.
Why it’s wrong:
h in J·s and c in m/s require length in meters. If you use cm, the energy will be off by 102.
How to avoid:
- Stick to SI units for h, c, λ, ν.
- If you want eV directly, use the convenient constant:
hc=1240eV⋅nm
Then E(eV)=λ(nm)1240 — this avoids unit errors entirely.
5. Misinterpreting the “Scale” of Photon Energies
The Mistake:
After calculating energies, students fail to connect the order of magnitude to the source (e.g., radio waves have tiny eV, gamma rays have huge MeV). They just list numbers without insight.
Why it’s wrong:
The question explicitly asks: “In what way are the different scales of photon energies related to the sources?” — this is a conceptual link.
How to avoid:
- Compare orders of magnitude:
- Radio: ∼10−6 eV (electronic circuits)
- Microwave: ∼10−3 eV (molecular rotation)
- Visible: ∼1–3 eV (electronic transitions in atoms)
- X-ray: ∼103–105 eV (inner shell transitions) …
- AP EAPCET 2025Set ap-2025-05-20-FN1 markMCQQ.To dissociate a molecule into its component atoms, the energy required is 13.2 eV. The frequency of the electromagnetic radiation corresponding to this energy lies in (A) infrared region (B) visible region (C) microwave region (D) ultraviolet region
›Reveal solutionSolution
Converting the 13.2 eV dissociation energy to a photon frequency/wavelength via E=hf=hc/λ gives a wavelength around 94 nm, which lies in the ultraviolet region.
Concept and Intuition
Each photon of electromagnetic radiation carries energy E=hf=λhc. To identify which part of the spectrum corresponds to a given bond/dissociation energy, convert that energy into a wavelength and compare it against the known spectral ranges (radio, microwave, infrared, ~400–700 nm visible, ultraviolet below ~400 nm, X-rays, etc.).
Step-by-Step Solution
- Convert energy to joules: E=13.2 eV×1.6×10−19 J/eV=2.112×10−18 J.
- Find frequency: f=hE=6.63×10−342.112×10−18≈3.19×1015 Hz.
- Find wavelength: λ=fc=3.19×10153×108≈9.4×10−8 m =94 nm. …
- AP EAPCET 2025Set eng-2025-05-24-FN1 markMCQQ.A laser produces a beam of light of frequency 5×1014 Hz with an output power of 33 mW. The average number of photons emitted by the laser per second is (Planck's constant =6.6×10−34 J s) (A) 40×1016 (B) 10×1016 (C) 30×1016 (D) 20×1016
›Reveal solutionSolution
Tests converting beam power into a photon flux using E=hf; the answer is 10×1016 photons/s.
Concept and Intuition
A beam's power is the total energy it delivers per second. If each photon of frequency f carries a fixed quantum of energy E=hf, then the number of photons crossing per second is simply the power divided by the energy of one photon: N=P/E.
Step-by-Step Solution
- Energy of one photon: E=hf=(6.6×10−34)(5×1014)=3.3×10−19 J.
- Convert power to SI: P=33 mW=3.3×10−2 W. …
- AP EAPCET 2025Set eng-2025-05-26-FN1 markMCQQ.The minimum wavelength of X-rays produced by 20 kV electrons is nearly (A) 0.62 Å (B) 1.8 Å (C) 3.2 Å (D) 6.5 Å
›Reveal solutionSolution
This tests the Duane-Hunt law for the short-wavelength (minimum wavelength) limit of the continuous X-ray spectrum; for 20 kV accelerating voltage, λmin=0.62 Å.
Concept and Intuition
When high-speed electrons strike a target, some lose their entire kinetic energy in a single collision, emitting one photon carrying all of it — this photon has the maximum possible energy and hence the minimum possible wavelength in the continuous (bremsstrahlung) X-ray spectrum. Since the electron's kinetic energy comes from being accelerated through potential difference V, energy conservation gives eV=λminhc.
Step-by-Step Solution
- From eV=λminhc: λmin=eVhc.
- Using the standard combination ehc≈12400eVA˚ (i.e. hc/e expressed conveniently in eV·Å), λmin=V(in volts)12400A˚. …
- AP EAPCET 2024Set eng-2024-05-21-AN1 markMCQQ.A transmitter of power 10 kW emits radio waves of wavelength 500 m. The number of photons emitted per second by the transmitter is of the order of (A) 1037 (B) 1031 (C) 1025 (D) 1043
›Reveal solutionSolution
Divide the transmitted power by the energy of a single photon at the given wavelength. Answer: order 1031.
Concept and Intuition
A radio transmitter emits energy as a stream of photons, each carrying energy E=hc/λ. The number of photons emitted per second is simply the total power divided by the energy per photon, since power is energy delivered per unit time.
Step-by-Step Solution
- P=10 kW=104 W, λ=500 m.
- Ephoton=λhc=5006.63×10−34×3×108=3.98×10−28 J.
- n=EphotonP=3.98×10−28104≈2.5×1031 photons/second. …
- AP EAPCET 2024Set eng-2024-05-21-FN1 markMCQQ.A blue lamp emits light of mean wavelength 4500Å. The lamp is rated at 150 W and 8% efficiency. Then the number of photons are emitted by the lamp per second (A) 27.17×1018 (B) 17.17×1018 (C) 27.17×1015 (D) 54×1016
›Reveal solutionSolution
Only 8% of the rated power actually becomes light; dividing this useful power by the energy of one photon (from E=hc/λ) gives the photon emission rate.
Concept and Intuition
The lamp's rated 150 W is the total electrical power drawn, but only a fraction (the stated efficiency) is converted into visible light — the rest is lost as heat. To find how many photons are emitted per second, we need the light power, then divide by the energy carried by a single photon of the given wavelength.
Step-by-Step Solution
- Useful (optical) power: Plight=0.08×150=12 W.
- Photon energy: E=λhc=4500×10−106.63×10−34×3×108.
- Numerator: 6.63×3=19.89⇒19.89×10−26. Denominator: 4.5×10−7.
- E=4.5×10−719.89×10−26=4.42×10−19 J. …
- AP EAPCET 2022Set eng-2022-07-07-FN1 markMCQQ.The average number of photons emitted per second by a laser of power 6.6×10−3 W producing a light of wavelength 600 nm is (Planck's constant, h=6.6×10−34 J s) (A) 2×1016 (B) 3×1016 (C) 4×1016 (D) 6×1016
›Reveal solutionSolution
This is a direct photon-counting problem: divide laser power by the energy of a single photon to get the photon emission rate, 2×1016 per second.
Concept and Intuition
A laser's power output is just the total energy emitted per second, which equals (number of photons per second) × (energy per photon). Since each photon of wavelength λ carries energy E=hc/λ (or hν), the photon rate is simply power divided by this per-photon energy.
Step-by-Step Solution
- Energy per photon: E=λhc=6×10−7(6.6×10−34)(3×108).
- Numerator: 6.6×10−34×3×108=19.8×10−26=1.98×10−25 J·m.
- E=6×10−71.98×10−25=0.33×10−18=3.3×10−19 J. …
- AP EAPCET 2021Set ap-2021-09-03-AN1 markMCQQ.A photon of frequency 'ν' has a momentum associated with it. If 'c' is the velocity of light then momentum is ______ (A) c2hν (B) hνc (C) cν (D) chν
›Reveal solutionSolution
Combining the photon energy E=hν with the relativistic energy-momentum relation for a massless particle, p=E/c, gives p=hν/c.
Concept and Intuition
A photon has zero rest mass, so its total energy and momentum are related simply by E=pc (the massless limit of E2=(pc)2+(mc2)2). Since a photon of frequency ν carries energy E=hν (Planck's relation), substituting gives its momentum directly.
Step-by-Step Solution
- Photon energy: E=hν.
- Massless-particle relation: E=pc, so p=cE.
- Substitute: p=chν. …
- AP EAPCET 2021Set ap-2021-09-03-FN1 markMCQQ.A radio transmitter operates at a frequency 880 kHz and a power of 10 kW. What is the number of photons emitted per second? (A) 1.50×1025 (B) 1.60×1030 (C) 1.72×1031 (D) 2.80×1030
›Reveal solutionSolution
This tests the conversion of a macroscopic radio-wave power output into a photon count, using Ephoton=hf and N=P/Ephoton. The answer is 1.72×1031 photons per second.
Concept and Intuition
Even though radio waves behave classically at the level of everyday antennas, the electromagnetic energy they carry is still quantized into photons of energy E=hf. Because radio-frequency photons are extremely low-energy (since f is small), an ordinary transmitter emits an enormous number of them per second to deliver even modest total power — this is the conceptual bridge between the quantum picture (individual photons) and the classical picture (continuous power output).
Step-by-Step Solution
- Frequency: f=880 kHz=8.8×105 Hz.
- Energy per photon: E=hf=(6.626×10−34)(8.8×105)=5.831×10−28 J.
- Total power: P=10 kW=1×104 W=1×104 J/s. …
- AP EAPCET 2021Set eng-2021-08-20-AN1 markMCQQ.The shortest wavelength of X-rays emitted from an X-ray tube depends upon _______ (A) Nature of the gas in the tube (B) Voltage applied to tube (C) Current in the tube (D) Nature of target of the tube
›Reveal solutionSolution
The cut-off wavelength of the continuous (bremsstrahlung) X-ray spectrum is fixed purely by the accelerating voltage across the tube, since it corresponds to an electron converting its entire kinetic energy into a single photon.
Concept and Intuition
In an X-ray tube, electrons are accelerated through a potential difference V and slammed into a target. Most electrons undergo multiple deceleration events, radiating a continuous spectrum of photon energies (Bremsstrahlung), but the maximum possible photon energy — and hence the minimum possible wavelength — occurs when an electron loses all of its kinetic energy eV in a single collision, emitting one photon of energy eV=hνmax=λminhc. This depends only on how much energy the electron was given by the accelerating voltage, not on which target it hits or how much current flows.
Step-by-Step Solution
- Kinetic energy gained by an electron accelerated through voltage V: KE=eV.
- Maximum photon energy possible from a single electron = its entire KE: hνmax=eV.
- λmin=eVhc — depends only on V (and universal constants h,c,e). …
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