JEE Main Atomic Structure 2027 — Bohr Model, Quantum Numbers, Orbitals, de Broglie and 35 Practice MCQs - JEE Gurukul

JEE Main Atomic Structure 2027 — Bohr Model, Quantum Numbers, Orbitals, de Broglie and 35 Practice MCQs

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Last Updated: May 2026

JEE 2027 — Atomic Structure overview

For JEE Main 2027 Atomic Structure, expect 2-3 questions covering Bohr’s model numerics, quantum numbers, orbital configuration, photoelectric effect formulas and de Broglie wavelength. The chapter sits at the foundation of physical chemistry and bridges into modern physics in JEE Physics — making formula-recall here doubly valuable.

Bohr Model — Master Formulas

Quantity Formula Notes
Radius of nth orbit (H) rn = 0.529 × n² /Z Å 0.529 Å = Bohr radius
Velocity in nth orbit vn = 2.18 × 10⁶ × Z/n m/s
Energy of nth orbit En = –13.6 × Z²/n² eV For H: −13.6, −3.4, −1.51, −0.85 eV
Energy in joules En = –2.18 × 10⁻¹⁸ × Z²/n² J
Frequency of transition ν = (Ei – Ef)/h h = 6.626 × 10⁻³⁴ J·s
Rydberg formula 1/λ = RH·Z²(1/n₁² – 1/n₂²) RH = 1.097 × 10⁷ m⁻¹

Hydrogen Spectrum Series

Series Final n (n₁) Region First line λ
Lyman 1 Ultraviolet 121.6 nm
Balmer 2 Visible 656.3 nm (Hα, red)
Paschen 3 Infrared 1875 nm
Brackett 4 Far infrared 4050 nm
Pfund 5 Far infrared 7460 nm

Photoelectric Effect

  • Einstein’s equation: hν = φ + KEmax
  • φ = work function = hν₀ (threshold frequency)
  • Stopping potential: eVs = KEmax = h(ν − ν₀)
  • KEmax depends on frequency, not intensity
  • Number of electrons emitted depends on intensity, not frequency

de Broglie Wavelength

  • λ = h/p = h/(mv)
  • For an electron accelerated through V volts: λ = 12.27/√V Å (where V is in volts)
  • Photon: p = h/λ; E = pc

Heisenberg Uncertainty Principle

Δx · Δp ≥ h/(4π) — applies to conjugate variables (position-momentum, energy-time). Cannot simultaneously know exact position and momentum.

Quantum Numbers

Quantum No. Symbol Range Determines
Principal n 1, 2, 3,… Energy, size of orbit
Azimuthal l 0 to (n−1) Subshell shape (s, p, d, f)
Magnetic ml –l to +l Orbital orientation
Spin ms +½, –½ Electron spin

Aufbau: Fill orbitals in order of increasing (n+l), with lower n first when (n+l) is equal. Pauli’s exclusion: No two electrons in an atom can have all four quantum numbers identical. Hund’s rule: Maximum unpaired electrons in degenerate orbitals before pairing.

Number of Orbitals and Electrons

  • Total orbitals in nth shell: n²
  • Total electrons in nth shell: 2n²
  • s subshell: 1 orbital, 2 electrons
  • p subshell: 3 orbitals, 6 electrons
  • d subshell: 5 orbitals, 10 electrons
  • f subshell: 7 orbitals, 14 electrons

Number of Radial and Angular Nodes

  • Radial nodes = n − l − 1
  • Angular nodes = l
  • Total nodes = n − 1

35 Practice MCQs

  1. Bohr radius for H is — (A) 0.529 Å (B) 1.058 Å (C) 5.29 Å (D) 0.0529 Å
  2. Energy of H atom in n=1 — (A) −13.6 eV (B) −3.4 eV (C) +13.6 eV (D) 0
  3. Energy of H atom in n=2 — (A) −13.6 eV (B) −3.4 eV (C) −1.51 eV (D) −0.85 eV
  4. Lyman series lies in — (A) UV (B) visible (C) IR (D) far IR
  5. Balmer series lies in — (A) UV (B) visible (C) IR (D) microwave
  6. Hα line is in — (A) Lyman (B) Balmer (C) Paschen (D) Pfund
  7. Number of orbitals in n=3 — (A) 1 (B) 4 (C) 9 (D) 16
  8. Maximum electrons in n=3 — (A) 2 (B) 8 (C) 18 (D) 32
  9. Number of f orbitals — (A) 1 (B) 3 (C) 5 (D) 7
  10. Maximum value of ml for l=2 — (A) ±1 (B) ±2 (C) ±3 (D) 0
  11. 3p subshell electrons — (A) 2 (B) 6 (C) 10 (D) 14
  12. de Broglie wavelength of an electron at 100 V is — (A) 12.27 Å (B) 1.227 Å (C) 0.1227 Å (D) 12.27 nm
  13. Heisenberg’s principle: Δx·Δp ≥ — (A) h (B) h/2 (C) h/(4π) (D) h/π
  14. Threshold frequency for K (work function 2.3 eV) — (A) 5.55×10¹⁴ Hz (B) 1.0×10¹⁵ Hz (C) 1.5×10¹⁵ Hz (D) 7.0×10¹⁴ Hz
  15. Stopping potential depends on — (A) frequency (B) intensity (C) both (D) neither
  16. Photoelectric current depends on — (A) frequency (B) intensity (C) both (D) neither
  17. The Aufbau order: 4s vs 3d — fills first — (A) 3d (B) 4s (C) simultaneously (D) depends on element
  18. Cu electronic config — (A) [Ar]3d⁹4s² (B) [Ar]3d¹⁰4s¹ (C) [Ar]3d¹⁰4s² (D) [Ar]3d⁸4s²
  19. Cr electronic config — (A) [Ar]3d⁴4s² (B) [Ar]3d⁵4s¹ (C) [Ar]3d⁶4s⁰ (D) [Ar]3d³4s³
  20. Total nodes in 3p orbital — (A) 0 (B) 1 (C) 2 (D) 3
  21. Radial nodes in 3p — (A) 0 (B) 1 (C) 2 (D) 3
  22. Angular nodes in 4d — (A) 0 (B) 1 (C) 2 (D) 4
  23. Quantum number determining orbital shape — (A) n (B) l (C) ml (D) ms
  24. For 4s subshell: l = (A) 0 (B) 1 (C) 2 (D) 3
  25. Pauli’s exclusion principle states — (A) no two electrons same quantum numbers (B) electrons fill lowest energy first (C) maximize unpaired (D) all are random
  26. Speed of electron in n=2 of H = — (A) 1.09×10⁶ m/s (B) 2.18×10⁶ m/s (C) 4.36×10⁶ m/s (D) 1.5×10⁷ m/s
  27. Hund’s rule applies to — (A) degenerate orbitals (B) different shells (C) all atoms (D) noble gases
  28. Wavelength of first line of Lyman series of H ≈ — (A) 121.6 nm (B) 656.3 nm (C) 91.2 nm (D) 410 nm
  29. The number of electrons with n=3, l=2 in iron — (A) 6 (B) 5 (C) 4 (D) 0 (no 3d in Fe? actually Fe = [Ar]3d⁶4s²)
  30. Photon momentum p = (A) hν/c (B) hλ (C) h/c (D) hc
  31. Compton effect demonstrated — (A) wave nature of light (B) particle nature of light (C) wave nature of matter (D) zero rest mass
  32. Davisson-Germer experiment proved — (A) wave nature of electrons (B) particle nature (C) Bohr’s model (D) Pauli’s principle
  33. Schrödinger equation gives — (A) wave function ψ (B) trajectory (C) classical orbit (D) field
  34. The probability density is — (A) ψ (B) ψ² (C) ψ⁻¹ (D) ψ + ψ*
  35. Zeeman effect is — (A) splitting of spectral lines in magnetic field (B) photoelectric (C) Compton (D) Doppler

Answer Key

1-A, 2-A, 3-B, 4-A, 5-B, 6-B, 7-C, 8-C, 9-D, 10-B, 11-B, 12-B, 13-C, 14-A, 15-A, 16-B, 17-B, 18-B, 19-B, 20-C, 21-B, 22-C, 23-B, 24-A, 25-A, 26-A, 27-A, 28-A, 29-A, 30-A, 31-B, 32-A, 33-A, 34-B, 35-A

FAQ

How many questions from Atomic Structure in JEE Main 2027?

Typically 2–3 questions, mostly numerical (Bohr radius/energy, de Broglie, photoelectric).

Should I memorise spectrum series wavelengths?

Memorise the series names + their final n + spectrum region. Specific wavelengths are derivable from Rydberg’s formula in the exam.

Which is the highest-yield formula here?

Rydberg’s: 1/λ = RH·Z²(1/n₁² − 1/n₂²). Combined with En = −13.6Z²/n² eV, these two cover 70% of JEE Atomic Structure numerics.

Are anomalous configs of Cr, Cu important?

Yes — Cr [Ar]3d⁵4s¹ and Cu [Ar]3d¹⁰4s¹ are recurrent JEE asks for “exception to Aufbau”.

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