Structure of Atom Class 11 NCERT true-false

Updated for 2026 Boards • JEE • NEET

Structure of Atom Class 11 – True/False Practice (NCERT Chapter 2)

Test your understanding of modern atomic theory with exam‑style True/False questions. Each statement targets core ideas like models of the atom, quantum numbers, and electronic configuration to sharpen accuracy for Boards, JEE, and NEET.

Last Updated: February 2026 | Practice Set – Instant Feedback

Interactive True/False quiz with instant checking, score tracking, and a downloadable PDF answer sheet containing all questions, correct answers, and brief explanations for your attempted statements.

Academia Aeternum Editorial Team

Reviewed by Subject Experts • Updated Feb 2026

Academia Aeternum Editorial Team

Reviewed by Subject Experts • Updated Feb 2026

Why Structure of Atom MCQs Matter for JEE & NEET

MCQs from this chapter frequently check ideas like quantum numbers, electronic configuration, and spectral lines in a time-bound format. Regular practice improves speed, accuracy, and your grip on conceptual traps.

Exam Trend Analysis • Updated 2026

How Structure of Atom MCQs Appear in JEE & NEET 2026

Recent papers emphasise multi‑concept MCQs linking Bohr’s model, de Broglie relation, and quantum numbers in a single question. Many items are NCERT‑based but framed with tricky options and calculation‑heavy data.

Are You Sure You Understand Atomic Structure?
Most students lose marks in JEE & NEET not because they don’t know theory — but because they misread one word like “always” or “only”.

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1. The charge on an electron is \(-1.602\times10^{-19}\,\text{C}\).
2. Cathode rays consist of positively charged particles.
3. The mass of a proton is approximately equal to that of a neutron.
4. The radius of an atom is of the order \(10^{-10}\,\text{m}\).
5. In Rutherford’s model, electrons remain stationary around the nucleus.
6. Isotopes have the same mass number but different atomic numbers.
7. The atomic number represents the number of neutrons in a neutral atom.
8. The frequency of radiation is inversely proportional to its wavelength: \( \nu=\frac{c}{\lambda} \).
9. Line spectra arise due to electronic transitions between discrete energy levels.
10. The photoelectric effect supports the wave nature of light.
11. According to Bohr, angular momentum of electron is quantized as \(mvr=\frac{nh}{2\pi}\).
12. The ground state of hydrogen corresponds to \(n=0\).
13. The energy of an electron in hydrogen is given by \(E_n=-\frac{13.6}{n^2}\,\text{eV}\).
14. Heisenberg uncertainty principle allows exact position and momentum simultaneously.
15. Orbit and orbital represent the same physical concept.
16. The shape of a \(p\)-orbital is spherical.
17. For a given \(n\), total orbitals equal \(n^2\).
18. The maximum number of electrons in a shell is \(2n^2\).
19. The de Broglie wavelength of a particle decreases with increasing momentum.
20. In multi-electron atoms, orbital energies depend only on \(n\).
21. The order of orbital filling follows the \(n+l\) rule.
22. A node is a region where probability density of finding electron is zero.
23. The number of radial nodes equals \(n-l-1\).
24. The shortest wavelength in X-ray spectra corresponds to complete loss of kinetic energy of electrons.
25. If velocity of an electron doubles, its de Broglie wavelength becomes half.

Frequently Asked Questions

Because a single incorrect term like “always”, “never”, or “only” can make an otherwise correct statement false, testing precision of conceptual understanding.

Check whether the values satisfy allowed limits such as \( n \ge 1 \), \( 0 \le l \le n-1 \), and \( m_l = -l \text{ to } +l \).

In multi-electron atoms, energy depends on both \( n \) and \( l \) due to shielding and penetration effects.

Bohr’s model does not include electron spin or relativistic corrections, so it cannot explain fine structure splitting.

The correct formula is \( 2n^2 \), derived from quantum mechanical considerations.

4s is lower in neutral atoms initially, but after ionization 3d becomes lower in energy.

According to Heisenberg’s uncertainty principle \( \Delta x \Delta p \ge \frac{\hbar}{2} \), exact position and momentum cannot be simultaneously known.

Isotopes differ in mass number, affecting properties like density and rate of diffusion.

Probability density is given by \( \psi^2 \), not \( \psi \) itself.

The energy is negative because it is measured relative to zero at infinite separation.

While degenerate in energy, d-orbitals have different spatial orientations and shapes.

Exceptions occur due to half-filled and fully filled subshell stability (e.g., Be vs B).

Lyman transitions end at \( n=1 \) and lie in the ultraviolet region.

Correct expression is \( \sqrt{l(l+1)}\hbar \), not simply \( n\hbar \).

Only s-orbitals are spherical; p and d orbitals have distinct shapes.

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