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Nuclear Chemistry and Radioactivity — Class 11 MCQs with Answers

Class 11 CBSE Chemistry · Chapter 307

40 practice questions · 20 Easy · 20 Medium · Updated

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Practise the most important Class 11 CBSE Chemistry questions from Chapter 307, "Nuclear Chemistry and Radioactivity". You get 4 timed quizzes made from 40 NCERT-based MCQs, with answers and explanations. The questions are split into 20 Easy and 20 Medium. Warm up on the basics, then move on to the exam-level questions that top scorers in CBSE & Maharashtra HSC Board exams, JEE Main, MHT-CET, JEE Advanced and NEET UG get right.

To score well in "Nuclear Chemistry and Radioactivity", focus on reactions, key concepts and careful numericals. Each MCQ here is timed and uses exam-style marking (+4 correct, −1 wrong, 0 skipped). This helps you stay accurate when time is short, just as real papers need. Every question has a short explanation, so a wrong answer becomes a quick lesson. It is the fastest way to fix gaps before a test.

Use this chapter for focused revision. Start with the Easy set to check your basics on Nuclear Chemistry and Radioactivity, then move to Medium to practise applying them. Your accuracy, streaks and XP save automatically. This chapter also adds to your overall Class 11 Chemistry mastery score. Try the 4 sample questions below: tap an option to see the answer and a worked explanation. Sign in free to start practising.

Nuclear Chemistry and Radioactivity — important questions & MCQs with answers (Class 11 Chemistry)

4 solved questions from this chapter's difficulty levels, each with its answer and explanation. Tap an option to check yourself.

0 of 4 answered

  1. Q1 of 4Easy

    Radioactivity was discovered in 1896 while studying the behaviour of uranium salts by

    Show answer

    Answer: Henri Becquerel

    Explanation: Henri Becquerel found that a potassium uranyl sulphate salt fogged a wrapped photographic plate on its own, which showed that uranium emits penetrating radiation spontaneously.

  2. Q2 of 4Easy

    When a nucleus emits one α-particle, its mass number and atomic number change by

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    Answer: mass number decreases by 4, atomic number decreases by 2

    Explanation: An α-particle carries away 2 protons and 2 neutrons, so A falls by 4 and Z falls by 2.

  3. Q3 of 4Medium

    The half-life of a radioactive isotope is 20 minutes. The fraction of the original sample left undecayed after 1 hour is

    Show answer

    Answer: 1/8

    Explanation: 60 minutes is 3 half-lives, and the fraction left is (1/2)³ = 1/8.

  4. Q4 of 4Medium

    Fission of ²³⁵U by a slow neutron can sustain a chain reaction because each fission event

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    Answer: releases 2 to 3 fresh neutrons that can split further nuclei

    Explanation: Each ²³⁵U fission emits 2 to 3 neutrons on average; if enough of them are slowed and captured, the number of fissions multiplies and the reaction becomes self-sustaining.

Nuclear Chemistry and Radioactivity notes: key concepts (Class 11 Chemistry)

Ordinary chemistry rearranges electrons; nuclear chemistry changes the nucleus itself. Beginning with Becquerel's accidental discovery in 1896 that uranium salts fog a wrapped photographic plate, this chapter looks at the three natural radiations α, β and γ and how they differ in charge, mass, ionising power and penetrating power. It then explains why some nuclei are unstable in terms of the neutron-to-proton ratio and the band of stability, works through the decay modes (α, β⁻, β⁺ and electron capture) and the group displacement law, treats decay as a first order rate process with a decay constant, half-life and average life, and finally covers artificial transmutation, fission, fusion, mass defect and binding energy, nuclear reactors and the everyday uses of radioisotopes in dating, medicine and agriculture.

Radioactivity
The spontaneous emission of α, β or γ radiation by an unstable nucleus. It was discovered by Henri Becquerel in 1896 with uranium salts, and Marie and Pierre Curie then isolated polonium and radium from pitchblende. The rate is unaffected by temperature, pressure or chemical combination.
Alpha, beta and gamma radiation
An α-particle is a helium nucleus ⁴₂He²⁺, a β-particle is a fast electron ⁰₋₁e, and a γ-ray is a high energy photon with no charge and no rest mass. Ionising power falls α > β > γ while penetrating power rises in the reverse order α < β < γ; α is stopped by paper, β by thin aluminium and γ needs thick lead.
The penetrating power of the three radiations from a radioactive source in a lead block. α particles are stopped by a sheet of paper. β particles pass through the paper but are stopped by a thin sheet of aluminium. γ rays pass through both and are only reduced in intensity by thick lead, shown by a fainter dashed arrow beyond it. Penetrating power rises α < β < γ while ionising power falls α > β > γ.
n/p ratio and the band of stability
Plotting neutrons against protons for stable nuclides gives a narrow band. Light stable nuclei have n/p about 1, and the ratio rises to roughly 1.5 near the heavy end. Nuclides outside the band are radioactive and every nuclide with atomic number greater than 83 is unstable.
A graph of the number of neutrons n against the number of protons Z for stable nuclides. The stable nuclides lie in a narrow band. For light nuclei the band follows the dashed line n = p (n/p = 1); it curves above that line as Z increases, reaching n/p of about 1.5 near Z = 82. Nuclides above the band have too many neutrons and emit β⁻ particles, moving down towards the band; nuclides below it have too many protons and emit positrons or capture an electron, moving up towards it. Beyond Z = 83 every nuclide is unstable and heavy ones emit α particles.
Modes of decay
A nucleus above the band (too many neutrons) emits a β⁻ particle, turning a neutron into a proton. A nucleus below the band (too many protons) emits a positron or captures a K-shell electron, turning a proton into a neutron. Very heavy nuclides shed mass by α emission, and γ emission simply removes excess energy.
Group displacement law
Stated by Soddy, Fajans and Russell: loss of an α-particle lowers the atomic number by 2 and moves the daughter two groups to the left in the periodic table, while loss of a β⁻ particle raises the atomic number by 1 and moves the daughter one group to the right, with the mass number unchanged.
Decay constant and half-life
Decay obeys first order kinetics, −dN/dt = λN, so N = N₀e^(−λt). The decay constant λ is the fraction of nuclei disintegrating per unit time. The half-life t½ = 0.693/λ is the time for half the sample to decay and is a fixed property of a nuclide, independent of the amount taken.
A graph of the number N of undecayed nuclei against time t. N starts at N₀ and falls along a smooth exponential curve that never reaches zero. Dashed guide lines show that after one half-life T½ the number has fallen to N₀/2, and after 2T½ to N₀/4: in every half-life, half of the nuclei that remain decay. The curve is N = N₀ e^(−λt), where λ is the decay constant.
Average life and activity
Average (mean) life τ = 1/λ = 1.44 t½ is the average survival time of a nucleus. Activity A = λN is the number of disintegrations per unit time; its SI unit is the becquerel (1 Bq = 1 disintegration per second) and the older unit is the curie, with 1 Ci = 3.7 × 10¹⁰ Bq.
Radioactive series and artificial transmutation
Heavy natural nuclides decay in chains, such as the ²³⁸U series that ends at stable ²⁰⁶Pb and the ²³²Th series that ends at ²⁰⁸Pb. Artificial transmutation is the deliberate conversion of one element into another by bombarding it with particles, first done by Rutherford using α-particles on nitrogen to give oxygen and a proton.
Mass defect and binding energy
The actual mass of a nucleus is less than the sum of the masses of its nucleons; this difference Δm is the mass defect and it appears as the binding energy E = Δmc² that holds the nucleus together. Binding energy per nucleon measures stability and peaks near mass number 56, which is why both fission of heavy nuclei and fusion of light nuclei release energy.
A graph of binding energy per nucleon B/A, in MeV, against mass number A from 0 to 250. The curve rises steeply through the light nuclei, reaches a broad peak of about 8.8 MeV near A = 56 (iron), and then falls slowly to about 7.6 MeV at A = 238 (uranium). Light nuclei on the left can release energy by fusion, joining to move up the curve towards the peak; heavy nuclei on the right can release energy by fission, splitting into middle-mass nuclei that sit higher on the curve.
Fission, fusion and reactors
In fission a heavy nucleus such as ²³⁵U splits into two medium fragments plus 2 to 3 neutrons, which can sustain a chain reaction. In fusion light nuclei combine at temperatures near 10⁷ K, as in the sun. A reactor uses fuel rods, a moderator (graphite or heavy water) to slow neutrons, cadmium or boron control rods to absorb them, and a coolant.
A slow neutron strikes a uranium-235 nucleus, which splits into two lighter nuclei, barium-144 and krypton-89, and releases three neutrons and about 200 MeV of energy. The fragments have a higher binding energy per nucleon than uranium, which is where the energy comes from, and the released neutrons can go on to split further uranium nuclei.
Applications of radioisotopes
Carbon dating with ¹⁴C (t½ = 5730 years) fixes the age of once-living material, and ²³⁸U/²⁰⁶Pb ratios date rocks. In medicine ⁶⁰Co gives γ-rays for cancer therapy and ¹³¹I is used for thyroid disorders. In agriculture ³²P traces fertiliser uptake and γ-irradiation preserves food.
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Nuclear Chemistry and Radioactivity — FAQs

What are the key concepts in Class 11 Chemistry Nuclear Chemistry and Radioactivity?+

Ordinary chemistry rearranges electrons; nuclear chemistry changes the nucleus itself. Beginning with Becquerel's accidental discovery in 1896 that uranium salts fog a wrapped photographic plate, this chapter looks at the three natural radiations α, β and γ and how they differ in charge, mass, ionising power and penetrating power. It then explains why some nuclei are unstable in terms of the neutron-to-proton ratio and the band of stability, works through the decay modes (α, β⁻, β⁺ and electron capture) and the group displacement law, treats decay as a first order rate process with a decay constant, half-life and average life, and finally covers artificial transmutation, fission, fusion, mass defect and binding energy, nuclear reactors and the everyday uses of radioisotopes in dating, medicine and agriculture. Key ideas include Radioactivity, Alpha, beta and gamma radiation, n/p ratio and the band of stability, Modes of decay, Group displacement law, Decay constant and half-life.

What does Class 11 Chemistry Chapter 307 (Nuclear Chemistry and Radioactivity) cover on XamBaaz?+

It has 40 NCERT-based MCQs on "Nuclear Chemistry and Radioactivity": 20 Easy and 20 Medium. Together they make 4 timed quizzes, and you never get the same set twice. Every question has an instant explanation. They help you prepare for CBSE & Maharashtra HSC Board exams, JEE Main, MHT-CET, JEE Advanced and NEET UG.

Are these "Nuclear Chemistry and Radioactivity" questions free to practise?+

Yes. Sign in with Google to practise "Nuclear Chemistry and Radioactivity" free. Full unlimited access is ₹1,999/year. One year from the day you pay. You stay in Class 11 till 31 March; on 1 April your account moves up to Class 12 and the rest of your year carries over. No chapter is charged separately.

How should I revise "Nuclear Chemistry and Radioactivity" for the exam?+

Start with the Easy quiz to check your basics, then try Medium to practise applying them. There are 4 timed quizzes on this chapter, so you can come back for a fresh set instead of one you have seen. Read each explanation, retry the questions you miss, and track your accuracy until it stays high.

Are these "Nuclear Chemistry and Radioactivity" MCQs available with answers?+

Yes. 4 sample questions are on this page with answers: tap an option, or "Show answer", to see the correct option and a step-by-step explanation. Sign in free with Google to start practising, with instant scoring.

Is there negative marking in the "Nuclear Chemistry and Radioactivity" quizzes?+

Yes. The timed quizzes use exam-style marking: +4 for a right answer, −1 for a wrong one and 0 for a skip, the same negative marking as JEE Main, JEE Advanced and NEET UG. MHT-CET and CBSE board papers have no negative marking. Our mocks for those are scored their way.

What are the important questions from Nuclear Chemistry and Radioactivity (Class 11 Chemistry)?+

The questions that matter most test Radioactivity, Alpha, beta and gamma radiation, n/p ratio and the band of stability, Modes of decay, Group displacement law, Decay constant and half-life. This page shows 4 solved important MCQs with answers and explanations. Sign in to practise all 40 questions on the chapter as timed quizzes.

Is there an online quiz for Nuclear Chemistry and Radioactivity?+

Yes — Class 11 Chemistry Nuclear Chemistry and Radioactivity has timed online quizzes at Easy and Medium levels, with instant scoring and a worked explanation on every question. The first quiz on the chapter is free.

Are there question answers and extra questions for Nuclear Chemistry and Radioactivity (Class 11 Chemistry)?+

Yes. This page has 4 solved questions on Nuclear Chemistry and Radioactivity, each with the correct answer and a short explanation. Sign in to practise all 40 questions on the chapter as timed quizzes.

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