Mississippi Science PHY.6.3

ScienceGrades 9–12Physics

The Standard

PHY.6
Students will demonstrate an understanding of the basic principles of nuclear energy.
Investigate the conservation of mass and the conservation of charge by writing and balancing nuclear decay equations for alpha and beta decay.

2026 Mississippi College- and Career-Readiness Standards for Science · Nuclear Energy

Teacher's field guide

What This Standard Means

What Students Need to Do

Students write alpha and beta-minus decay equations from a parent isotope. They find the daughter isotope by balancing mass numbers and atomic numbers on both sides. They treat mass number as a count of protons and neutrons, not exact measured mass.

What Mastery Looks Like

Given an unfamiliar isotope, students can write its alpha or beta-minus decay equation and name the daughter isotope. They check both number sums, including the emitted electron's zero mass number and negative charge.

Common Misconceptions

Students often subtract four from both numbers in alpha decay, though the atomic number drops by two. They may think beta-minus decay removes an electron from the atom rather than changing a neutron into a proton. Some mistake mass number for exact measured mass, which can change as energy is released.

How to Assess It

Exit ticket: Fill in ²³⁸₉₂U → ___ + ⁴₂He and ¹⁴₆C → ___ + ⁰₋₁e, then show the mass-number and charge sums for each.

Lesson moves

Ways to Teach It

  1. Give pairs 6 red proton counters, 8 blue neutron counters, and an electron slip; have them model carbon-14 beta-minus decay and write the equation.

  2. Ask, "Why does carbon-14 become nitrogen-14 if its mass number stays 14?" Have students explain using proton and neutron counts.

  3. Play decay match: students pair parent isotope cards with daughter and emitted particle cards, then check both number sums.

  4. Show a carbon-dating diagram; ask students to write the decay equation that produces nitrogen-14 and check both number sums.

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