Mississippi Science CHE.2.4

ScienceGrades 9–12Chemistry

The Standard

CHE.2
Students will demonstrate an understanding of the atomic structure and the historical developments leading to modern atomic theory.
Research appropriate sources to evaluate the way absorption and emission spectra are used to study astronomy and the formation of the universe.

2026 Mississippi College- and Career-Readiness Standards for Science · Atomic Theory

Teacher's field guide

What This Standard Means

What Students Need to Do

Find reliable sources about light from stars and galaxies. Explain how dark absorption lines and bright emission lines help identify elements. Use shifts in those lines as evidence for cosmic expansion and clues to the early universe.

What Mastery Looks Like

Given a spectrum and reference lines, students identify an element by matching line positions. They explain how redshift across many galaxies supports an expanding universe. They cite a science source and separate what astronomers observe from what they conclude.

Common Misconceptions

Students may think dark lines mean an element is absent, rather than absorbing light at certain wavelengths. They may think redshift means a galaxy looks red, or that one spectrum reveals exactly how the universe began.

How to Assess It

Give students printed hydrogen line references, a redshifted galaxy spectrum, and short explanations from NASA and an unsigned blog. Ask them to match a line, explain its shift, and choose which explanation to cite and why.

Lesson moves

Ways to Teach It

  1. View an incandescent bulb and a fluorescent lamp through diffraction gratings; sketch their patterns, then compare them with printed absorption lines.

  2. Compare a NASA explanation of galaxy redshift with an unsigned blog post; write which claims the evidence supports and which source you would cite.

  3. Give pairs printed hydrogen, helium, and star spectra; have them match line positions and label dark and bright lines.

  4. Use a Sloan Digital Sky Survey galaxy spectrum and a laboratory hydrogen spectrum; mark a shifted line and explain what it suggests.

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Printable CHE.2.4 Worksheet

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