Mississippi Science E.5.8B

Science5th GradeEarth and Space Science

Standard Cluster

Students will demonstrate an understanding of the principles that govern moon phases, day and night, appearance of objects in the sky, and seasonal changes. Analyze and interpret data from observations and research (e.g., from NASA, NOAA, or the USGS) to explain patterns in the location, movement, and appearance of the moon throughout a month and over the course of a year. Develop and use a model of the Earth-Sun-Moon system to analyze the cyclic patterns of lunar phases, solar and lunar eclipses, and seasons. Develop and use models to explain the factors (e.g., tilt, revolution, and angle of sunlight) that result in Earth’s seasonal changes. Obtain information and analyze how our understanding of the solar system has evolved over time (e.g., Earth-centered model of Aristotle and Ptolemy compared to the Sun-centered model of Copernicus and Galileo).

2026 Mississippi College- and Career-Readiness Standards for Science · Earth and the Universe

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E.5.8B is a cluster heading. These are the individual standards under it.

Teacher's field guide

What This Cluster Means

What Students Need to Do

Students track the Moon’s shape and position using dated sky observations. They use models to explain day and night, Moon phases, eclipses, and seasons. They compare Earth-centered and Sun-centered models with observations.

What Mastery Looks Like

Students can predict the Moon’s next phase from a month of sketches. They use a lamp and globe to show why eclipses happen and why Earth’s tilt causes seasons. They explain why the Sun-centered model better fits observations.

Common Misconceptions

Students may think Earth’s shadow causes ordinary Moon phases or that every full moon brings an eclipse. They may think seasons happen because Earth moves closer to the Sun. Some confuse the Sun’s apparent daily movement with the Sun orbiting Earth.

How to Assess It

Exit ticket: Give students four dated Moon sketches in order. Ask them to draw the next phase and explain why it is not caused by Earth’s shadow.

Lesson moves

Ways to Teach It

  1. Use a lamp, foam Moon ball, and tilted globe to model a lunar eclipse, then compare sunlight on each hemisphere.

  2. Show Galileo’s drawings of Venus’s phases beside Earth-centered and Sun-centered diagrams; ask which diagram explains all the drawings.

  3. Give pairs dated Moon photos from one month; have them order the photos and sketch the next phase.

  4. Use a local moonrise calendar; have students graph four weeks of times and explain why the Moon is not always visible at night.

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