• Educator Background

    We don't experience eclipses every month on Earth because the orbit of the Moon is tilted with respect to Earth's orbit around the Sun, causing the Sun-Moon-Earth alignment needed for an eclipse to be less frequent. Eclipses only occur around the time of the equinoxes, which is a direct connection with the different orbital planes of Earth and the Moon.

  • Learning Constraints

    At the high school level, students are applying math to predict the motion of objects in the Solar System (HS-ESS1-4) and are quantifying Newton's Law of Gravity and Kepler's Laws of Motion (HS-PS2-4).

  • Connect to Heliophysics

    Connect to the Sun by having students explore how the motions of Earth and the Moon are controlled by gravity (Newton) and how this determines the duration of eclipses and other variables that affect the appearance of the eclipse, for example the type of eclipse. The elliptical shape of the Moon’s orbit around Earth determines whether we experience an annular or total solar eclipse (Kepler).

  • Extend Exploration

    Extend student exploration by investigating why orbits change over time. Have them use their calculations to model how scientists predict future eclipses and to predict when the last total solar eclipse will be possible on Earth.

  • Differentiate for Beginner Learners

    Support beginner students by having them develop models for the basic mechanics of eclipses, including the stages of an eclipse (MS-ESS1-2,3).

  • Differentiate for More Advanced Learners

    Challenge students at the next level by having them investigate the scientific breakthroughs made by scientists by observing the Sun during a total solar eclipse, including evidence used to prove Einstein's General Theory of Relativity.

Featured Advanced Resources

Explore this guiding question with these featured advanced level resources.

Early drawings of eclipses

Lesson Plan

What Do Scientists Learn About the Universe From Observing Solar Eclipses?

Layers of semi-opaque red colored gas and dust, bottom left, with three prominent pillars rise toward the top right. The left pillar is the largest and widest, the second and third pillars are set off in darker shades of brown and have red outlines.

Digital Activity

Learning from Stars and Solar Eclipses

Hands-on Activity

Modeling the Sun-Earth-Moon System

Math-infused Activity

Angular Momentum and Kepler's Second Law