Students use the mathematical constant pi to measure the approximate size of the shadow that will fall on Earth during a total solar eclipse.

Students use the Danjon Scale of Lunar Eclipse Brightness to illustrate the range of colors and brightness the Moon can take on during a total lunar eclipse.

Students learn about scale models and distance by creating a classroom-size Earth-Moon system.

Students use mobile devices to measure the impact a solar eclipse has on the energy received at Earth’s surface.

In this illustrated problem set, students use the mathematical constant pi to solve real-world science and engineering problems related to craters on Mars, a total solar eclipse, a daring orbit about Saturn, and the search for habitable worlds.

Students use math concepts related to transits to discover real-world data about Mercury, Venus and planets outside our solar system.

Students learn about the phases of the moon by acting them out.