In this lesson, students use orbital models of the Moon and Venus …
In this lesson, students use orbital models of the Moon and Venus to demonstrate: the moon's apparent diameter changes very little in the course of one complete orbit of the Earth; how if Venus orbited the Earth, there would be little change in its apparent diameter; and how the diameter of Venus's orbit changes greatly as it orbits the Sun.
In this lesson, students build a physical model to simulate the Sun's …
In this lesson, students build a physical model to simulate the Sun's tracks across the sky at the solstices and equinoxes. A bead will be used to illustrate the Sun moving from rising along the eastern horizon to setting on the western.
No restrictions on your remixing, redistributing, or making derivative works. Give credit to the author, as required.
Your remixing, redistributing, or making derivatives works comes with some restrictions, including how it is shared.
Your redistributing comes with some restrictions. Do not remix or make derivative works.
Most restrictive license type. Prohibits most uses, sharing, and any changes.
Copyrighted materials, available under Fair Use and the TEACH Act for US-based educators, or other custom arrangements. Go to the resource provider to see their individual restrictions.
