Reading the Night Sky
Students learn why the sky appears to turn, how to use Polaris and pointer patterns to navigate the sky, and why most constellations are chance line-ups of stars at very different distances.
Grades 5-8About 15 minutes of narrated flight, plus discussion stops9 stops
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What students will see and do
Students fly from Earth to Polaris, Vega, Deneb, Arcturus, Orion, Sirius, Betelgeuse and Aldebaran while Aetherion narrates how to star-hop from one pattern to the next. The class pauses at Polaris, Orion and Betelgeuse to discuss latitude, seasonal constellations and star color.
Learning objectives
- Explain that the apparent nightly motion of stars is caused by Earth's rotation and the seasonal change in constellations is caused by Earth's orbit around the Sun.
- Use the Big Dipper's pointer stars and handle, and Orion's belt, to locate Polaris, Arcturus, Sirius and Aldebaran on a star chart.
- Describe how the altitude of Polaris above the horizon relates to an observer's latitude.
- Distinguish between a constellation, an asterism and a true star cluster, using Deneb, Vega, Aldebaran and the Hyades as evidence.
NGSS connections
| MS-ESS1-1 | Students use a model of the Earth-Sun system to explain the daily motion of the stars and why different constellations are visible in different seasons. |
|---|---|
| MS-ESS1-3 | Students compare star distances and brightness to see that patterns in the sky do not reflect real positions in space. |
Stops on this journey
- Why the Sky Turns
- The North Star (discussion stop)
- Vega and the Summer Triangle
- Deneb, the Far Away Giant
- Arc to Arcturus
- Orion the Hunter (discussion stop)
- Sirius, the Brightest Star
- Betelgeuse, the Red Shoulder (discussion stop)
- Aldebaran, the Bull's Eye
Vocabulary
- constellation
- asterism
- celestial sphere
- celestial pole
- latitude
- light-year
- precession
- red supergiant