Inside the Asteroid Belt
Students discover that the asteroid belt is mostly empty space, learn how Jupiter's gravity kept a planet from forming there and carved the Kirkwood gaps, and compare rocky, metallic and carbon-rich asteroids by visiting Ceres, Vesta, Pallas and Psyche.
Grades 5-8About 15 minutes of narrated flight, plus discussion stops9 stops
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What students will see and do
Students view the solar system from above, then fly to Mars, Jupiter, back above the belt, and into the belt to Ceres, Vesta, Pallas and Psyche before ending at Earth. Aetherion pauses for discussion at Mars (movie asteroid fields versus the real, mostly empty belt), above the solar system (how resonance with Jupiter clears the Kirkwood gaps, using a swing analogy) and at Psyche (what a metal-rich asteroid could teach about planetary cores).
Learning objectives
- Describe where the main asteroid belt is and how spread out its asteroids really are.
- Explain how Jupiter's gravity kept a planet from forming in the belt and created the Kirkwood gaps.
- Compare rocky (stony), metallic and carbon-rich asteroids and how scientists tell them apart.
- Identify Ceres, Vesta, Pallas and Psyche and one key fact about each.
NGSS connections
| MS-ESS1-2 | Students explain how Jupiter's gravity shapes the asteroid belt, including orbital resonances that clear the Kirkwood gaps. |
|---|---|
| MS-ESS1-3 | Students compare the sizes, compositions and spacing of asteroids and relate them to the scale of the solar system. |
Stops on this journey
- A Ring Around the Sun
- Emptier Than You Think (discussion stop)
- Jupiter in Charge
- The Kirkwood Gaps (discussion stop)
- Ceres, the Giant of the Belt
- Vesta, the Bright Rock
- Pallas and the Asteroid Families
- Psyche, a World of Metal (discussion stop)
- Pieces of the Belt at Home
Vocabulary
- asteroid
- asteroid belt
- Kirkwood gap
- orbital resonance
- meteorite
- dwarf planet
- carbon-rich asteroid
- metallic asteroid