π Introduction: Dwarf Planet Showdown
Welcome to a comparative study of three fascinating dwarf planets: Pluto, Ceres, and Eris. This lesson will explore their key characteristics, differences, and similarities. Get ready to discover the unique features of these celestial bodies!
π― Objectives
π― Learn the definition of a dwarf planet according to the International Astronomical Union (IAU).
- π Identify the location of Pluto, Ceres, and Eris within our solar system.
- π Compare the size, mass, and composition of these three dwarf planets.
- π‘οΈ Contrast the surface conditions and atmospheric properties (if any) of each dwarf planet.
π§ͺ Materials
- π Internet access for research and simulations
- π Notebook and pen for note-taking
- πΌοΈ Images and videos of Pluto, Ceres, and Eris
- π Comparative data tables (provided below)
π Warm-up (5 mins)
- β What comes to mind when you hear the word 'planet'?
- π What do you already know about Pluto?
- π‘ Have you heard of Ceres or Eris before? What do you know about them?
π Main Instruction
Defining Dwarf Planets: According to the IAU, a dwarf planet is a celestial body that:
- π Is in orbit around the Sun.
- βοΈ Has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape.
- ποΈ Has not cleared the neighbourhood around its orbit.
- π Is not a satellite.
π Pluto
- π Location: Kuiper Belt
- π Diameter: Approximately 2,377 km
- Composition: Primarily rock and ice
- π‘οΈ Surface: Covered in nitrogen, methane, and carbon monoxide ices
- π¨ Atmosphere: Thin, temporary atmosphere that exists when Pluto is closest to the Sun
- π Moons: Has five known moons, including Charon, its largest moon
βοΈ Ceres
- π Location: Asteroid Belt
- π Diameter: Approximately 940 km
- Composition: Rocky core surrounded by an icy mantle
- π§ Surface: Evidence of water ice and hydrated minerals
- π¨ Atmosphere: No significant atmosphere
- π Moons: None
π Eris
- π Location: Scattered Disc
- π Diameter: Approximately 2,326 km
- Composition: Likely similar to Pluto, composed of rock and ice
- π‘οΈ Surface: Covered in methane ice
- π¨ Atmosphere: Possible temporary atmosphere when Eris is closest to the Sun
- π Moons: Has one known moon, Dysnomia
π Comparative Data Table
| Feature |
Pluto |
Ceres |
Eris |
| Location |
Kuiper Belt |
Asteroid Belt |
Scattered Disc |
| Diameter (km) |
2,377 |
940 |
2,326 |
| Composition |
Rock and ice |
Rocky core, icy mantle |
Rock and ice |
| Atmosphere |
Temporary |
None |
Possible temporary |
| Moons |
5 |
0 |
1 |
β
Assessment
β Which dwarf planet is located in the Asteroid Belt?
- π Briefly describe the key differences between Pluto and Eris.
- π‘ Explain why Pluto is no longer classified as a planet.
- π Compare the composition of Ceres to that of Pluto.
- π Which of the three dwarf planets is the largest?