Model Answer
0 min readIntroduction
Meteorites are extraterrestrial rocks that have survived passage through the Earth’s atmosphere and impacted its surface. They provide valuable insights into the early solar system’s composition and formation processes. These celestial visitors are broadly classified based on their bulk composition, which reflects their origin within asteroids, planets, or even comets. Understanding these classifications is crucial for deciphering the history of our solar system.
Types of Meteorites
Meteorites are categorized into three main types:
1. Stony Meteorites ( ~95% of falls)
- Chondrites: Contain chondrules – small, round grains formed in the early solar system. They are the most primitive meteorites.
- Achondrites: Lack chondrules and are formed from differentiated parent bodies (asteroids that melted and formed layers). Examples include HED meteorites (Howardites, Eucrites, Diogenites).
2. Iron Meteorites (~5% of falls)
Composed primarily of iron-nickel alloy. They originate from the cores of differentiated asteroids that were shattered by collisions.
- Octahedrites: Most common type, exhibiting Widmanstätten patterns (crystal structures) when etched.
- Hexahedrites: Contain a higher nickel content and less common patterns.
3. Stony-Iron Meteorites (~1% of falls)
A mixture of silicate minerals and iron-nickel metal.
- Pallasites: Contain olivine crystals embedded in an iron-nickel matrix.
- Mesosiderites: Breccias (rocks composed of fragments) containing silicate and metal components.
| Type | Composition | Origin |
|---|---|---|
| Stony (Chondrite) | Silicates, Chondrules | Primitive Asteroids |
| Iron (Octahedrite) | Iron-Nickel Alloy | Asteroid Cores |
| Stony-Iron (Pallasite) | Silicates & Iron-Nickel | Core-Mantle Boundary of Asteroids |
Conclusion
In conclusion, meteorites are classified primarily by their composition – stony, iron, and stony-iron – each providing unique clues about the formation and evolution of the solar system. The study of these extraterrestrial rocks continues to refine our understanding of planetary processes and the origins of Earth itself. Further research, including isotopic analysis, helps pinpoint their specific parent bodies and refine our cosmological models.
Answer Length
This is a comprehensive model answer for learning purposes and may exceed the word limit. In the exam, always adhere to the prescribed word count.