Meteorites: Messengers from the Early Solar System
Meteorites are fragments from solar system bodies, dominantly asteroids. A small fraction is derived from the Moon and from Mars. These rocks tell a rich history of the early solar system and range from solids little changed since the earliest phases of solid matter condensation in the solar nebula...
| Published in: | CHIMIA |
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| Main Author: | |
| Format: | Article in Journal/Newspaper |
| Language: | English |
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Swiss Chemical Society
2010
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| Subjects: | |
| Online Access: | https://www.chimia.ch/chimia/article/view/2010_736 https://doi.org/10.2533/chimia.2010.736 |
| Summary: | Meteorites are fragments from solar system bodies, dominantly asteroids. A small fraction is derived from the Moon and from Mars. These rocks tell a rich history of the early solar system and range from solids little changed since the earliest phases of solid matter condensation in the solar nebula (chondrites) to material representing asteroidal metamorphism and melting, impact processes on the Moon and even aqueous alteration near the surface of Mars. Meteorites are very rare. Currently many meteorites result from searches in Antarctica and the hot deserts of North Africa and Arabia. The present high find rate likely represents a unique short-term event, asking for a careful management of this scarce scientific resource. |
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