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Published byDarcy Robertson Modified over 9 years ago
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Exploring NASA’s Moon Rocks, Lunar Soil Samples & Meteorite Disks!!
National Aeronautics and Space Administration Exploring NASA’s Moon Rocks, Lunar Soil Samples & Meteorite Disks!!
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Lunar Surface Features
Two dramatically different kinds of terrain: Highlands: Mountainous terrain, scarred by craters Light gray/older Lowlands: ~ 3 km lower than highlands; smooth surfaces: Dark gray/younger Maria (pl. of mare): Basins flooded by lava flows
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Impact Cratering Impact craters on the moon can be seen easily even with small telescopes. Ejecta from the impact can be seen as bright rays originating from young craters
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Impact Cratering = ‘Soil’ formation
Impacts of objects hitting the moon have pulverized the moon’s crust to physically break down the rocks to make smaller sand & clay sized particles called lunar soil or ‘Regolith’.
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No sedimentary rocks => No sign of water ever present on the moon.
Moon Rocks All moon rocks brought back to Earth are igneous (= solidified lava) No sedimentary rocks => No sign of water ever present on the moon. Different types of moon rocks: Vesicular (= containing holes from gas bubbles in the lava) basalts, typical of dark rocks found in maria Breccias (= fragments of different types of rock cemented together), also containing anorthosites (= bright, low-density rocks typical of highlands) Older rocks become pitted with small micrometeorite craters
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Moon Rock Sample Disk
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Moon Rock Samples Basalt Breccia Anorthosite
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Lunar Soil Sample Disk
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Lunar Soil Samples Lunar Soil - Orange Lunar Soil - Maria
Lunar Soil - Highlands
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Meteorite Sample Disk
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Meteorite Samples 1-3 EET83227 ALH90411 ALLENDE
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Meteorite Samples 4-6 GIBEON LEW87030 BRENHAM
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