Meteors and Meteorites Notes
Module 7: Meteors and Meteorites
Definition of Key Terms
- Meteoroid
- Small rocky or metallic object
- Located in outer space
- Generally less than 10m in size
Characteristics of Meteors
- Meteor
- A meteoroid that vaporizes upon entering Earth’s atmosphere
- Often seen as a flash or streak of light in the night sky
- Compositions
- Pieces of meteoroids, asteroids, or comets
- Frequency of visibility
- Approximately one meteor can be observed every 10 minutes
- Commonly referred to as “shooting stars”
Understanding Meteorites
- Meteorite
- A meteoroid that survives its passage through the atmosphere and lands on Earth
- Contributes to Earth’s mass, adding approximately 300 tons per day
- Characteristics
- Usually very small but dense
- Most often composed of rock; some are made of iron and nickel
- Similar in composition to terrestrial rocky planets and the moon
Types of Meteorites
- Classifications of Meteorites
- Stony Meteorites
- Iron Meteorites
- Very dense, metallic appearance
- Stony-Iron Meteorites
- The rarest type; contains both stony and metallic elements
Carbonaceous Meteorites
- Characteristics
- Typically black or dark gray
- Originates from carbonaceous asteroids
- Significance
- Radiometric dating indicates they are very old (4.4-4.6 billion years old)
- Similar in age to Moon rocks
Impacts on Earth
- Historic Meteor Events
- Tunguska Event (1908)
- Occurred in Siberia, caused by an 80m meteoroid
- Exploded in the air with energy comparable to a 10 megaton nuclear bomb
- Resulted in darkened skies in California
- Chelyabinsk Event (2013)
- Exploded 20 miles above a lake in Russia
- Resulted in 1600 injuries but zero fatalities
Craters on Earth
- Formed by large meteorite impacts
- Over 200 craters identified on Earth, with less than 500 million years old
- Barringer Crater
- Formed by a 200,000 ton meteoroid (50m in diameter)
- 25 tons of fragments discovered
Meteor Showers
- Occur when Earth passes through debris trails left by comets
- Approximately 30 meteor showers occur annually
- Named after the constellation from which they appear to originate
Notable Meteorites
- Allende Meteorite
- Discovered in Mexico in 1969
- Contained isotopes formed during supernova events, dated to 4.6 billion years ago
- Suggests that the solar system may have formed from a supernova shockwave
- Cretaceous-Paleogene Extinction (65 million years ago)
- First hypotheses discovered in Italy
- Possible causes include dust blocking sunlight or resulting wildfires
- Chicxulub Impact Crater
- Evidence found in Mexico, with structure partially on land and partially underwater
- Evidence of Prior Extinction Events
- Additional findings indicate another mass extinction occurred 250 million years ago as a result of asteroid impact.