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Solar System Debris - Asteroids - Comets - Meteoroids. Asteroids - First one discovered in 1801 - 1,000’s catalogued, probably millions exist - largest is Pallas (520 km in dia.) - most less than 1 km in dia. - composed of rock - most reside in the Asteroid belt, 2 - 3.5 AU from Sun.
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Solar System Debris - Asteroids - Comets - Meteoroids
Asteroids - First one discovered in 1801 - 1,000’s catalogued, probably millions exist - largest is Pallas (520 km in dia.) - most less than 1 km in dia. - composed of rock - most reside in the Asteroid belt, 2 - 3.5 AU from Sun
- Trojan Asteroids: 60 degrees in front of and behind Jupiter - Apollo Asteroids: have Earth-crossing orbits
Ida Dactyl
Asteroid Types - C-type: Carbon-rich (carbonaceous), very dark (3-4% reflectivity), primitive, 75% of all asteroids
- S-type: Stony composition not as dark (20% reflectivity), primitive, 17% of all asteroids
- M-type: Metallic composition (Fe, Ni) not as dark (20% reflectivity), differentiated, 8% of all asteroids
The Evidence 1. The K-T boundary No Dinosaur fossils K-T Boundary Dinosaur fossils
- chunks of ice, dust and rock - ices: water, methane, ammonia - contain hydrocarbons, amino acids - most located in the Kuiper Belt and Oort Cloud - probably billions exist in our solar system
Dust Tail Ion Tail Sun
1. Meteoroids: small chunks of asteroids or debris from comets 2. Meteors: trail of ionized air as meteoroid passes through atmosphere 3. Meteorites: a meteoroid that reaches the ground
Meteorites - Stony (95%) - Iron (4%) - Stony-Iron (1%) - Carbonaceous Chondrites: stony meteorites with carbon compounds, water, and amino acids
Meteor showers - Earth passes through debris trail from a comet - occur regularly
Some Meteor Showers Name Date of Meteors / Hour Parent Maximum at Max Quadrantids Jan. 4 110 -- Perseids Aug. 12 68 Comet 1862 III Orionids Oct. 21 30 Comet Halley Leonids Nov. 17 10 Comet P/Tempel-Tuttle Geminids Dec. 14 58 3200 Phaethon