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ar System Debris: or Bodies of the Solar System Asteroids Comets Meteoroids

Solar System Debris: Minor Bodies of the Solar System

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Solar System Debris: Minor Bodies of the Solar System. Asteroids Comets Meteoroids. ~few hundred miles. sand grain. How big?. Everywhere!. * Where are they?. . . . But concentrated mainly in the:. Main Asteroid Belt Kuiper Belt Oort Cloud. Asteroids. * Debris left-over - PowerPoint PPT Presentation

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Page 1: Solar System Debris: Minor Bodies of the Solar System

Solar System Debris:Minor Bodies of the Solar System

Asteroids

Comets

Meteoroids

Page 2: Solar System Debris: Minor Bodies of the Solar System

Howbig?

~few hundred miles

sandgrain

Page 3: Solar System Debris: Minor Bodies of the Solar System

* Where are they?

Everywhere!

. . . But concentrated mainly in the:

1. Main Asteroid Belt

2. Kuiper Belt

3. Oort Cloud

Page 4: Solar System Debris: Minor Bodies of the Solar System

Asteroids

Page 5: Solar System Debris: Minor Bodies of the Solar System

* Debris left-overfrom solar systemformation!

Average separation 4 million miles

p. 197

Page 6: Solar System Debris: Minor Bodies of the Solar System

Ida & Dactyl

35 mi

Page 7: Solar System Debris: Minor Bodies of the Solar System

Asteroidsviewedfrom Earth

p. 198

Page 8: Solar System Debris: Minor Bodies of the Solar System

Asteroid433 Eros

20 mi

Near-Earth Asteroids: Orbits pass near and/or cross Earth’s orbit.

Page 9: Solar System Debris: Minor Bodies of the Solar System
Page 10: Solar System Debris: Minor Bodies of the Solar System
Page 11: Solar System Debris: Minor Bodies of the Solar System

Asteroid 1994 XM1

Missed Earth by 65,000 mi!

Page 12: Solar System Debris: Minor Bodies of the Solar System

Comets

Page 13: Solar System Debris: Minor Bodies of the Solar System

Kuiper Belt

Page 14: Solar System Debris: Minor Bodies of the Solar System

Kuiper Belt Object(KBO) 1993 SC

4.6 hrs

* KBOs: mainly icy in composition ?

Is Pluto just the largest KBO?

Galaxy

Page 15: Solar System Debris: Minor Bodies of the Solar System

OortCloud

somecomets

originatehere

100,000 AU

p. 203

Page 16: Solar System Debris: Minor Bodies of the Solar System

Many comets orbitwell out of planeof planets’ orbits.

Page 17: Solar System Debris: Minor Bodies of the Solar System

Comet Hyakutake (1996)

~ 50o

Page 18: Solar System Debris: Minor Bodies of the Solar System

Comet Hale-Bopp(1997)

Ion tail: ions energizedby solar photons.

Dust tail: dust particlesscatter (reflect) sunlight.

Nucleus: ice withintermixed ‘gravel.’ .p. 201

Page 19: Solar System Debris: Minor Bodies of the Solar System

March 1, 2001: Hale-Bopp~13 AU from Sun

Page 20: Solar System Debris: Minor Bodies of the Solar System

Comet tails alwayspoint away from the sun.

Solar wind +radiation pressure

p. 202

Page 21: Solar System Debris: Minor Bodies of the Solar System

Nucleus of Comet Halley

“Dirty Snowball”

Page 22: Solar System Debris: Minor Bodies of the Solar System

Comet Borrelly

5 mi

Page 23: Solar System Debris: Minor Bodies of the Solar System

Periodic comets eventually evaporate . . . Some break up near the sun . . .

Page 24: Solar System Debris: Minor Bodies of the Solar System

. . . And some comets dive into the sun.

Page 25: Solar System Debris: Minor Bodies of the Solar System

Meteoroids

Page 26: Solar System Debris: Minor Bodies of the Solar System

* Stuff falls on Earth continuously – most of it harmlessly.

Meteor – streak oflight caused by heating of Meteoroidas it passes throughEarth’s atmosphere.

Page 27: Solar System Debris: Minor Bodies of the Solar System

Meteorite – piece of meteoroid that reaches the ground.

Page 28: Solar System Debris: Minor Bodies of the Solar System

Large meteoroids:chipped from asteroids

Small meteoroids:comet debris

Meteor showers

Page 29: Solar System Debris: Minor Bodies of the Solar System

Leonid Shower(mid-November)

Page 30: Solar System Debris: Minor Bodies of the Solar System

Radiant

Leo

November, 2001

Page 31: Solar System Debris: Minor Bodies of the Solar System

Leonid Storm of Nov 17, 1966

Page 32: Solar System Debris: Minor Bodies of the Solar System

“Thirteen of us, mostly students, drove to observe and record the Leonids atop Kitt Peak on the night of Nov. 16-17, 1966. We formed a circle of chairs and began to study our assigned areas of the sky for meteors. It started off slowly, about 30/hour. After 3 hours it picked up dramatically, and we observed a peak of about 40/second that lasted for 10 to 20 minutes. This was 24,000 in a ten minute period, a rate of 144,000/hour. We stood in awe as the sky seemed filled with meteors.”