chapter 9a remnants of rock and ice asteroids, comets, and pluto

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Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

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Page 1: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Chapter 9aRemnants of Rock and Ice

Asteroids, Comets, and Pluto

Page 3: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

9.1 Asteroids and Meteorites

Our Goals for Learning

• Why is there an asteroid belt?

• How are meteorites related to asteroids?

Page 4: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Asteroid Facts

• Asteroids are rocky leftovers of planet formation.• Largest is Ceres, diameter ~1,000 km (est. 974 km)• 150,000 in catalogs, and probably over a million with

diameter >1 km.• Small asteroids are more common than large asteroids.• All the asteroids in the solar system wouldn’t add up

to even a small terrestrial planet.

Page 5: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Asteroids are cratered and not round

Page 6: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Types of Asteroid• C type:

– Carbonaceous chondrites, similar in composition to sun without H and He

– 75%

• S type:– Stony (Fe-Mg silicates) with metal– 17%

• M type:– Metallic (Fe-Ni)– About 8%

Page 7: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Why is there an asteroid belt?

Page 8: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

More than 150,000 asteroids at their predicted locations for Jan 1 2004

On this scale, asteroids are much smaller than the dots used to represent them

Page 9: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Why are there very few asteroids beyond Jupiter’s orbit?

A. There was no rocky material beyond Jupiter’s orbit.

B. The heaviest rocks sank towards the center of the solar system.

C. Ice could form in the outer solar system.D. A passing star probably stripped away all of

those asteroids, even if they were there at one time.

Page 10: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Why are there very few asteroids beyond Jupiter’s orbit?

A. There was no rocky material beyond Jupiter’s orbit.

B. The heaviest rocks sank towards the center of the solar system.

C. Ice could form in the outer solar system.D. A passing star probably stripped away all of

those asteroids, even if they were there at one time.

Page 11: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Which explanation seems to be the most plausible?

A. The belt is where all the asteroids happened to form.

B. The belt is the remnant of a large terrestrial planet that used to be between Mars and Jupiter.

C. The belt is where all the asteroids happened to survive.

Page 12: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Which explanation seems to be the most plausible?

A. The belt is where all the asteroids happened to form.

B. The belt is the remnant of a large terrestrial planet that used to be between Mars and Jupiter.

C. The belt is where all the asteroids happened to survive. But WHY didn’t they

form a little planet?

Page 13: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Gravitational interactions (orbital resonances) with Jupiter have ejected asteroids on certain orbits.

Page 14: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Rocky planetesimals survived in the asteroid belt between Mars and Jupiter because they did not accrete into a planet.

Jupiter’s gravity, through the influence of orbital resonances, stirred up asteroid orbits and thereby prevented their accretion into a planet.

Page 15: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

How are meteorites related to asteroids?

Page 16: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

How are meteorites related to asteroids?

Meteorites are pieces of asteroids - or sometimes planets or the Moon.

Sometimes they get close to us LINK

Page 17: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Meteor: The bright tail of hot debris from the rock

Meteorite: A rock from space that reaches Earth’s surface

Page 19: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Meteorite Types

1) Primitive: Unchanged in composition since they first formed 4.6 billion years ago.

2) Processed: Younger, have experienced processes like volcanism or differentiation.

Page 20: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Primitive Meteorites: simple, all ingredients mixed together

Page 21: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Processed Meteorites: shattered fragments of larger objects

Iron from a core

Volcanic rock from a crust or mantle

Page 22: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

What do we learn from meteorites?

• Primitive meteorites tell us what the original planetesimals were like.

• The ages of primitive meteorites tell us when solar system formation began.

• Processed meteorites tell us what asteroids are like on the inside.

• Processed meteorites provide direct proof that differentiation and volcanism happened on asteroids.

Page 23: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

Meteorites from Moon and Mars

• A few meteorites arrive from the Moon and Mars• Composition differs from the asteroid fragments.• A cheap (but slow) way to acquire moon rocks and

Mars rocks.• One Mars meteorite generated a stir when scientists

claimed evidence for microscopic life in it.

Page 24: Chapter 9a Remnants of Rock and Ice Asteroids, Comets, and Pluto

What have we learned?• Why is there an asteroid belt?

• Orbital resonances with Jupiter disrupted the orbits of planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the asteroid belt today. Most asteroids in other regions of the inner solar system accreted into one of the planets.

• How are meteorites related to asteroids?

• Most meteorites are pieces of asteroids. Primitive meteorites are essentially unchanged since the birth of the solar system. Processed meteorites are fragments of larger asteroids that underwent differentiation.