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Vagabonds of the Solar System Chapter 17

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Page 1: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Vagabonds of the Solar System

Chapter 17

Page 2: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Guiding Questions

1. How and why were the asteroids first discovered?2. Why didn’t the asteroids coalesce to form a single

planet?3. What do asteroids look like?4. How might an asteroid have caused the extinction of the

dinosaurs?5. What are the differences among meteoroids, meteors,

and meteorites?6. What do meteorites tell us about the way in which the

solar system formed?7. Why do comets have tails?8. Where do comets come from?9. What is the connection between comets and meteor

showers?

Page 3: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

A search for a planet between Mars and Jupiter led to the discovery of asteroids

• Astronomers first discovered the asteroids while searching for a “missing planet”

• Thousands of asteroids with diameters ranging from a few kilometers up to 1000 kilometers orbit within the asteroid belt between the orbits of Mars and Jupiter

Page 4: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 5: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 6: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

The asteroids are the relics of planetesimalsthat failed to accrete into a full-sized planet, thanks to the effects of Jupiter and other Mars-sized objects.

Page 7: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Jupiter’s gravity helped shape the asteroid belt

• Even today, gravitational perturbations by Jupiter deplete certain orbits within the asteroid belt

• The resulting gaps, called Kirkwood gaps, occur at simple fractions of Jupiter’s orbital period

Page 8: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Jupiter’s gravity also captures asteroids in two locations, called Lagrangian points, along Jupiter’s orbit

Page 9: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 10: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 11: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 12: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Asteroids occasionally collide with one another

• Asteroids undergo collisions with each other, causing them to break up into smaller fragments

Page 13: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Asteroids are found outside the asteroid belt—and have struck the Earth

• Some asteroids, called near-Earth objects, move in elliptical orbits that cross the orbits of Mars and Earth

• If such an asteroid strikes the Earth, it forms an impact crater whose diameter depends on both the mass and the speed of the asteroid

Page 14: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 15: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

An asteroid may have struck the Earth 65 million years ago, possibly causing the extinction of the dinosaurs and

many other species

Page 16: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 17: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Small rocks in space are called meteoroids

• If a meteoroid enters the Earth’s atmosphere, it produces a fiery trail called a meteor

• If part of the object survives the fall, the fragment that reaches the Earth’s surface is called a meteorite

Page 18: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Meteorites are classified as stones, stony irons,or irons, depending on their composition

Page 19: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 20: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Irons and stony irons are fragments of the core of an asteroid that was large enough and hot enough to have undergone

chemical differentiation, just like a terrestrial planet

Page 21: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Some meteorites retain traces of the early solar system

• Some stony meteorites come from the crust of such differentiated meteorites, while others are fragments of small asteroids that never underwent differentiation

• Rare stony meteorites called carbonaceous chondrites may be relatively unmodified material from the solar nebula

• These meteorites often contain organic material and may have played a role in the origin of life on Earth

• Analysis of isotopes in certain meteorites suggests that a nearby supernova may have triggered the formation of the solar system 4.56 billion years ago

Page 22: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

A comet is a dusty chunk of ice that partiallyvaporizes as it passes near the Sun

Page 23: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

• A comet is a chunk of ice with imbedded rock fragments that generally moves in a highly elliptical orbit about the Sun

Page 24: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

As a comet approaches the Sun, its icy nucleus develops a luminous coma, surrounded by a vast hydrogen envelope

Page 25: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

An ion tail and a dust tail extend from the comet, pushed away from the Sun by the solar wind and radiation pressure

Page 26: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 27: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 28: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 29: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Comets originate either from a belt beyond Plutoor from a vast cloud in near interstellar space

• The Oort cloud contains billions of comet nuclei in a spherical distribution that extends out to 50,000 AU from the Sun

• Intermediate period and long-period comets are thought to originate in the Oort cloud

• As yet no objects in the Oort cloud have been detected directly

Page 30: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 31: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

• The Kuiper belt lies in the plane of the ecliptic at distances between 30 and 500 AU from the Sun

• It is thought to contain many tens of thousands of comet nuclei

Page 32: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

• Many Jupiter-family comets probably come from the Kuiper belt, and hundreds of larger objects have been observed in the Kuiper belt

Page 33: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Comets eventually break apart, and their fragments give rise to meteor showers

Page 34: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

• Fragments of “burned out” comets produce meteoritic swarms

• A meteor shower is seen when the Earth passes through a meteoritic swarm

Page 35: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to
Page 36: Vagabonds of the Solar System Chapter 17. Guiding Questions 1.How and why were the asteroids first discovered? 2.Why didn’t the asteroids coalesce to

Key Words• amino acids• asteroid• asteroid belt• carbonaceous chondrite• coma (of a comet)• comet• differentiated asteroid• dust tail• fusion crust• Hirayama family• hydrogen envelope• intermediate-period comet• iron meteorite (iron)• ion tail• Jupiter-family comet• Kirkwood gaps• Kuiper belt• long-period comet

• meteor• meteor shower• meteorite• meteoritic swarm• meteoroid• minor planet• near-Earth object (NEO)• nucleus (of a comet)• Oort cloud• radiant (of a meteor shower)• radiation pressure• stable Lagrange points• stony iron meteorite• stony meteorite (stone)• supernova• tail (of a comet)• Trojan asteroid• undifferentiated asteroid• Widmanstätten patterns