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2. Resources Chapter Presentation Bellringers Image Bank
Standards Assessment
Math Focus
Visual Concepts

3. Chapter 15 Table of Contents Section 1 Stars
Stars, Galaxies, and the Universe
Table of Contents
Section 1 Stars
Section 2 The Life Cycle of the Stars
Section 3 Galaxies
Section 4 Formation of the Universe

4. Chapter 15 Bellringer List ways that stars differ from one another.
Section 1 Stars
Bellringer
List ways that stars differ from one another.
How is the sun like other stars? How is it different?
Write your answers in your Science Journal.

5. Chapter 15 What You Will Learn
Section 1 Stars
What You Will Learn
Stars differ in size, temperature, composition, brightness, and color.
Distances between stars are very large and are measured in light-years.

6. Chapter 15
Section 1 Stars
Color of Stars
The color of a star indicates the star’s temperature.
Red stars are the coolest, and blue stars are the hottest.
If two stars differ in color, you can conclude that they differ in temperature too.

7. Chapter 15 Composition of Stars
Section 1 Stars
Composition of Stars
Astronomers use an instrument called a spectroscope to separate a star’s light into a spectrum (plural, spectra).
A spectrum is the band of colors produced when white light passes through a prism.

8. Composition of Stars, continued
Chapter 15
Section 1 Stars
Composition of Stars, continued
A continuous spectrum shows all of the colors, while an absorption spectrum shows which wavelengths of light are absorbed.
The spectrum of a star is an absorption spectrum because the atmosphere of the star absorbs certain portions of the light produced by the star.

9. Composition of Stars, continued
Chapter 15
Section 1 Stars
Composition of Stars, continued
When a chemical element emits light, only some colors in the spectrum show up. The colors that appear are called emission lines.
Every element has a unique set of emission lines that act like a fingerprint for that element.

10. Composition of Stars, continued
Chapter 15
Section 1 Stars
Composition of Stars, continued
The pattern of lines in a star’s absorption spectrum is unique to that star.
A star’s absorption spectrum can be used to determine the elements in that star’s atmosphere and the stage the star occupies in its life cycle.
Stars are made of mostly hydrogen and helium gases.

11. Composition of Stars, continued
Chapter 15
Stars, Galaxies, and the Universe
Composition of Stars, continued

12. Chapter 15 Classifying Stars
Section 1 Stars
Classifying Stars
Stars are now classified by how hot they are.
Temperature differences between stars result in color differences that can be seen. For example, class O stars are blue—the hottest stars.

13. Classifying Stars, continued
Chapter 15
Section 1 Stars
Classifying Stars, continued
Magnitude is used to compare the brightness of one object with the brightness of another object.
To express the brightness of stars, astronomers use a system of magnitudes.

14. Classifying Stars, continued
Chapter 15
Section 1 Stars
Classifying Stars, continued
Positive magnitude numbers represent dim stars. Negative magnitude numbers represent bright stars.
The brightest star in the night sky, Sirius, has a magnitude of -1.4.

15. Chapter 15
Stars, Galaxies, and the Universe
Classifying Stars

16. Chapter 15 How Bright Is That Star?
Section 1 Stars
How Bright Is That Star?
The apparent magnitude is the brightness of a star as seen from Earth. The absolute magnitude is the brightness that a star would have at a distance of 32.6 light-years from Earth.
If all stars were the same distance away, their absolute magnitudes would be the same as their apparent magnitudes.

17. Absolute and Apparent Magnitude
Chapter 15
Stars, Galaxies, and the Universe
Absolute and Apparent Magnitude

18. Chapter 15 Distance to the Stars
Section 1 Stars
Distance to the Stars
Because stars are so far away, astronomers use a unit called a light-year to measure the distance from Earth to the stars.
A light-year is the distance that light travels in one year, about 9.46 trillion kilometers.

19. Distance to the Stars, continued
Chapter 15
Section 1 Stars
Distance to the Stars, continued
Parallax is an apparent shift in the position of an object when viewed from different locations.
Astronomers use parallax and trigonometry to find the actual distance to stars that are close to Earth.

20. Chapter 15 Motions of Stars
Section 1 Stars
Motions of Stars
All of the stars in the sky appear to make one complete circle around Polaris every 24 h.
This apparent motion of the stars is due to Earth’s rotation and its revolution around the sun.
Each star is actually moving in space. But because stars are so distant, their actual motion is hard to see.

21. Chapter 15
Stars, Galaxies, and the Universe

22. Chapter 15 Bellringer List 3 stages in the life cycle of an insect.
Section 2 The Life Cycle of Stars
Bellringer
List 3 stages in the life cycle of an insect.
List 3 stages in the life cycle of a human.
List any stages you may know of in the life cycle of a star.
Write your answers in your Science Journal.

23. Chapter 15 What You Will Learn
Section 2 The Life Cycle of Stars
What You Will Learn
During star formation, gravity pulls dust and gas into a sphere, and when the sphere gets dense enough, nuclear fusion begins.
The stages of a star’s life cycle and the star’s properties at each stage can be plotted on the H-R diagram.

24. Chapter 15
Section 2 The Life Cycle of Stars
Types of Stars
Stars can be classified by mass, size, brightness, color, temperature, composition, and age.
A star is classified differently as its properties change. Its properties often relate to whether the star can generate energy by nuclear fusion.

25. The Life Cycle of Sunlike Stars
Chapter 15
Section 2 The Life Cycle of Stars
The Life Cycle of Sunlike Stars
New stars form from gas and dust, which are pulled into a sphere by gravity.
As the sphere becomes denser, hydrogen combines into helium and energy is released in a process called nuclear fusion.

26. The Life Cycle of Sunlike Stars, continued
Chapter 15
Section 2 The Life Cycle of Stars
The Life Cycle of Sunlike Stars, continued
After a sunlike star forms, it enters the main sequence stage, the longest stage of its life cycle. The main sequence is the location on the H-R diagram where most stars lie.
During the main sequence stage, energy is generated in the core of the star from nuclear fusion.

27. The Life Cycle of Sunlike Stars, continued
Chapter 15
Section 2 The Life Cycle of Stars
The Life Cycle of Sunlike Stars, continued
When a main-sequence star uses all of the hydrogen in its core, the atmosphere of the star grows very large and cools. The star may become a red giant or red supergiant.
In the final stage of its life cycle, a sunlike star becomes a white dwarf. A white dwarf no longer generates energy by nuclear fusion.

28. A Tool for Studying Stars
Chapter 15
Section 2 The Life Cycle of Stars
A Tool for Studying Stars
The H-R diagram is a tool for studying the life cycles of stars. The H-R diagram is a graph that shows the relationship between the star’s surface temperature and absolute magnitude.
The stages of a star’s life cycle and its properties at each stage can be plotted on an H-R diagram.

29. Chapter 15
Stars, Galaxies, and the Universe

30. Chapter 15
Stars, Galaxies, and the Universe

31. Chapter 15
Stars, Galaxies, and the Universe
H-R Diagram

32. The Aging of Massive Stars
Chapter 15
Section 2 The Life Cycle of Stars
The Aging of Massive Stars
Massive stars use their hydrogen very fast and tend to have shorter lives than other stars do.
A supernova is a gigantic explosion in which a massive star collapses and throws its outer layers into space.

33. The Aging of Massive Stars, continued
Chapter 15
Section 2 The Life Cycle of Stars
The Aging of Massive Stars, continued
Following a supernova, the center of the collapsed star may contract into a very small dense ball of neutrons called a neutron star.
If a neutron star is spinning, it is called a pulsar. Pulsars send out beams of radiation that sweep across space.

34. The Aging of Massive Stars, continued
Chapter 15
Section 2 The Life Cycle of Stars
The Aging of Massive Stars, continued
If the center of a collapsed massive star has a mass that is several times the mass of the sun, the star may contract further and leave a black hole.
A black hole is an object that is so dense and massive that light cannot escape its gravity.

35. Chapter 15 Bellringer What do you think galaxies are made of?
Section 3 Galaxies
Bellringer
What do you think galaxies are made of?
What is the name of the galaxy in which we live?
Draw a sketch of what you think a spiral galaxy looks like when viewed from outside that galaxy.
Record your answers in your Science Journal.

36. Chapter 15 What You Will Learn
Section 3 Galaxies
What You Will Learn
The three types of galaxies are spiral galaxies, elliptical galaxies, and irregular galaxies.
Galaxies are composed of stars, planetary systems, nebulas, and star clusters.
Looking at distant galaxies reveals what young galaxies looked like.

37. Chapter 15 Types of Galaxies
Section 3 Galaxies
Types of Galaxies
A galaxy is a collection of stars, dust, and gas bound together by gravity.
Astronomers classify a galaxy as spiral, elliptical, or irregular according to its shape and rate of star formation.

38. Types of Galaxies, continued
Chapter 15
Section 3 Galaxies
Types of Galaxies, continued
Spiral galaxies have a bulge at the center and spiral arms.
The spiral arms are made of gas, dust, and new stars that have formed.
The galaxy in which we live is a spiral galaxy called the Milky Way.

39. Types of Galaxies, continued
Chapter 15
Section 3 Galaxies
Types of Galaxies, continued
Most elliptical galaxies are round or oval and seem to have stopped making new stars.
Elliptical galaxies are among the largest galaxies in the universe.
Irregular galaxies have no definite shape and form new stars slowly.

40. Chapter 15 Contents of Galaxies
Section 3 Galaxies
Contents of Galaxies
Some galaxies contain nebulas and star clusters.
A nebula is a large cloud of gas and dust in interstellar space.
Nebulas are a region in space where stars are born.

41. Contents of Galaxies, continued
Chapter 15
Section 3 Galaxies
Contents of Galaxies, continued
A globular cluster is a highly concentrated group of up to 1 million stars that looks like a ball.
Open clusters are groups of 100 to 1,000 stars that are close together relative to other stars.

42. Chapter 15
Stars, Galaxies, and the Universe
Contents of Galaxies

43. Chapter 15
Section 3 Galaxies
Quasars
Quasars are among the most distant objects in the universe and are located in the centers of galaxies.
Quasars generate energy at a high rate and are among the most powerful energy sources in the universe.

44. Chapter 15 Origin of Galaxies
Section 3 Galaxies
Origin of Galaxies
Because light takes time to travel through space, looking through a telescope is like looking back in time.
Looking at distant galaxies reveals what early galaxies looked like.

45. Section 4 Formation of the Universe
Chapter 15
Bellringer
Write a paragraph that describes how you think the universe formed.
Write your answers in your Science Journal.

46. Chapter 15 What You Will Learn
Section 4 Formation of the Universe
Chapter 15
What You Will Learn
The big bang theory is the standard theory to explain the formation of the universe.
Gravity controls the size and shape of the universe.

47. Chapter 15 The Big Bang Theory
Section 4 Formation of the Universe
Chapter 15
The Big Bang Theory
Cosmology is the study of the origin, structure, processes, and evolution of the universe.
Careful measurements have shown that most galaxies are moving away from each other and that the universe is expanding. With these findings, scientists have worked backward in time to figure out how the universe formed.

48. The Big Bang Theory, continued
Section 4 Formation of the Universe
Chapter 15
The Big Bang Theory, continued
The big bang theory is the theory that all matter and energy in the universe was compressed into an extremely small volume that about 14 billion years ago exploded and began expanding in all directions.
Scientists believe that radio “noise” coming from all directions in space is cosmic background radiation left over from the big bang.

49. Chapter 15
Stars, Galaxies, and the Universe

50. Gravity and the Universe
Section 4 Formation of the Universe
Chapter 15
Gravity and the Universe
After the big bang, gravitational attraction caused the matter distributed throughout the universe to form galaxies.
Because gravity acts over such great distances, gravity controls the size and shape of the universe.
Every object in the universe is part of a larger system and gravity acts within each system.

51. Structure of the Universe
Chapter 15
Stars, Galaxies, and the Universe
Structure of the Universe

52. Chapter 15 How Old Is the Universe?
Section 4 Formation of the Universe
Chapter 15
How Old Is the Universe?
Scientists use white dwarfs to estimate the age of the universe. The oldest white dwarfs are 12 billion to 13 billion years old.
It took about 1 billion years after the big bang for the first white dwarf to form. So, the universe must be about 14 billion years old.

53. A Forever-Expanding Universe?
Section 4 Formation of the Universe
Chapter 15
A Forever-Expanding Universe?
The universe is composed of matter, dark matter, and dark energy.
Dark matter does not give off light but has gravity and can be detected. Dark energy seems to be accelerating the expansion of the universe.
Scientists think that the universe may keep growing and expanding forever.

54. Chapter 15
Stars, Galaxies, and the Universe
Concept Map
Use the terms below to complete the concept map on the next slide.
spectra
absolute magnitude
brightness
color
temperature
spectroscope
stars
emission lines

55. Chapter 15
Stars, Galaxies, and the Universe
Concept Map

56. Chapter 15
Stars, Galaxies, and the Universe
Concept Map

57. Chapter 15 End of Chapter 15 Show
Stars, Galaxies, and the Universe
End of Chapter 15 Show

58. Chapter 15
Standards Assessment
1. Which of the following words means “a whole that is built or put together from parts”?
A. structure
B. identity
C. concept
D. cycle

59. Chapter 15
Standards Assessment
1. Which of the following words means “a whole that is built or put together from parts”?
A. structure
B. identity
C. concept
D. cycle

60. Chapter 15
Standards Assessment
2. Choose the appropriate form of the word maintain for the following sentence: “She _____ a B average at school, even while she was in the play.”
A. maintaining
B. maintains
C. maintained
D. maintenance

61. Chapter 15
Standards Assessment
2. Choose the appropriate form of the word maintain for the following sentence: “She _____ a B average at school, even while she was in the play.”
A. maintaining
B. maintains
C. maintained
D. maintenance

62. Chapter 15
Standards Assessment
3. In the sentence “Scientists study the universe by studying the evolution of stars,” what does the word evolution mean?
A. the pattern of change and growth
B. the process by which species develop
C. the way characteristics are passed along
D. the advancement of life in space

63. Chapter 15
Standards Assessment
3. In the sentence “Scientists study the universe by studying the evolution of stars,” what does the word evolution mean?
A. the pattern of change and growth
B. the process by which species develop
C. the way characteristics are passed along
D. the advancement of life in space

64. Chapter 15
Standards Assessment
4. Which of the following words is the closest in meaning to the word role?
A. spin
B. personality
C. tumble
D. function

65. Chapter 15
Standards Assessment
4. Which of the following words is the closest in meaning to the word role?
A. spin
B. personality
C. tumble
D. function

66. Chapter 15
Standards Assessment
5. What is the unit that astronomers use to measure the distances between Earth and stars called?
A. apparent magnitude
B. absolute magnitude
C. light-year
D. parallax

67. Chapter 15
Standards Assessment
5. What is the unit that astronomers use to measure the distances between Earth and stars called?
A. apparent magnitude
B. absolute magnitude
C. light-year
D. parallax

68. Chapter 15
Standards Assessment
6. Which of the following stars has the coolest temperature?
A. a blue-white star
B. a yellow star
C. a yellow-white star
D. an orange star

69. Chapter 15
Standards Assessment
6. Which of the following stars has the coolest temperature?
A. a blue-white star
B. a yellow star
C. a yellow-white star
D. an orange star

70. Chapter 15
Standards Assessment
7. What do scientists learn by studying the pattern of lines in a star’s absorption spectrum?
A. the brightness of the star
B. the elements of the star
C. the distance of the star from Earth
D. the size of the star

71. Chapter 15
Standards Assessment
7. What do scientists learn by studying the pattern of lines in a star’s absorption spectrum?
A. the brightness of the star
B. the elements of the star
C. the distance of the star from Earth
D. the size of the star

72. Chapter 15 8. The picture below shows an example of
Standards Assessment
8. The picture below shows an example of
A. an elliptical galaxy.
B. an irregular galaxy.
C. a supernova.
D. a spiral galaxy.

73. Chapter 15 8. The picture below shows an example of
Standards Assessment
8. The picture below shows an example of
A. an elliptical galaxy.
B. an irregular galaxy.
C. a supernova.
D. a spiral galaxy.

74. Chapter 15 Use the diagram below to answer the next question.
Standards Assessment
Use the diagram below to answer the next question.

75. Chapter 15 9. Which statement about the H-R diagram above is true?
Standards Assessment
9. Which statement about the H-R diagram above is true?
A. Alpha Centauri is hotter and brighter than the sun.
B. Sadr is cooler but brighter than the star Pollux.
C. Pollux is the hottest star shown in the graph.
D. Sadr is the hottest star shown in the graph.

76. Chapter 15 9. Which statement about the H-R diagram above is true?
Standards Assessment
9. Which statement about the H-R diagram above is true?
A. Alpha Centauri is hotter and brighter than the sun.
B. Sadr is cooler but brighter than the star Pollux.
C. Pollux is the hottest star shown in the graph.
D. Sadr is the hottest star shown in the graph.

77. Chapter 15
Standards Assessment
10. The universe contains galaxies, stars, and planets. How does gravity affect these bodies in space?
A. Gravity pulls bodies away from each other.
B. Gravity organizes bodies into nebulas, galaxies, and planetary systems.
C. Gravity attracts bodies with similar compositions to each other.
D. Gravity causes bodies to be scattered randomly throughout the universe

78. Chapter 15
Standards Assessment
10. The universe contains galaxies, stars, and planets. How does gravity affect these bodies in space?
A. Gravity pulls bodies away from each other.
B. Gravity organizes bodies into nebulas, galaxies, and planetary systems.
C. Gravity attracts bodies with similar compositions to each other.
D. Gravity causes bodies to be scattered randomly throughout the universe.

79. Chapter 15
Standards Assessment
11. Which of the following particles is always found in the nucleus of an atom?
A. protons
B. neutrons
C. electrons
D. positrons

80. Chapter 15
Standards Assessment
11. Which of the following particles is always found in the nucleus of an atom?
A. protons
B. neutrons
C. electrons
D. positrons

81. Chapter 15 12. Which group in the periodic table contains helium?
Standards Assessment
12. Which group in the periodic table contains helium?
A. Group 18, the noble gases
B. Group 13, the boron group
C. Group 15, the nitrogen group
D. Group 1, the alkali metals

82. Chapter 15 12. Which group in the periodic table contains helium?
Standards Assessment
12. Which group in the periodic table contains helium?
A. Group 18, the noble gases
B. Group 13, the boron group
C. Group 15, the nitrogen group
D. Group 1, the alkali metals

83. Chapter 15 13. How do geologists measure the precise age of Earth?
Standards Assessment
13. How do geologists measure the precise age of Earth?
A. by measuring the erosion of land formations
B. by analyzing the fossil record
C. by measuring the temperature of Earth’s mantle
D. by measuring the radioactive decay of natural elements

84. Chapter 15 13. How do geologists measure the precise age of Earth?
Standards Assessment
13. How do geologists measure the precise age of Earth?
A. by measuring the erosion of land formations
B. by analyzing the fossil record
C. by measuring the temperature of Earth’s mantle
D. by measuring the radioactive decay of natural elements

85. Chapter 15
Standards Assessment
14. Cyanobacteria were some of the first organisms to appear on Earth. What is the most significant way in which these bacteria affected life on Earth?
A. They were a predator that preyed on organisms that threatened to cause the extinction of other species.
B. They released oxygen through photosynthesis, which led to the formation of the ozone layer.
C. They were a primary food source for producers.
D. They floated on water, shielding other organisms from the sun’s radiation.

86. Chapter 15
Standards Assessment
14. Cyanobacteria were some of the first organisms to appear on Earth. What is the most significant way in which these bacteria affected life on Earth?
A. They were a predator that preyed on organisms that threatened to cause the extinction of other species.
B. They released oxygen through photosynthesis, which led to the formation of the ozone layer.
C. They were a primary food source for producers.
D. They floated on water, shielding other organisms from the sun’s radiation.

87. Chapter 15
Stars, Galaxies, and the Universe