CHAPTER 26 Study Guide

26.1 The Sun

Key Concepts

  • The sun's energy is produced in its core by fusion.

  • The sun remains stable because the inward pull of gravity balances the outward pressure from fusion.

  • The sun's interior consists of the core, radiation zone, and convection zone. Layers of the sun's atmosphere are the photosphere, chromosphere, and corona.

  • Features of the sun's atmosphere include sunspots, prominences, and solar flares.

Vocabulary

core, p. 830; radiation zone, p. 830; convection zone, p. 831; photosphere, p. 831; chromosphere, p. 831; corona, p. 831; solar wind, p. 831; sunspots, p. 832; prominences, p. 833; solar flare, p. 833

26.2 Stars

Key Concepts

  • Astronomers measure the parallax of nearby stars to determine their distance from Earth.

  • Astronomers use several properties to classify stars.

  • Most stars have a composition similar to the sun.

  • H-R diagrams are used to estimate the sizes and distances of stars and to infer how stars change.

Vocabulary

star, p. 834; light-year, p. 834; parallax, p. 835; apparent brightness, p. 836; absolute brightness, p. 837; absorption lines, p. 837; H-R diagram, p. 838; main sequence, p. 839; supergiants, p. 839; giants, p. 839; white dwarf, p. 839

26.3 Life Cycles of Stars

Key Concepts

  • A star is formed when nuclear fusion begins.

  • A star's mass determines the star's place on the main sequence and how long it will stay there.

  • A star ends up as a white dwarf, neutron star, or black hole once it exhausts its fuel supply.

Vocabulary

nebula, p. 840; protostar, p. 841; planetary nebula, p. 842; supernova, p. 843; neutron star, p. 844; pulsar, p. 844; black hole, p. 844

26.4 Groups of Stars

Key Concepts

  • • Astronomers have determined that more than half of all stars are members of star systems.

  • • There are three basic kinds of star clusters: open clusters, associations, and globular clusters.

  • • Astronomers classify galaxies into four main types: spiral, barred-spiral, elliptical, and irregular.

Vocabulary

constellation, p. 846; star system, p. 847; binary star, p. 847; globular cluster, p. 847; galaxy, p. 848; spiral galaxies, p. 848; barred-spiral galaxies, p. 848; elliptical galaxies, p. 848; irregular galaxies, p. 848; quasars, p. 849

26.5 The Expanding Universe

Key Concepts

  • The observed red shift in the spectra of galaxies shows that the universe is expanding.

  • Astronomers theorize that the universe came into being in an event called the big bang.

  • Dark matter can only be detected by observing its gravitational effects on visible matter.

Vocabulary

red shift, p. 852; Hubble's Law, p. 853; big bang theory, p. 854; dark matter, p. 855

Thinking Visually

Comparing and Contrasting Use information from the chapter to complete the table below.

Property

Sun

Supergiant

Lifetime on main sequence

a.

A few million years

Current location on H-R diagram

b.

c.

Next stage in evolution

Red giant

d.

Final stage in evolution

e.

Neutron star or black hole


End ofPage 862

Table of Contents

Physical Science CHAPTER 1 Science Skills CHAPTER 2 Properties of Matter CHAPTER 3 States of Matter CHAPTER 4 Atomic Structure CHAPTER 5 The Periodic Table CHAPTER 6 Chemical Bonds CHAPTER 7 Chemical Reactions CHAPTER 8 Solutions, Acids, and Bases CHAPTER 9 Carbon Chemistry CHAPTER 10 Nuclear Chemistry CHAPTER 11 Motion CHAPTER 12 Forces and Motion CHAPTER 13 Forces in Fluids CHAPTER 14 Work, Power, and Machines CHAPTER 15 Energy CHAPTER 16 Thermal Energy and Heat CHAPTER 17 Mechanical Waves and Sound CHAPTER 18 The Electromagnetic Spectrum and Light CHAPTER 19 Optics CHAPTER 20 Electricity CHAPTER 21 Magnetism CHAPTER 22 Earth's Interior CHAPTER 23 Earth's Surface CHAPTER 24 Weather and Climate CHAPTER 25 The Solar System CHAPTER 26 Exploring the Universe Skills and Reference Handbook