18: Stellar Birth and Evolution
- Page ID
- 115110
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)- 18.1: The Birth of Stars and the Discovery of Planets outside the Solar System
- Do planets orbit other stars or is ours the only planetary system? In the past few decades, new technology has enabled us to answer that question by revealing nearly 3500 exoplanets in over 2600 planetary systems. Even before planets were detected, astronomers had predicted that planetary systems were likely to be byproducts of the star-formation process. In this chapter, we look at how interstellar matter is transformed into stars and planets.
- 18.1.1: Thinking Ahead
- 18.1.2: Star Formation
- 18.1.3: The H-R and the Study of Stellar Evolution
- 18.1.4: Evidence That Planets Form around Other Stars
- 18.1.5: Planets beyond the Solar System- Search and Discovery
- 18.1.6: Exoplanets Everywhere - What we are Learning
- 18.1.7: New Perspectives on Planet Formation
- 18.1.8: Key Terms
- 18.1.9: Summary
- 18.1.10: For Further Exploration
- 18.1.11: Collaborative Group Activities
- 18.1.12: Exercises
- 18.1.12.1: Review Questions
- 18.1.12.2: Thought Questions
- 18.1.12.3: Figuring for Yourself
- 18.2: Stars from Adolescence to Old Age
- The Sun and other stars cannot last forever. Eventually they will exhaust their nuclear fuel and cease to shine. But how do they change during their long lifetimes? And what do these changes mean for the future of Earth? We now turn from the birth of stars to the rest of their life stories. This is not an easy task since stars live much longer than astronomers. Thus, we cannot hope to see the life story of any single star unfold before our eyes or telescopes.
- 18.2.1: Thinking Ahead
- 18.2.2: Evolution from the Main Sequence to Red Giants
- 18.2.3: Star Clusters
- 18.2.4: Checking Out the Theory
- 18.2.5: Further Evolution of Stars
- 18.2.6: The Evolution of More Massive Stars
- 18.2.7: Key Terms
- 18.2.8: Summary
- 18.2.9: For Further Exploration
- 18.2.10: Collaborative Group Activities
- 18.2.11: Exercises
- 18.2.11.1: Review Questions
- 18.2.11.2: Thought Questions
- 18.2.11.3: Figuring for Yourself
- 18.3: The Death of Stars
- Do stars die with a bang or a whimper? In the preceding two chapters, we followed the life story of stars, from the process of birth to the brink of death. Now we are ready to explore the ways that stars end their lives. Sooner or later, each star exhausts its store of nuclear energy. Without a source of internal pressure to balance the weight of the overlying layers, every star eventually gives way to the inexorable pull of gravity and collapses under its own weight.
- 18.3.1: Thinking Ahead
- 18.3.2: The Death of Low-Mass Stars
- 18.3.3: Evolution of Massive Stars- An Explosive Finish
- 18.3.4: Supernova Observations
- 18.3.5: Pulsars and the Discovery of Neutron Stars
- 18.3.6: The Evolution of Binary Star Systems
- 18.3.7: The Mystery of the Gamma-Ray Bursts
- 18.3.8: Key Terms
- 18.3.9: Summary
- 18.3.10: For Further Exploration
- 18.3.11: Collaborative Group Activities
- 18.3.12: Exercises
- 18.3.12.1: Review Questions
- 18.3.12.2: Thought Questions
- 18.3.12.3: Figuring for Yourself
- 18.4: Black Holes and Curved Spacetime
- For most of the twentieth century, black holes seemed the stuff of science fiction, portrayed either as monster vacuum cleaners consuming all the matter around them or as tunnels from one universe to another. But the truth about black holes is almost stranger than fiction. As we continue our voyage into the universe, we will discover that black holes are the key to explaining many mysterious and remarkable objects—including collapsed stars.
- 18.4.1: Thinking Ahead
- 18.4.2: Introducing General Relativity
- 18.4.3: Spacetime and Gravity
- 18.4.4: Tests of General Relativity
- 18.4.5: Time in General Relativity
- 18.4.6: Black Holes
- 18.4.7: Evidence for Black Holes
- 18.4.8: Gravitational Wave Astronomy
- 18.4.9: Key Terms
- 18.4.10: Summary
- 18.4.11: For Further Exploration
- 18.4.12: Collaborative Group Activities
- 18.4.13: Exercises
- 18.4.13.1: Review Questions
- 18.4.13.2: Thought Questions
- 18.4.13.3: Figuring for Yourself

