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          <TitleText>On the Edge of the Cosmos</TitleText>
          <Subtitle>A Century of Revolution in Astronomy</Subtitle>
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        <PersonName>Alain Omont</PersonName>
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        <BiographicalNote>&lt;p&gt;Alain Omont se trouve au coeur de cette aventure au sein de nombreuses collaborations internationales autour des grands instruments de l’astronomie au sol et dans l’espace. Il a été le premier directeur de l’Observatoire de Grenoble, puis directeur de l’Institut d’Astrophysique de Paris (Sorbonne Université-CNRS) où il est aujourd’hui Directeur de recherche émérite CNRS.&lt;/p&gt;</BiographicalNote>
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        <Text language="fre">&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;In a world where intergalactic wars are a common topic for movies, it is hard to imagine that the discovery of galaxies was made less than a century ago. In fact, it was one of the key astrophysical milestones of the first half of the 20th century, along with the revelation of the expansion of the Universe and the understanding of the source of the stars’ energy.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The second half of last century saw &lt;/span&gt;&lt;span style="color: rgb(0, 0, 0); font-family: MilibusLt-Regular; font-size: 18.6667px; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; font-weight: 400; letter-spacing: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial; display: inline !important; float: none;"&gt;the un&lt;/span&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;expected discovery of fantastic objects and extreme events in the Universe including neutron stars, black holes, radio galaxies, quasars, exoplanets, or stellar explosions. Modern cosmology was simultaneously established with the Big Bang model, leading to an astonishingly precise determination of the parameters of the Universe.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The author here retraces the adventure of twentieth-century astronomy and describes how it has changed our vision of the cosmos. By assessing the major successes of this undertaking and highlighting the fundamental questions that still remain, he puts into perspective the recent progress at the dawn of the new millennium including the acceleration of the expansion of the Universe and dark energy, dark matter, exoplanets, black hole mergers and gravitational waves, to name only the most spectacular discoveries. This book thus offers, in a concise and accessible form, a synthesis of our current knowledge of astrophysics, including many beautiful images from leading observatories.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;</Text>
        <Text language="eng">&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;In a world where intergalactic wars are a common topic for movies, it is hard to imagine that the discovery of galaxies was made less than a century ago. In fact, it was one of the key astrophysical milestones of the first half of the 20th century, along with the revelation of the expansion of the Universe and the understanding of the source of the stars’ energy.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The second half of last century saw the unexpected discovery of fantastic objects and extreme events in the Universe including neutron stars, black holes, radio galaxies, quasars, exoplanets, or stellar explosions.Modern cosmology was simultaneously established with the Big Bang model, leading to an astonishingly precise determination of the parameters of the Universe.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The author here retraces the adventure of twentieth-century astronomy and describes how it has changed our vision of the cosmos. By assessing the major successes of this undertaking and highlighting the fundamental questions that still remain, he puts into perspective the recent progress at the dawn of the new millennium including the acceleration of the expansion of the Universe and dark energy, dark matter, exoplanets, black hole mergers and gravitational waves, to name only the most spectacular discoveries. This book thus offers, in a concise and accessible form, a synthesis of our current knowledge of astrophysics, including many beautiful images from leading observatories.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;</Text>
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        <Text language="fre">&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The author here retraces the adventure of twentieth-century astronomy and describes how it has changed our vision of the cosmos.This book thus offers, in a concise and accessible form, a synthesis of our current knowledge of astrophysics, including many beautiful images from leading observatories.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;&amp;nbsp;&lt;/span&gt;&lt;/p&gt;</Text>
        <Text language="eng">&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The author here retraces the adventure of twentieth-century astronomy and describes how it has changed our vision of the cosmos. This book thus offers, in a concise and accessible form, a synthesis of our current knowledge of astrophysics, including many beautiful images from leading observatories.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;&amp;nbsp;&lt;/span&gt;&lt;/p&gt;</Text>
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        <Text language="fre">&lt;p&gt;Contents&lt;/p&gt;&lt;p&gt;General Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . III&lt;/p&gt;&lt;p&gt;Acknowledgments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . VII&lt;/p&gt;&lt;p&gt;Part I A Century of Revolution in Our Vision of the Universe . . . . . . . . . . 1&lt;/p&gt;&lt;p&gt;CHAPTER 1 &lt;/p&gt;&lt;p&gt;General View of 20th Century Astronomy and Its Starting Point . . . . . . . . . 3&lt;/p&gt;&lt;p&gt;1.1 Astronomy, the Key to Our Vision of the World . . . . . . . . . . . . . . . . . 3&lt;/p&gt;&lt;p&gt;1.2 Benchmarks on 1900 Astronomy and Its Shortcomings . . . . . . . . . . . . 7&lt;/p&gt;&lt;p&gt;CHAPTER 2&lt;/p&gt;&lt;p&gt;Scientific and Technical Revolutions, Drivers of 20th Century Astronomy . . . 21&lt;/p&gt;&lt;p&gt;2.1 Physics Revolutions, Keys to Astrophysics . . . . . . . . . . . . . . . . . . . . . 21&lt;/p&gt;&lt;p&gt;2.2 Giant Telescopes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22&lt;/p&gt;&lt;p&gt;2.3 Overcoming the Disturbances of the Earth Atmosphere. . . . . . . . . . . . 24&lt;/p&gt;&lt;p&gt;2.4 Exploiting All Spectral Domains from Radio to X-ray and Gamma-ray . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29&lt;/p&gt;&lt;p&gt;2.5 Visiting the Planets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35&lt;/p&gt;&lt;p&gt;2.6 No Pause in the Progress of Signal Detection and Exploitation . . . . . . 35&lt;/p&gt;&lt;p&gt;Part II Stars are Well Understood . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39&lt;/p&gt;&lt;p&gt;CHAPTER 3&lt;/p&gt;&lt;p&gt;How does a Star Work? . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41&lt;/p&gt;&lt;p&gt;3.1 Understanding the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41&lt;/p&gt;&lt;p&gt;3.2 Solving the Mystery of the Origin of the Energy of the Sun and the Stars . . . . . . . . . . . . .&amp;nbsp; . . . . . . . . . . . . . . . . . . . . . . 42&lt;/p&gt;&lt;p&gt;3.3 The Life of the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46&lt;/p&gt;&lt;p&gt;3.4 Our Atoms were Born in the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . 51&lt;/p&gt;&lt;p&gt;3.5 Stars also Die . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52&lt;/p&gt;&lt;p&gt;CHAPTER 4&lt;/p&gt;&lt;p&gt;Complexities of Star Birth and Physics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57&lt;/p&gt;&lt;p&gt;4.1 General Star Formation Scenario . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57&lt;/p&gt;&lt;p&gt;4.2 Young Infrared Stars: Born in Dusty Cocoons . . . . . . . . . . . . . . . . . . . 59&lt;/p&gt;&lt;p&gt;4.3 Gravitational Contraction, Accretion and Discs. . . . . . . . . . . . . . . . . . 59&lt;/p&gt;&lt;p&gt;4.4 Universality of Stellar Pairs – Complex Ending of Their Lives . . . . . . . 61&lt;/p&gt;&lt;p&gt;4.5 Brown Dwarfs, Billions of Aborted Stars . . . . . . . . . . . . . . . . . . . . . . . 63&lt;/p&gt;&lt;p&gt;4.6 Stars are Still at the Forefront of Current Astronomy . . . . . . . . . . . . . 65&lt;/p&gt;&lt;p&gt;4.7 Stars and Ecology of Planets and Galaxies . . . . . . . . . . . . . . . . . . . . . 68&lt;/p&gt;&lt;p&gt;Part III The New World of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 71&lt;/p&gt;&lt;p&gt;CHAPTER 5&lt;/p&gt;&lt;p&gt;Discovery of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73&lt;/p&gt;&lt;p&gt;5.1 The Appreciation of the Nature of Galaxies Dates Back Only to the Beginning of the 20th Century . . . . . . . . . . . . . 73&lt;/p&gt;&lt;p&gt;5.2 First Steps in the World of Nearby Galaxies . . . . . . . . . . . . . . . . . . . . 77&lt;/p&gt;&lt;p&gt;5.3 Architecture and Stellar Content of Galaxies . . . . . . . . . . . . . . . . . . . . 81&lt;/p&gt;&lt;p&gt;CHAPTER 6&lt;/p&gt;&lt;p&gt;Our Galaxy and Its Interstellar Medium . . . . . . . . . . . . . . . . . . . . . . . . . . . . 83&lt;/p&gt;&lt;p&gt;6.1 Exploration of Our Galaxy, the Milky Way . . . . . . . . . . . . . . . . . . . . . 83&lt;/p&gt;&lt;p&gt;6.2 An Ordinary Galaxy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 84&lt;/p&gt;&lt;p&gt;6.3 Current Organization of Stars Resulting from the Milky Way History . 86&lt;/p&gt;&lt;p&gt;6.4 The Interstellar Gas, a Key Player in the Evolution of Galaxies . . . . . 86&lt;/p&gt;&lt;p&gt;6.5 Other Players in the Interstellar Medium . . . . . . . . . . . . . . . . . . . . . . 90&lt;/p&gt;&lt;p&gt;6.6 Exotic Components of the Milky Way . . . . . . . . . . . . . . . . . . . . . . . . . 94&lt;/p&gt;&lt;p&gt;CHAPTER 7&lt;/p&gt;&lt;p&gt;Hundreds of Billions of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97&lt;/p&gt;&lt;p&gt;7.1 Galaxies at All Stages of Their Life . . . . . . . . . . . . . . . . . . . . . . . . . . . 97&lt;/p&gt;&lt;p&gt;7.2 The Turbulent Family Life of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . 99&lt;/p&gt;&lt;p&gt;7.3 Understanding the Formation and Evolution of Galaxies . . . . . . . . . . . 106&lt;/p&gt;&lt;p&gt;Part IV Cosmology, the Science of the Universe as a Whole . . . . . . . . . . . . 109&lt;/p&gt;&lt;p&gt;CHAPTER 8&lt;/p&gt;&lt;p&gt;Birth of Cosmology. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111&lt;/p&gt;&lt;p&gt;8.1 The Universe of Galaxies is Expanding . . . . . . . . . . . . . . . . . . . . . . . . 111&lt;/p&gt;&lt;p&gt;8.2 The Saga of the Big Bang Confirmation . . . . . . . . . . . . . . . . . . . . . . . 114&lt;/p&gt;&lt;p&gt;8.3 The Very First Phase in the History of the Universe: Uncertain Physics . . . . . . . . . . . . . . . . . . . 116&lt;/p&gt;&lt;p&gt;8.4 AWell-Understood Second Phase: The Standard Big Bang Model . . . . 118&lt;/p&gt;&lt;p&gt;CHAPTER 9&lt;/p&gt;&lt;p&gt;Content of the Universe and Structure Formation . . . . . . . . . . . . . . . . . . . . . 123&lt;/p&gt;&lt;p&gt;9.1 Formation of Galaxies and Structures of the Present Universe . . . . . . . 123&lt;/p&gt;&lt;p&gt;9.2 Fundamental Parameters of the Universe are Better Known than Its Physics . . . . . . . . . . . . . . . . . . 125&lt;/p&gt;&lt;p&gt;9.3 Age of the Universe and Variations of the Determinations of the Hubble Constant . . . . . . . . . . . . . . 128&lt;/p&gt;&lt;p&gt;9.4 An Overall Density Very Close to the Critical Density . . . . . . . . . . . . 128&lt;/p&gt;&lt;p&gt;9.5 Need and Nature of Dark Matter . . . . . . . . . . . . . . . . . . . . . . . . . . . . 129&lt;/p&gt;&lt;p&gt;9.6 A Last-Minute Surprise, the Re-Acceleration of the Expansion Involving an Unknown Source of Cosmic Energy . . . . . . . 131&lt;/p&gt;&lt;p&gt;9.7 Summarizing: An Unexpected Universe Model Validated in Multiple Ways . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132&lt;/p&gt;&lt;p&gt;Part V Singular Stars and Cataclysms in Extreme Physical Conditions . . . 135&lt;/p&gt;&lt;p&gt;CHAPTER 10&lt;/p&gt;&lt;p&gt;Explosions of Stars and Their Singular Residues . . . . . . . . . . . . . . . . . . . . . . 137&lt;/p&gt;&lt;p&gt;10.1 Extreme Physics of Supernova Implosion/Explosion . . . . . . . . . . . . . 137&lt;/p&gt;&lt;p&gt;10.2 Neutron Stars, Hyper-Dense Supernova Residues. . . . . . . . . . . . . . . . 145&lt;/p&gt;&lt;p&gt;10.3 Gamma-Ray Bursts, Even More Powerful Bursts . . . . . . . . . . . . . . . . 147&lt;/p&gt;&lt;p&gt;10.4 Cosmic Rays, Messenger Particles of the High Energy Universe . . . . . 149&lt;/p&gt;&lt;p&gt;CHAPTER 11&lt;/p&gt;&lt;p&gt;Black Holes and Their Power . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155&lt;/p&gt;&lt;p&gt;11.1 Black Holes, General Relativity and the Cosmos . . . . . . . . . . . . . . . . 155&lt;/p&gt;&lt;p&gt;11.2 Stellar Black Holes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157&lt;/p&gt;&lt;p&gt;11.3 GravitationalWaves, Propagation of Spacetime-Curvature Disturbances. . . 158&lt;/p&gt;&lt;p&gt;11.4 Quasars: New Stars a Thousand Times Brighter than Galaxies . . . . . 162&lt;/p&gt;&lt;p&gt;11.5 Manifestations of Super-Massive Black Holes and Their Interpretation . . . 164&lt;/p&gt;&lt;p&gt;11.6 Co-evolution of Galaxies and Their Black Hole . . . . . . . . . . . . . . . . . 170&lt;/p&gt;&lt;p&gt;11.7 The Super-Massive Black Hole of Our Galaxy and Others . . . . . . . . . 171&lt;/p&gt;&lt;p&gt;Part VI Planets, in the Solar System and Outside . . . . . . . . . . . . . . . . . . . 173&lt;/p&gt;&lt;p&gt;CHAPTER 12&lt;/p&gt;&lt;p&gt;Direct Exploration of the Planets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 175&lt;/p&gt;&lt;p&gt;12.1 Planets, Stars of Astronomy until the 19th Century . . . . . . . . . . . . . 175&lt;/p&gt;&lt;p&gt;12.2 Half a Century Without Revolution for Planetology . . . . . . . . . . . . . 178&lt;/p&gt;&lt;p&gt;12.3 Humans Went to the Moon! . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180&lt;/p&gt;&lt;p&gt;12.4 We Broadly Understand the Origin of the Moon and Its Importance for the Earth . . . . . . . . .&amp;nbsp; . . . . . . . . . . . . 181&lt;/p&gt;&lt;p&gt;12.5 Very Rich Close-up Photos of All the Bodies of the Solar System . . . 183&lt;/p&gt;&lt;p&gt;12.6 Summary of Planetary Expeditions . . . . . . . . . . . . . . . . . . . . . . . . . . 184&lt;/p&gt;&lt;p&gt;12.7 Searching for Life in the Solar System: Where and When? . . . . . . . . . 191&lt;/p&gt;&lt;p&gt;CHAPTER 13&lt;/p&gt;&lt;p&gt;Entering the Dream World of Exoplanets . . . . . . . . . . . . . . . . . . . . . . . . . . . 197&lt;/p&gt;&lt;p&gt;13.1 Explosion of Discoveries of New Planets . . . . . . . . . . . . . . . . . . . . . . 197&lt;/p&gt;&lt;p&gt;13.2 The Majority of Stars have a Planetary System. . . . . . . . . . . . . . . . . 201&lt;/p&gt;&lt;p&gt;13.3 Surprising Variety of Exoplanets . . . . . . . . . . . . . . . . . . . . . . . . . . . . 202&lt;/p&gt;&lt;p&gt;13.4 The Search for Earth-Like Planets. . . . . . . . . . . . . . . . . . . . . . . . . . . 204&lt;/p&gt;&lt;p&gt;Conclusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 209&lt;/p&gt;&lt;p&gt;CHAPTER 14&lt;/p&gt;&lt;p&gt;A New Cosmos in the 21st Century?. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211&lt;/p&gt;&lt;p&gt;14.1 A New Cosmos . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211&lt;/p&gt;&lt;p&gt;14.2 Auguries for 21st Century Astronomy? . . . . . . . . . . . . . . . . . . . . . . . 212&lt;/p&gt;&lt;p&gt;Glossary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 217&lt;/p&gt;&lt;p&gt;Acronyms and Space Missions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 223&lt;/p&gt;&lt;p&gt;References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 227&lt;/p&gt;&lt;p&gt;Index . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 231&lt;/p&gt;&lt;p&gt;The asterisks * indicate words or acronyms whose meaning is explained in the&lt;/p&gt;&lt;p&gt;“Glossary” or “Acronyms and space missions” sections at the end of the book.&lt;/p&gt;</Text>
        <Text language="eng">&lt;p&gt;Contents&lt;/p&gt;&lt;p&gt;General Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . III&lt;/p&gt;&lt;p&gt;Acknowledgments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . VII&lt;/p&gt;&lt;p&gt;Part I A Century of Revolution in Our Vision of the Universe . . . . . . . . . . 1&lt;/p&gt;&lt;p&gt;CHAPTER 1&lt;/p&gt;&lt;p&gt;General View of 20th Century Astronomy and Its Starting Point . . . . . . . . . 3&lt;/p&gt;&lt;p&gt;1.1 Astronomy, the Key to Our Vision of the World . . . . . . . . . . . . . . . . . 3&lt;/p&gt;&lt;p&gt;1.2 Benchmarks on 1900 Astronomy and Its Shortcomings . . . . . . . . . . . . 7&lt;/p&gt;&lt;p&gt;CHAPTER 2&lt;/p&gt;&lt;p&gt;Scientific and Technical Revolutions, Drivers of 20th Century Astronomy . . . 21&lt;/p&gt;&lt;p&gt;2.1 Physics Revolutions, Keys to Astrophysics . . . . . . . . . . . . . . . . . . . . . 21&lt;/p&gt;&lt;p&gt;2.2 Giant Telescopes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22&lt;/p&gt;&lt;p&gt;2.3 Overcoming the Disturbances of the Earth Atmosphere. . . . . . . . . . . . 24&lt;/p&gt;&lt;p&gt;2.4 Exploiting All Spectral Domains from Radio to X-ray and Gamma-ray . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29&lt;/p&gt;&lt;p&gt;2.5 Visiting the Planets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35&lt;/p&gt;&lt;p&gt;2.6 No Pause in the Progress of Signal Detection and Exploitation . . . . . . 35&lt;/p&gt;&lt;p&gt;Part II Stars are Well Understood . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39&lt;/p&gt;&lt;p&gt;CHAPTER 3&lt;/p&gt;&lt;p&gt;How does a Star Work? . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41&lt;/p&gt;&lt;p&gt;3.1 Understanding the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41&lt;/p&gt;&lt;p&gt;3.2 Solving the Mystery of the Origin of the Energy of the Sun and the Stars . . . . . . . . . . . . . . . . . .. . . . . . . . . . . . . . . 42&lt;/p&gt;&lt;p&gt;3.3 The Life of the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46&lt;/p&gt;&lt;p&gt;3.4 Our Atoms were Born in the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . 51&lt;/p&gt;&lt;p&gt;3.5 Stars also Die . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52&lt;/p&gt;&lt;p&gt;CHAPTER 4&lt;/p&gt;&lt;p&gt;Complexities of Star Birth and Physics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57&lt;/p&gt;&lt;p&gt;4.1 General Star Formation Scenario . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57&lt;/p&gt;&lt;p&gt;4.2 Young Infrared Stars: Born in Dusty Cocoons . . . . . . . . . . . . . . . . . . . 59&lt;/p&gt;&lt;p&gt;4.3 Gravitational Contraction, Accretion and Discs. . . . . . . . . . . . . . . . . . 59&lt;/p&gt;&lt;p&gt;4.4 Universality of Stellar Pairs – Complex Ending of Their Lives . . . . . . . 61&lt;/p&gt;&lt;p&gt;4.5 Brown Dwarfs, Billions of Aborted Stars . . . . . . . . . . . . . . . . . . . . . . . 63&lt;/p&gt;&lt;p&gt;4.6 Stars are Still at the Forefront of Current Astronomy . . . . . . . . . . . . . 65&lt;/p&gt;&lt;p&gt;4.7 Stars and Ecology of Planets and Galaxies . . . . . . . . . . . . . . . . . . . . . 68&lt;/p&gt;&lt;p&gt;Part III The New World of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 71&lt;/p&gt;&lt;p&gt;CHAPTER 5&lt;/p&gt;&lt;p&gt;Discovery of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73&lt;/p&gt;&lt;p&gt;5.1 The Appreciation of the Nature of Galaxies Dates Back Only to the Beginning of the 20th Century . . . . . . . . .&amp;nbsp; . . . . . . 73&lt;/p&gt;&lt;p&gt;5.2 First Steps in the World of Nearby Galaxies . . . . . . . . . . . . . . . . . . . . 77&lt;/p&gt;&lt;p&gt;5.3 Architecture and Stellar Content of Galaxies . . . . . . . . . . . . . . . . . . . . 81&lt;/p&gt;&lt;p&gt;CHAPTER 6&lt;/p&gt;&lt;p&gt;Our Galaxy and Its Interstellar Medium . . . . . . . . . . . . . . . . . . . . . . . . . . . . 83&lt;/p&gt;&lt;p&gt;6.1 Exploration of Our Galaxy, the Milky Way . . . . . . . . . . . . . . . . . . . . . 83&lt;/p&gt;&lt;p&gt;6.2 An Ordinary Galaxy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 84&lt;/p&gt;&lt;p&gt;6.3 Current Organization of Stars Resulting from the Milky Way History . 86&lt;/p&gt;&lt;p&gt;6.4 The Interstellar Gas, a Key Player in the Evolution of Galaxies . . . . . 86&lt;/p&gt;&lt;p&gt;6.5 Other Players in the Interstellar Medium . . . . . . . . . . . . . . . . . . . . . . 90&lt;/p&gt;&lt;p&gt;6.6 Exotic Components of the Milky Way . . . . . . . . . . . . . . . . . . . . . . . . . 94&lt;/p&gt;&lt;p&gt;CHAPTER 7&lt;/p&gt;&lt;p&gt;Hundreds of Billions of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97&lt;/p&gt;&lt;p&gt;7.1 Galaxies at All Stages of Their Life . . . . . . . . . . . . . . . . . . . . . . . . . . . 97&lt;/p&gt;&lt;p&gt;7.2 The Turbulent Family Life of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . 99&lt;/p&gt;&lt;p&gt;7.3 Understanding the Formation and Evolution of Galaxies . . . . . . . . . . . 106&lt;/p&gt;&lt;p&gt;Part IV Cosmology, the Science of the Universe as a Whole . . . . . . . . . . . . 109&lt;/p&gt;&lt;p&gt;CHAPTER 8&lt;/p&gt;&lt;p&gt;Birth of Cosmology. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111&lt;/p&gt;&lt;p&gt;8.1 The Universe of Galaxies is Expanding . . . . . . . . . . . . . . . . . . . . . . . . 111&lt;/p&gt;&lt;p&gt;8.2 The Saga of the Big Bang Confirmation . . . . . . . . . . . . . . . . . . . . . . . 114&lt;/p&gt;&lt;p&gt;8.3 The Very First Phase in the History of the Universe: Uncertain Physics . . . . . . . . . . . . . . . . . . . . . 116&lt;/p&gt;&lt;p&gt;8.4 AWell-Understood Second Phase: The Standard Big Bang Model . . . . 118&lt;/p&gt;&lt;p&gt;CHAPTER 9&lt;/p&gt;&lt;p&gt;Content of the Universe and Structure Formation . . . . . . . . . . . . . . . . . . . . . 123&lt;/p&gt;&lt;p&gt;9.1 Formation of Galaxies and Structures of the Present Universe . . . . . . . 123&lt;/p&gt;&lt;p&gt;9.2 Fundamental Parameters of the Universe are Better Known than Its Physics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 125&lt;/p&gt;&lt;p&gt;9.3 Age of the Universe and Variations of the Determinations of the Hubble Constant . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 128&lt;/p&gt;&lt;p&gt;9.4 An Overall Density Very Close to the Critical Density . . . . . . . . . . . . 128&lt;/p&gt;&lt;p&gt;9.5 Need and Nature of Dark Matter . . . . . . . . . . . . . . . . . . . . . . . . . . . . 129&lt;/p&gt;&lt;p&gt;9.6 A Last-Minute Surprise, the Re-Acceleration of the Expansion Involving an Unknown Source of Cosmic Energy . . . . . . . . . . . 131&lt;/p&gt;&lt;p&gt;9.7 Summarizing: An Unexpected Universe Model Validated in Multiple Ways . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132&lt;/p&gt;&lt;p&gt;Part V Singular Stars and Cataclysms in Extreme Physical Conditions . . . 135&lt;/p&gt;&lt;p&gt;CHAPTER 10&lt;/p&gt;&lt;p&gt;Explosions of Stars and Their Singular Residues . . . . . . . . . . . . . . . . . . . . . . 137&lt;/p&gt;&lt;p&gt;10.1 Extreme Physics of Supernova Implosion/Explosion . . . . . . . . . . . . . 137&lt;/p&gt;&lt;p&gt;10.2 Neutron Stars, Hyper-Dense Supernova Residues. . . . . . . . . . . . . . . . 145&lt;/p&gt;&lt;p&gt;10.3 Gamma-Ray Bursts, Even More Powerful Bursts . . . . . . . . . . . . . . . . 147&lt;/p&gt;&lt;p&gt;10.4 Cosmic Rays, Messenger Particles of the High Energy Universe . . . . . 149&lt;/p&gt;&lt;p&gt;CHAPTER 11&lt;/p&gt;&lt;p&gt;Black Holes and Their Power . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155&lt;/p&gt;&lt;p&gt;11.1 Black Holes, General Relativity and the Cosmos . . . . . . . . . . . . . . . . 155&lt;/p&gt;&lt;p&gt;11.2 Stellar Black Holes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157&lt;/p&gt;&lt;p&gt;11.3 GravitationalWaves, Propagation of Spacetime-Curvature Disturbances. . . 158&lt;/p&gt;&lt;p&gt;11.4 Quasars: New Stars a Thousand Times Brighter than Galaxies . . . . . 162&lt;/p&gt;&lt;p&gt;11.5 Manifestations of Super-Massive Black Holes and Their Interpretation . . . 164&lt;/p&gt;&lt;p&gt;11.6 Co-evolution of Galaxies and Their Black Hole . . . . . . . . . . . . . . . . . 170&lt;/p&gt;&lt;p&gt;11.7 The Super-Massive Black Hole of Our Galaxy and Others . . . . . . . . . 171&lt;/p&gt;&lt;p&gt;Part VI Planets, in the Solar System and Outside . . . . . . . . . . . . . . . . . . . 173&lt;/p&gt;&lt;p&gt;CHAPTER 12&lt;/p&gt;&lt;p&gt;Direct Exploration of the Planets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 175&lt;/p&gt;&lt;p&gt;12.1 Planets, Stars of Astronomy until the 19th Century . . . . . . . . . . . . . 175&lt;/p&gt;&lt;p&gt;12.2 Half a Century Without Revolution for Planetology . . . . . . . . . . . . . 178&lt;/p&gt;&lt;p&gt;12.3 Humans Went to the Moon! . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180&lt;/p&gt;&lt;p&gt;12.4 We Broadly Understand the Origin of the Moon and Its Importance for the Earth . . . . . . . .&amp;nbsp; . . . . . . . . . . . . . . 181&lt;/p&gt;&lt;p&gt;12.5 Very Rich Close-up Photos of All the Bodies of the Solar System . . . 183&lt;/p&gt;&lt;p&gt;12.6 Summary of Planetary Expeditions . . . . . . . . . . . . . . . . . . . . . . . . . . 184&lt;/p&gt;&lt;p&gt;12.7 Searching for Life in the Solar System: Where and When? . . . . . . . . . 191&lt;/p&gt;&lt;p&gt;CHAPTER 13&lt;/p&gt;&lt;p&gt;Entering the Dream World of Exoplanets . . . . . . . . . . . . . . . . . . . . . . . . . . . 197&lt;/p&gt;&lt;p&gt;13.1 Explosion of Discoveries of New Planets . . . . . . . . . . . . . . . . . . . . . . 197&lt;/p&gt;&lt;p&gt;13.2 The Majority of Stars have a Planetary System. . . . . . . . . . . . . . . . . 201&lt;/p&gt;&lt;p&gt;13.3 Surprising Variety of Exoplanets . . . . . . . . . . . . . . . . . . . . . . . . . . . . 202&lt;/p&gt;&lt;p&gt;13.4 The Search for Earth-Like Planets. . . . . . . . . . . . . . . . . . . . . . . . . . . 204&lt;/p&gt;&lt;p&gt;Conclusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 209&lt;/p&gt;&lt;p&gt;CHAPTER 14&lt;/p&gt;&lt;p&gt;A New Cosmos in the 21st Century?. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211&lt;/p&gt;&lt;p&gt;14.1 A New Cosmos . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211&lt;/p&gt;&lt;p&gt;14.2 Auguries for 21st Century Astronomy? . . . . . . . . . . . . . . . . . . . . . . . 212&lt;/p&gt;&lt;p&gt;Glossary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 217&lt;/p&gt;&lt;p&gt;Acronyms and Space Missions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 223&lt;/p&gt;&lt;p&gt;References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 227&lt;/p&gt;&lt;p&gt;Index . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 231&lt;/p&gt;&lt;p&gt;The asterisks * indicate words or acronyms whose meaning is explained in the&lt;/p&gt;&lt;p&gt;“Glossary” or “Acronyms and space missions” sections at the end of the book.&lt;/p&gt;</Text>
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        <Text language="fre">&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;In a world where intergalactic wars are a common topic for movies, it is hard to imagine that the discovery of galaxies was made less than a century ago. In fact, it was one of the key astrophysical milestones of the first half of the 20th century, along with the revelation of the expansion of the Universe and the understanding of the source of the stars’ energy.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The second half of last century saw &lt;/span&gt;&lt;span style="color: rgb(0, 0, 0); font-family: MilibusLt-Regular; font-size: 18.6667px; font-style: normal; font-variant-ligatures: normal; font-variant-caps: normal; font-weight: 400; letter-spacing: normal; orphans: 2; text-align: start; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-stroke-width: 0px; background-color: rgb(255, 255, 255); text-decoration-thickness: initial; text-decoration-style: initial; text-decoration-color: initial; display: inline !important; float: none;"&gt;the un&lt;/span&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;expected discovery of fantastic objects and extreme events in the Universe including neutron stars, black holes, radio galaxies, quasars, exoplanets, or stellar explosions. Modern cosmology was simultaneously established with the Big Bang model, leading to an astonishingly precise determination of the parameters of the Universe.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The author here retraces the adventure of twentieth-century astronomy and describes how it has changed our vision of the cosmos. By assessing the major successes of this undertaking and highlighting the fundamental questions that still remain, he puts into perspective the recent progress at the dawn of the new millennium including the acceleration of the expansion of the Universe and dark energy, dark matter, exoplanets, black hole mergers and gravitational waves, to name only the most spectacular discoveries. This book thus offers, in a concise and accessible form, a synthesis of our current knowledge of astrophysics, including many beautiful images from leading observatories.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;</Text>
        <Text language="eng">&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;In a world where intergalactic wars are a common topic for movies, it is hard to imagine that the discovery of galaxies was made less than a century ago. In fact, it was one of the key astrophysical milestones of the first half of the 20th century, along with the revelation of the expansion of the Universe and the understanding of the source of the stars’ energy.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The second half of last century saw the unexpected discovery of fantastic objects and extreme events in the Universe including neutron stars, black holes, radio galaxies, quasars, exoplanets, or stellar explosions.Modern cosmology was simultaneously established with the Big Bang model, leading to an astonishingly precise determination of the parameters of the Universe.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The author here retraces the adventure of twentieth-century astronomy and describes how it has changed our vision of the cosmos. By assessing the major successes of this undertaking and highlighting the fundamental questions that still remain, he puts into perspective the recent progress at the dawn of the new millennium including the acceleration of the expansion of the Universe and dark energy, dark matter, exoplanets, black hole mergers and gravitational waves, to name only the most spectacular discoveries. This book thus offers, in a concise and accessible form, a synthesis of our current knowledge of astrophysics, including many beautiful images from leading observatories.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;</Text>
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        <Text language="eng">&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;The author here retraces the adventure of twentieth-century astronomy and describes how it has changed our vision of the cosmos. This book thus offers, in a concise and accessible form, a synthesis of our current knowledge of astrophysics, including many beautiful images from leading observatories.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="margin-bottom:0cm;line-height:normal;mso-layout-grid-align:none;text-autospace:none"&gt;&lt;span lang="EN-US" style="font-size:14.0pt;font-family:MilibusLt-Regular;mso-bidi-font-family:MilibusLt-Regular;color:black;mso-ansi-language:EN-US"&gt;&amp;nbsp;&lt;/span&gt;&lt;/p&gt;</Text>
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        <Text language="fre">&lt;p&gt;Contents&lt;/p&gt;&lt;p&gt;General Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . III&lt;/p&gt;&lt;p&gt;Acknowledgments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . VII&lt;/p&gt;&lt;p&gt;Part I A Century of Revolution in Our Vision of the Universe . . . . . . . . . . 1&lt;/p&gt;&lt;p&gt;CHAPTER 1 &lt;/p&gt;&lt;p&gt;General View of 20th Century Astronomy and Its Starting Point . . . . . . . . . 3&lt;/p&gt;&lt;p&gt;1.1 Astronomy, the Key to Our Vision of the World . . . . . . . . . . . . . . . . . 3&lt;/p&gt;&lt;p&gt;1.2 Benchmarks on 1900 Astronomy and Its Shortcomings . . . . . . . . . . . . 7&lt;/p&gt;&lt;p&gt;CHAPTER 2&lt;/p&gt;&lt;p&gt;Scientific and Technical Revolutions, Drivers of 20th Century Astronomy . . . 21&lt;/p&gt;&lt;p&gt;2.1 Physics Revolutions, Keys to Astrophysics . . . . . . . . . . . . . . . . . . . . . 21&lt;/p&gt;&lt;p&gt;2.2 Giant Telescopes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22&lt;/p&gt;&lt;p&gt;2.3 Overcoming the Disturbances of the Earth Atmosphere. . . . . . . . . . . . 24&lt;/p&gt;&lt;p&gt;2.4 Exploiting All Spectral Domains from Radio to X-ray and Gamma-ray . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29&lt;/p&gt;&lt;p&gt;2.5 Visiting the Planets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35&lt;/p&gt;&lt;p&gt;2.6 No Pause in the Progress of Signal Detection and Exploitation . . . . . . 35&lt;/p&gt;&lt;p&gt;Part II Stars are Well Understood . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39&lt;/p&gt;&lt;p&gt;CHAPTER 3&lt;/p&gt;&lt;p&gt;How does a Star Work? . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41&lt;/p&gt;&lt;p&gt;3.1 Understanding the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41&lt;/p&gt;&lt;p&gt;3.2 Solving the Mystery of the Origin of the Energy of the Sun and the Stars . . . . . . . . . . . . .&amp;nbsp; . . . . . . . . . . . . . . . . . . . . . . 42&lt;/p&gt;&lt;p&gt;3.3 The Life of the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46&lt;/p&gt;&lt;p&gt;3.4 Our Atoms were Born in the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . 51&lt;/p&gt;&lt;p&gt;3.5 Stars also Die . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52&lt;/p&gt;&lt;p&gt;CHAPTER 4&lt;/p&gt;&lt;p&gt;Complexities of Star Birth and Physics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57&lt;/p&gt;&lt;p&gt;4.1 General Star Formation Scenario . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57&lt;/p&gt;&lt;p&gt;4.2 Young Infrared Stars: Born in Dusty Cocoons . . . . . . . . . . . . . . . . . . . 59&lt;/p&gt;&lt;p&gt;4.3 Gravitational Contraction, Accretion and Discs. . . . . . . . . . . . . . . . . . 59&lt;/p&gt;&lt;p&gt;4.4 Universality of Stellar Pairs – Complex Ending of Their Lives . . . . . . . 61&lt;/p&gt;&lt;p&gt;4.5 Brown Dwarfs, Billions of Aborted Stars . . . . . . . . . . . . . . . . . . . . . . . 63&lt;/p&gt;&lt;p&gt;4.6 Stars are Still at the Forefront of Current Astronomy . . . . . . . . . . . . . 65&lt;/p&gt;&lt;p&gt;4.7 Stars and Ecology of Planets and Galaxies . . . . . . . . . . . . . . . . . . . . . 68&lt;/p&gt;&lt;p&gt;Part III The New World of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 71&lt;/p&gt;&lt;p&gt;CHAPTER 5&lt;/p&gt;&lt;p&gt;Discovery of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73&lt;/p&gt;&lt;p&gt;5.1 The Appreciation of the Nature of Galaxies Dates Back Only to the Beginning of the 20th Century . . . . . . . . . . . . . 73&lt;/p&gt;&lt;p&gt;5.2 First Steps in the World of Nearby Galaxies . . . . . . . . . . . . . . . . . . . . 77&lt;/p&gt;&lt;p&gt;5.3 Architecture and Stellar Content of Galaxies . . . . . . . . . . . . . . . . . . . . 81&lt;/p&gt;&lt;p&gt;CHAPTER 6&lt;/p&gt;&lt;p&gt;Our Galaxy and Its Interstellar Medium . . . . . . . . . . . . . . . . . . . . . . . . . . . . 83&lt;/p&gt;&lt;p&gt;6.1 Exploration of Our Galaxy, the Milky Way . . . . . . . . . . . . . . . . . . . . . 83&lt;/p&gt;&lt;p&gt;6.2 An Ordinary Galaxy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 84&lt;/p&gt;&lt;p&gt;6.3 Current Organization of Stars Resulting from the Milky Way History . 86&lt;/p&gt;&lt;p&gt;6.4 The Interstellar Gas, a Key Player in the Evolution of Galaxies . . . . . 86&lt;/p&gt;&lt;p&gt;6.5 Other Players in the Interstellar Medium . . . . . . . . . . . . . . . . . . . . . . 90&lt;/p&gt;&lt;p&gt;6.6 Exotic Components of the Milky Way . . . . . . . . . . . . . . . . . . . . . . . . . 94&lt;/p&gt;&lt;p&gt;CHAPTER 7&lt;/p&gt;&lt;p&gt;Hundreds of Billions of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97&lt;/p&gt;&lt;p&gt;7.1 Galaxies at All Stages of Their Life . . . . . . . . . . . . . . . . . . . . . . . . . . . 97&lt;/p&gt;&lt;p&gt;7.2 The Turbulent Family Life of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . 99&lt;/p&gt;&lt;p&gt;7.3 Understanding the Formation and Evolution of Galaxies . . . . . . . . . . . 106&lt;/p&gt;&lt;p&gt;Part IV Cosmology, the Science of the Universe as a Whole . . . . . . . . . . . . 109&lt;/p&gt;&lt;p&gt;CHAPTER 8&lt;/p&gt;&lt;p&gt;Birth of Cosmology. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111&lt;/p&gt;&lt;p&gt;8.1 The Universe of Galaxies is Expanding . . . . . . . . . . . . . . . . . . . . . . . . 111&lt;/p&gt;&lt;p&gt;8.2 The Saga of the Big Bang Confirmation . . . . . . . . . . . . . . . . . . . . . . . 114&lt;/p&gt;&lt;p&gt;8.3 The Very First Phase in the History of the Universe: Uncertain Physics . . . . . . . . . . . . . . . . . . . 116&lt;/p&gt;&lt;p&gt;8.4 AWell-Understood Second Phase: The Standard Big Bang Model . . . . 118&lt;/p&gt;&lt;p&gt;CHAPTER 9&lt;/p&gt;&lt;p&gt;Content of the Universe and Structure Formation . . . . . . . . . . . . . . . . . . . . . 123&lt;/p&gt;&lt;p&gt;9.1 Formation of Galaxies and Structures of the Present Universe . . . . . . . 123&lt;/p&gt;&lt;p&gt;9.2 Fundamental Parameters of the Universe are Better Known than Its Physics . . . . . . . . . . . . . . . . . . 125&lt;/p&gt;&lt;p&gt;9.3 Age of the Universe and Variations of the Determinations of the Hubble Constant . . . . . . . . . . . . . . 128&lt;/p&gt;&lt;p&gt;9.4 An Overall Density Very Close to the Critical Density . . . . . . . . . . . . 128&lt;/p&gt;&lt;p&gt;9.5 Need and Nature of Dark Matter . . . . . . . . . . . . . . . . . . . . . . . . . . . . 129&lt;/p&gt;&lt;p&gt;9.6 A Last-Minute Surprise, the Re-Acceleration of the Expansion Involving an Unknown Source of Cosmic Energy . . . . . . . 131&lt;/p&gt;&lt;p&gt;9.7 Summarizing: An Unexpected Universe Model Validated in Multiple Ways . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132&lt;/p&gt;&lt;p&gt;Part V Singular Stars and Cataclysms in Extreme Physical Conditions . . . 135&lt;/p&gt;&lt;p&gt;CHAPTER 10&lt;/p&gt;&lt;p&gt;Explosions of Stars and Their Singular Residues . . . . . . . . . . . . . . . . . . . . . . 137&lt;/p&gt;&lt;p&gt;10.1 Extreme Physics of Supernova Implosion/Explosion . . . . . . . . . . . . . 137&lt;/p&gt;&lt;p&gt;10.2 Neutron Stars, Hyper-Dense Supernova Residues. . . . . . . . . . . . . . . . 145&lt;/p&gt;&lt;p&gt;10.3 Gamma-Ray Bursts, Even More Powerful Bursts . . . . . . . . . . . . . . . . 147&lt;/p&gt;&lt;p&gt;10.4 Cosmic Rays, Messenger Particles of the High Energy Universe . . . . . 149&lt;/p&gt;&lt;p&gt;CHAPTER 11&lt;/p&gt;&lt;p&gt;Black Holes and Their Power . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155&lt;/p&gt;&lt;p&gt;11.1 Black Holes, General Relativity and the Cosmos . . . . . . . . . . . . . . . . 155&lt;/p&gt;&lt;p&gt;11.2 Stellar Black Holes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157&lt;/p&gt;&lt;p&gt;11.3 GravitationalWaves, Propagation of Spacetime-Curvature Disturbances. . . 158&lt;/p&gt;&lt;p&gt;11.4 Quasars: New Stars a Thousand Times Brighter than Galaxies . . . . . 162&lt;/p&gt;&lt;p&gt;11.5 Manifestations of Super-Massive Black Holes and Their Interpretation . . . 164&lt;/p&gt;&lt;p&gt;11.6 Co-evolution of Galaxies and Their Black Hole . . . . . . . . . . . . . . . . . 170&lt;/p&gt;&lt;p&gt;11.7 The Super-Massive Black Hole of Our Galaxy and Others . . . . . . . . . 171&lt;/p&gt;&lt;p&gt;Part VI Planets, in the Solar System and Outside . . . . . . . . . . . . . . . . . . . 173&lt;/p&gt;&lt;p&gt;CHAPTER 12&lt;/p&gt;&lt;p&gt;Direct Exploration of the Planets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 175&lt;/p&gt;&lt;p&gt;12.1 Planets, Stars of Astronomy until the 19th Century . . . . . . . . . . . . . 175&lt;/p&gt;&lt;p&gt;12.2 Half a Century Without Revolution for Planetology . . . . . . . . . . . . . 178&lt;/p&gt;&lt;p&gt;12.3 Humans Went to the Moon! . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180&lt;/p&gt;&lt;p&gt;12.4 We Broadly Understand the Origin of the Moon and Its Importance for the Earth . . . . . . . . .&amp;nbsp; . . . . . . . . . . . . 181&lt;/p&gt;&lt;p&gt;12.5 Very Rich Close-up Photos of All the Bodies of the Solar System . . . 183&lt;/p&gt;&lt;p&gt;12.6 Summary of Planetary Expeditions . . . . . . . . . . . . . . . . . . . . . . . . . . 184&lt;/p&gt;&lt;p&gt;12.7 Searching for Life in the Solar System: Where and When? . . . . . . . . . 191&lt;/p&gt;&lt;p&gt;CHAPTER 13&lt;/p&gt;&lt;p&gt;Entering the Dream World of Exoplanets . . . . . . . . . . . . . . . . . . . . . . . . . . . 197&lt;/p&gt;&lt;p&gt;13.1 Explosion of Discoveries of New Planets . . . . . . . . . . . . . . . . . . . . . . 197&lt;/p&gt;&lt;p&gt;13.2 The Majority of Stars have a Planetary System. . . . . . . . . . . . . . . . . 201&lt;/p&gt;&lt;p&gt;13.3 Surprising Variety of Exoplanets . . . . . . . . . . . . . . . . . . . . . . . . . . . . 202&lt;/p&gt;&lt;p&gt;13.4 The Search for Earth-Like Planets. . . . . . . . . . . . . . . . . . . . . . . . . . . 204&lt;/p&gt;&lt;p&gt;Conclusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 209&lt;/p&gt;&lt;p&gt;CHAPTER 14&lt;/p&gt;&lt;p&gt;A New Cosmos in the 21st Century?. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211&lt;/p&gt;&lt;p&gt;14.1 A New Cosmos . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211&lt;/p&gt;&lt;p&gt;14.2 Auguries for 21st Century Astronomy? . . . . . . . . . . . . . . . . . . . . . . . 212&lt;/p&gt;&lt;p&gt;Glossary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 217&lt;/p&gt;&lt;p&gt;Acronyms and Space Missions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 223&lt;/p&gt;&lt;p&gt;References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 227&lt;/p&gt;&lt;p&gt;Index . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 231&lt;/p&gt;&lt;p&gt;The asterisks * indicate words or acronyms whose meaning is explained in the&lt;/p&gt;&lt;p&gt;“Glossary” or “Acronyms and space missions” sections at the end of the book.&lt;/p&gt;</Text>
        <Text language="eng">&lt;p&gt;Contents&lt;/p&gt;&lt;p&gt;General Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . III&lt;/p&gt;&lt;p&gt;Acknowledgments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . VII&lt;/p&gt;&lt;p&gt;Part I A Century of Revolution in Our Vision of the Universe . . . . . . . . . . 1&lt;/p&gt;&lt;p&gt;CHAPTER 1&lt;/p&gt;&lt;p&gt;General View of 20th Century Astronomy and Its Starting Point . . . . . . . . . 3&lt;/p&gt;&lt;p&gt;1.1 Astronomy, the Key to Our Vision of the World . . . . . . . . . . . . . . . . . 3&lt;/p&gt;&lt;p&gt;1.2 Benchmarks on 1900 Astronomy and Its Shortcomings . . . . . . . . . . . . 7&lt;/p&gt;&lt;p&gt;CHAPTER 2&lt;/p&gt;&lt;p&gt;Scientific and Technical Revolutions, Drivers of 20th Century Astronomy . . . 21&lt;/p&gt;&lt;p&gt;2.1 Physics Revolutions, Keys to Astrophysics . . . . . . . . . . . . . . . . . . . . . 21&lt;/p&gt;&lt;p&gt;2.2 Giant Telescopes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22&lt;/p&gt;&lt;p&gt;2.3 Overcoming the Disturbances of the Earth Atmosphere. . . . . . . . . . . . 24&lt;/p&gt;&lt;p&gt;2.4 Exploiting All Spectral Domains from Radio to X-ray and Gamma-ray . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29&lt;/p&gt;&lt;p&gt;2.5 Visiting the Planets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35&lt;/p&gt;&lt;p&gt;2.6 No Pause in the Progress of Signal Detection and Exploitation . . . . . . 35&lt;/p&gt;&lt;p&gt;Part II Stars are Well Understood . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39&lt;/p&gt;&lt;p&gt;CHAPTER 3&lt;/p&gt;&lt;p&gt;How does a Star Work? . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41&lt;/p&gt;&lt;p&gt;3.1 Understanding the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41&lt;/p&gt;&lt;p&gt;3.2 Solving the Mystery of the Origin of the Energy of the Sun and the Stars . . . . . . . . . . . . . . . . . .. . . . . . . . . . . . . . . 42&lt;/p&gt;&lt;p&gt;3.3 The Life of the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46&lt;/p&gt;&lt;p&gt;3.4 Our Atoms were Born in the Stars . . . . . . . . . . . . . . . . . . . . . . . . . . . 51&lt;/p&gt;&lt;p&gt;3.5 Stars also Die . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52&lt;/p&gt;&lt;p&gt;CHAPTER 4&lt;/p&gt;&lt;p&gt;Complexities of Star Birth and Physics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57&lt;/p&gt;&lt;p&gt;4.1 General Star Formation Scenario . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57&lt;/p&gt;&lt;p&gt;4.2 Young Infrared Stars: Born in Dusty Cocoons . . . . . . . . . . . . . . . . . . . 59&lt;/p&gt;&lt;p&gt;4.3 Gravitational Contraction, Accretion and Discs. . . . . . . . . . . . . . . . . . 59&lt;/p&gt;&lt;p&gt;4.4 Universality of Stellar Pairs – Complex Ending of Their Lives . . . . . . . 61&lt;/p&gt;&lt;p&gt;4.5 Brown Dwarfs, Billions of Aborted Stars . . . . . . . . . . . . . . . . . . . . . . . 63&lt;/p&gt;&lt;p&gt;4.6 Stars are Still at the Forefront of Current Astronomy . . . . . . . . . . . . . 65&lt;/p&gt;&lt;p&gt;4.7 Stars and Ecology of Planets and Galaxies . . . . . . . . . . . . . . . . . . . . . 68&lt;/p&gt;&lt;p&gt;Part III The New World of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 71&lt;/p&gt;&lt;p&gt;CHAPTER 5&lt;/p&gt;&lt;p&gt;Discovery of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73&lt;/p&gt;&lt;p&gt;5.1 The Appreciation of the Nature of Galaxies Dates Back Only to the Beginning of the 20th Century . . . . . . . . .&amp;nbsp; . . . . . . 73&lt;/p&gt;&lt;p&gt;5.2 First Steps in the World of Nearby Galaxies . . . . . . . . . . . . . . . . . . . . 77&lt;/p&gt;&lt;p&gt;5.3 Architecture and Stellar Content of Galaxies . . . . . . . . . . . . . . . . . . . . 81&lt;/p&gt;&lt;p&gt;CHAPTER 6&lt;/p&gt;&lt;p&gt;Our Galaxy and Its Interstellar Medium . . . . . . . . . . . . . . . . . . . . . . . . . . . . 83&lt;/p&gt;&lt;p&gt;6.1 Exploration of Our Galaxy, the Milky Way . . . . . . . . . . . . . . . . . . . . . 83&lt;/p&gt;&lt;p&gt;6.2 An Ordinary Galaxy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 84&lt;/p&gt;&lt;p&gt;6.3 Current Organization of Stars Resulting from the Milky Way History . 86&lt;/p&gt;&lt;p&gt;6.4 The Interstellar Gas, a Key Player in the Evolution of Galaxies . . . . . 86&lt;/p&gt;&lt;p&gt;6.5 Other Players in the Interstellar Medium . . . . . . . . . . . . . . . . . . . . . . 90&lt;/p&gt;&lt;p&gt;6.6 Exotic Components of the Milky Way . . . . . . . . . . . . . . . . . . . . . . . . . 94&lt;/p&gt;&lt;p&gt;CHAPTER 7&lt;/p&gt;&lt;p&gt;Hundreds of Billions of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97&lt;/p&gt;&lt;p&gt;7.1 Galaxies at All Stages of Their Life . . . . . . . . . . . . . . . . . . . . . . . . . . . 97&lt;/p&gt;&lt;p&gt;7.2 The Turbulent Family Life of Galaxies . . . . . . . . . . . . . . . . . . . . . . . . 99&lt;/p&gt;&lt;p&gt;7.3 Understanding the Formation and Evolution of Galaxies . . . . . . . . . . . 106&lt;/p&gt;&lt;p&gt;Part IV Cosmology, the Science of the Universe as a Whole . . . . . . . . . . . . 109&lt;/p&gt;&lt;p&gt;CHAPTER 8&lt;/p&gt;&lt;p&gt;Birth of Cosmology. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111&lt;/p&gt;&lt;p&gt;8.1 The Universe of Galaxies is Expanding . . . . . . . . . . . . . . . . . . . . . . . . 111&lt;/p&gt;&lt;p&gt;8.2 The Saga of the Big Bang Confirmation . . . . . . . . . . . . . . . . . . . . . . . 114&lt;/p&gt;&lt;p&gt;8.3 The Very First Phase in the History of the Universe: Uncertain Physics . . . . . . . . . . . . . . . . . . . . . 116&lt;/p&gt;&lt;p&gt;8.4 AWell-Understood Second Phase: The Standard Big Bang Model . . . . 118&lt;/p&gt;&lt;p&gt;CHAPTER 9&lt;/p&gt;&lt;p&gt;Content of the Universe and Structure Formation . . . . . . . . . . . . . . . . . . . . . 123&lt;/p&gt;&lt;p&gt;9.1 Formation of Galaxies and Structures of the Present Universe . . . . . . . 123&lt;/p&gt;&lt;p&gt;9.2 Fundamental Parameters of the Universe are Better Known than Its Physics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 125&lt;/p&gt;&lt;p&gt;9.3 Age of the Universe and Variations of the Determinations of the Hubble Constant . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 128&lt;/p&gt;&lt;p&gt;9.4 An Overall Density Very Close to the Critical Density . . . . . . . . . . . . 128&lt;/p&gt;&lt;p&gt;9.5 Need and Nature of Dark Matter . . . . . . . . . . . . . . . . . . . . . . . . . . . . 129&lt;/p&gt;&lt;p&gt;9.6 A Last-Minute Surprise, the Re-Acceleration of the Expansion Involving an Unknown Source of Cosmic Energy . . . . . . . . . . . 131&lt;/p&gt;&lt;p&gt;9.7 Summarizing: An Unexpected Universe Model Validated in Multiple Ways . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132&lt;/p&gt;&lt;p&gt;Part V Singular Stars and Cataclysms in Extreme Physical Conditions . . . 135&lt;/p&gt;&lt;p&gt;CHAPTER 10&lt;/p&gt;&lt;p&gt;Explosions of Stars and Their Singular Residues . . . . . . . . . . . . . . . . . . . . . . 137&lt;/p&gt;&lt;p&gt;10.1 Extreme Physics of Supernova Implosion/Explosion . . . . . . . . . . . . . 137&lt;/p&gt;&lt;p&gt;10.2 Neutron Stars, Hyper-Dense Supernova Residues. . . . . . . . . . . . . . . . 145&lt;/p&gt;&lt;p&gt;10.3 Gamma-Ray Bursts, Even More Powerful Bursts . . . . . . . . . . . . . . . . 147&lt;/p&gt;&lt;p&gt;10.4 Cosmic Rays, Messenger Particles of the High Energy Universe . . . . . 149&lt;/p&gt;&lt;p&gt;CHAPTER 11&lt;/p&gt;&lt;p&gt;Black Holes and Their Power . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155&lt;/p&gt;&lt;p&gt;11.1 Black Holes, General Relativity and the Cosmos . . . . . . . . . . . . . . . . 155&lt;/p&gt;&lt;p&gt;11.2 Stellar Black Holes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157&lt;/p&gt;&lt;p&gt;11.3 GravitationalWaves, Propagation of Spacetime-Curvature Disturbances. . . 158&lt;/p&gt;&lt;p&gt;11.4 Quasars: New Stars a Thousand Times Brighter than Galaxies . . . . . 162&lt;/p&gt;&lt;p&gt;11.5 Manifestations of Super-Massive Black Holes and Their Interpretation . . . 164&lt;/p&gt;&lt;p&gt;11.6 Co-evolution of Galaxies and Their Black Hole . . . . . . . . . . . . . . . . . 170&lt;/p&gt;&lt;p&gt;11.7 The Super-Massive Black Hole of Our Galaxy and Others . . . . . . . . . 171&lt;/p&gt;&lt;p&gt;Part VI Planets, in the Solar System and Outside . . . . . . . . . . . . . . . . . . . 173&lt;/p&gt;&lt;p&gt;CHAPTER 12&lt;/p&gt;&lt;p&gt;Direct Exploration of the Planets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 175&lt;/p&gt;&lt;p&gt;12.1 Planets, Stars of Astronomy until the 19th Century . . . . . . . . . . . . . 175&lt;/p&gt;&lt;p&gt;12.2 Half a Century Without Revolution for Planetology . . . . . . . . . . . . . 178&lt;/p&gt;&lt;p&gt;12.3 Humans Went to the Moon! . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180&lt;/p&gt;&lt;p&gt;12.4 We Broadly Understand the Origin of the Moon and Its Importance for the Earth . . . . . . . .&amp;nbsp; . . . . . . . . . . . . . . 181&lt;/p&gt;&lt;p&gt;12.5 Very Rich Close-up Photos of All the Bodies of the Solar System . . . 183&lt;/p&gt;&lt;p&gt;12.6 Summary of Planetary Expeditions . . . . . . . . . . . . . . . . . . . . . . . . . . 184&lt;/p&gt;&lt;p&gt;12.7 Searching for Life in the Solar System: Where and When? . . . . . . . . . 191&lt;/p&gt;&lt;p&gt;CHAPTER 13&lt;/p&gt;&lt;p&gt;Entering the Dream World of Exoplanets . . . . . . . . . . . . . . . . . . . . . . . . . . . 197&lt;/p&gt;&lt;p&gt;13.1 Explosion of Discoveries of New Planets . . . . . . . . . . . . . . . . . . . . . . 197&lt;/p&gt;&lt;p&gt;13.2 The Majority of Stars have a Planetary System. . . . . . . . . . . . . . . . . 201&lt;/p&gt;&lt;p&gt;13.3 Surprising Variety of Exoplanets . . . . . . . . . . . . . . . . . . . . . . . . . . . . 202&lt;/p&gt;&lt;p&gt;13.4 The Search for Earth-Like Planets. . . . . . . . . . . . . . . . . . . . . . . . . . . 204&lt;/p&gt;&lt;p&gt;Conclusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 209&lt;/p&gt;&lt;p&gt;CHAPTER 14&lt;/p&gt;&lt;p&gt;A New Cosmos in the 21st Century?. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211&lt;/p&gt;&lt;p&gt;14.1 A New Cosmos . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211&lt;/p&gt;&lt;p&gt;14.2 Auguries for 21st Century Astronomy? . . . . . . . . . . . . . . . . . . . . . . . 212&lt;/p&gt;&lt;p&gt;Glossary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 217&lt;/p&gt;&lt;p&gt;Acronyms and Space Missions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 223&lt;/p&gt;&lt;p&gt;References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 227&lt;/p&gt;&lt;p&gt;Index . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 231&lt;/p&gt;&lt;p&gt;The asterisks * indicate words or acronyms whose meaning is explained in the&lt;/p&gt;&lt;p&gt;“Glossary” or “Acronyms and space missions” sections at the end of the book.&lt;/p&gt;</Text>
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