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Sagittarius A*: The Complete Science of the Milky Way's Supermassive Black Hole: From Nobel Prize Stellar Orbits and the 2022 Event Horizon Telescope
Paperback
Series: Black Holes for Adult, Book 4
Technology & EngineeringAstronomy & Space
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ISBN13: 9798185742594
Publisher: Independently Published
Pages: 114
Weight: 0.36
Height: 0.24 Width: 6.00 Depth: 9.00
Language: English
Publisher: Independently Published
Pages: 114
Weight: 0.36
Height: 0.24 Width: 6.00 Depth: 9.00
Language: English
At the exact center of the Milky Way, 26,000 light-years from Earth, sits one of the most extraordinary objects in the universe. It is four million times more massive than the Sun. It fits inside a sphere smaller than the orbit of Mercury. And in 2022, for the first time in history, it was photographed.
Its name is Sagittarius A*. This book is its complete story.
Sagittarius A* is the most comprehensive adult-level account of the supermassive black hole at the center of our galaxy ever written. Fifteen deeply expanded chapters trace everything known about this object: from its accidental first detection as an anomalous radio signal in the 1930s through the two-decade stellar orbit campaigns that earned the 2020 Nobel Prize in Physics, through the extraordinary 2022 Event Horizon Telescope photograph, through the relativistic effects being detected in real time in the orbits of the S-stars, through the accretion physics that makes it one of the quietest supermassive black holes in the observable universe, all the way to the future observational program that will characterize galactic center science for the next generation.
This is the only book dedicated entirely to Sagittarius A at this depth.*
Across fifteen chapters, you will understand:
The complete history of how Sagittarius A* was discovered: from Karl Jansky's accidental radio detection in 1931, to Harlow Shapley's first correct estimate of the galactic center direction, to the naming of Sagittarius A* by Robert Brown in 1982, to the first detection of high stellar velocities that pointed unmistakably to an enormous concentration of mass, to the Nobel Prize-winning orbital campaigns of Reinhard Genzel and Andrea Ghez that built the case for a supermassive black hole to mathematical certainty over twenty-five years of painstaking observations.
The anatomy of the black hole itself: how its mass of 4.297 million solar masses has been measured to better than 0.3 percent precision through Keplerian orbital mechanics, what the Schwarzschild radius of 12.7 million kilometers means physically, and how the spin parameter of Sagittarius A* is being progressively constrained through photon ring morphology and stellar orbital precession measurements.
The 2022 Event Horizon Telescope image: what it actually shows and what it proves, why imaging Sagittarius A* was technically harder than imaging M87 despite its closer proximity, how the interstellar scattering correction was achieved, what the photon ring angular diameter tells us about the black hole mass, and how the image compares with the M87 photograph to confirm that the photon ring structure is a universal prediction of general relativity rather than an artifact of either specific system. The young star paradox: why the massive blue O and B stars orbiting within half a light-year of Sagittarius A* should not be there according to standard star formation theory, what the disk instability and Hills mechanism models propose as explanations, how hypervelocity stars in the galactic halo provide indirect evidence for the Hills mechanism, and what the G2 cloud encounter with the black hole in 2014 taught us about the limits of our theoretical models.
The future: how the Extremely Large Telescopes will find shorter-period S-stars to measure the Lense-Thirring frame dragging and test the no-hair theorem, how the expanded Event Horizon Telescope will produce movies of the accretion flow, how LISA will detect extreme mass ratio inspirals of stellar black holes into Sagittarius A*, how the Square Kilometre Array is hunting for the galactic center pulsar that would be the most powerful relativistic probe ever found, and why Sagittarius A* will remain the cornerstone of black hole physics for as long as observational astronomy exists.
Sagittarius A* is the most comprehensive adult-level account of the supermassive black hole at the center of our galaxy ever written. Fifteen deeply expanded chapters trace everything known about this object: from its accidental first detection as an anomalous radio signal in the 1930s through the two-decade stellar orbit campaigns that earned the 2020 Nobel Prize in Physics, through the extraordinary 2022 Event Horizon Telescope photograph, through the relativistic effects being detected in real time in the orbits of the S-stars, through the accretion physics that makes it one of the quietest supermassive black holes in the observable universe, all the way to the future observational program that will characterize galactic center science for the next generation.
This is the only book dedicated entirely to Sagittarius A at this depth.*
Across fifteen chapters, you will understand:
The complete history of how Sagittarius A* was discovered: from Karl Jansky's accidental radio detection in 1931, to Harlow Shapley's first correct estimate of the galactic center direction, to the naming of Sagittarius A* by Robert Brown in 1982, to the first detection of high stellar velocities that pointed unmistakably to an enormous concentration of mass, to the Nobel Prize-winning orbital campaigns of Reinhard Genzel and Andrea Ghez that built the case for a supermassive black hole to mathematical certainty over twenty-five years of painstaking observations.
The anatomy of the black hole itself: how its mass of 4.297 million solar masses has been measured to better than 0.3 percent precision through Keplerian orbital mechanics, what the Schwarzschild radius of 12.7 million kilometers means physically, and how the spin parameter of Sagittarius A* is being progressively constrained through photon ring morphology and stellar orbital precession measurements.
The 2022 Event Horizon Telescope image: what it actually shows and what it proves, why imaging Sagittarius A* was technically harder than imaging M87 despite its closer proximity, how the interstellar scattering correction was achieved, what the photon ring angular diameter tells us about the black hole mass, and how the image compares with the M87 photograph to confirm that the photon ring structure is a universal prediction of general relativity rather than an artifact of either specific system. The young star paradox: why the massive blue O and B stars orbiting within half a light-year of Sagittarius A* should not be there according to standard star formation theory, what the disk instability and Hills mechanism models propose as explanations, how hypervelocity stars in the galactic halo provide indirect evidence for the Hills mechanism, and what the G2 cloud encounter with the black hole in 2014 taught us about the limits of our theoretical models.
The future: how the Extremely Large Telescopes will find shorter-period S-stars to measure the Lense-Thirring frame dragging and test the no-hair theorem, how the expanded Event Horizon Telescope will produce movies of the accretion flow, how LISA will detect extreme mass ratio inspirals of stellar black holes into Sagittarius A*, how the Square Kilometre Array is hunting for the galactic center pulsar that would be the most powerful relativistic probe ever found, and why Sagittarius A* will remain the cornerstone of black hole physics for as long as observational astronomy exists.
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