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First Light: Switching on Stars at the Dawn of Time-Emma Chapman

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Astronomers have successfully observed a great deal of the Universe's history, from recording the afterglow of the Big Bang to imaging thousands of galaxies, and even to visualising an actual black hole. There's a lot for astronomers to be smug about. But when it comes to understanding how the Universe began and grew up we are literally in the dark ages. In effect, we are missing the first one billion years from the timeline of the Universe. This brief but far-reaching period in the Universe's history, known to astrophysicists as the 'Epoch of Reionisation', represents the start of the cosmos as we experience it today. The time when the very first stars burst into life, when darkness gave way to light. After hundreds of millions of years of dark, uneventful expansion, one by the one these stars suddenly came into being. This was the point at which the chaos of the Big Bang first began to yield to the order of galaxies, black holes and stars, kick-starting the pathway to planets, to comets, to moons, and to life itself. Incorporating the very latest research into this branch of astrophysics, this book sheds light on this time of darkness, telling the story of these first stars, hundreds of times the size of the Sun and a million times brighter, lonely giants that lived fast and died young in powerful explosions that seeded the Universe with the heavy elements that we are made of. Emma Chapman tells us how these stars formed, why they were so unusual, and what they can teach us about the Universe today. She also offers a first-hand look at the immense telescopes about to come on line to peer into the past, searching for the echoes and footprints of these stars, to take this period in the Universe's history from the realm of theoretical physics towards the wonder of observational astronomy.

Book First Light: Switching on Stars at the Dawn of Time Review :



This is a very well written overview of cosmology for the lay reader. The author is engaging and as succinct as possible without the use of equations. There is an obvious howler on page 112 where I believe the printer missed a decimal. We are 2.5 million light years from Andromeda not 250 million! I reccomend this book highly
A previous reviewer said the book, in parts, was more suited for a astrophysics course. I agree. Those parts I had to read and reread to digest them. Even then I thought it was too much detail, even for a college astrophysics or astronomy course, but would have been better suited for an astronomy grad student in the field actually studying certain aspects of astronomy, like stellar archeology. That said, the rest of the book was easy reading, for me anyway. And very informative, as I separated the academic wheat from the chaff.For instance, the discussion of cosmic microwave background, occurring about 380,000 years after the Big Bang, at which time protons and electrons combined sufficiently to allow photons to escape their confinement and thus be observable billions of years later, including now. A very significant date and occurrence. Then more than 100 million years after the Big Bang we have stars forming. The author groups stars, ancient and modern, into three groups, Population I, Ii, and III, with III being the oldest. We haven't found any of them yet.They are the Holy Grail of stellar evolution astronomers. These Population III stars are metal-poor, which means they have virtually no elements heavier than helium. Population I stars are much newer and are metal-rich, including very heavy elements, derived from stars that exploded millions and even billions of years ago. Our own sun is an example of this. It contains elements it did not produce that were present in the gas and particles from which the sun formed.There's a discussion of the fate of stars when they burn through sufficient fuel and can no long fight off the force of gravity, thus going into a supernova and, depending on their size, becoming a white dwarf (the fate of our sun), a neutron star or a black hole.The author tells us about the James Webb Space Telescope, set to be launched this year, 2021. It's a telescope designed to pick up infrared electromagnetic radiation, unlike the Hubble telescope which is an optical telescope. The Webb telescope will capture the longer wavelength radiation that the Hubble cannot see. Because of the tremendous expansion of the Universe, radiation emitted many billions of years ago has been red shifted from the visible spectrum into the longer wavelengths of the infrared spectrum.There's also a discussion of gravitational waves and their capture and recording and measurement by LIGO detectors. Well explained. Easy to understand.All in all, a worthwhile read, despite the tough parts of the book. I recommend it.

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