BiblioVault - Books about Astronomy

Cauldrons in the Cosmos: Nuclear Astrophysics
Claus E. Rolfs and William S. Rodney
University of Chicago Press, 1988
Library of Congress QB464.R65 1988 | Dewey Decimal 523.01

Nuclear astrophysics is, in essence, a science that attempts to understand and explain the physical universe beyond the Earth by studying its smallest particles. Cauldrons in the Cosmos, by Claus E. Rolfs and William S. Rodney, serves as a basic introduction to these endeavors. From the major discoveries in the field to a discussion of the makeup of stars to an explanation of standard lab techniques, this text provides students and scientists alike a thorough and fascinating survey of the accomplishments, goals, and methods of nuclear astrophysics. A classic in its field, Cauldrons in the Cosmos will surely remain an important reference in nuclear astrophysics for years to come.

"One could not wish for a better account of the current state of knowledge (and uncertainty) about nuclear reactions in stars."—B. E. J. Pagel, Nature

"Written in an informal style that those uninitiated into the jargon of nuclear astrophysics and astronomy will find readable and illuminating. . . . A useful and long-awaited introduction to nuclear astrophysics."—G. J. Mathews, Science

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Coloring the Universe: An Insider's Look at Making Spectacular Images of Space
Travis Rector, Kimberly Arcand, and Megan Watzke
University of Alaska Press, 2015
Library of Congress TR713.R43 2015 | Dewey Decimal 778.35

With a fleet of telescopes in space and giant observatories on the ground, professional astronomers produce hundreds of spectacular images of space every year. These colorful pictures have become infused into popular culture and can found everywhere, from advertising to television shows to memes. But they also invite questions: Is this what outer space really looks like? Are the colors real? And how do these images get from the stars to our screens?

Coloring the Universe uses accessible language to describe how these giant telescopes work, what scientists learn with them, and how they are used to make color images. It talks about how otherwise un-seeable rays, such as radio waves, infrared light, X-rays, and gamma rays, are turned into recognizable colors. And it is filled with fantastic images taken in far-away pockets of the universe. Informative and beautiful, Coloring the Universe will give space fans of all levels an insider’s look at how scientists bring deep space into brilliant focus.

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Comets
Laurel L. Wilkening
University of Arizona Press, 1982
Library of Congress QB721.C648 1982 | Dewey Decimal 523.6

Over forty authorities present sections on the nucleus, dust, coma, and tails of comets, along with sections on their origin, and relationships to other solar system bodies. . . . An excellent book.—Space News

"The volume is highly recommended to all interested in comets and the Solar System."—Journal of the British Astronomical Association

"A good representation of the studies that are currently being done on comets, and it is an extremely good source of information on a wide variety of topics."—International Comet Quarterly

"Extremely well-written and informative. . . . A must for library collections."—The Observatory

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Comets II
Edited by M. C. Festou, H. U. Keller, and H. A. Weaver
University of Arizona Press, 2004
Library of Congress QB721.C6484 2004 | Dewey Decimal 523.6

The study of comets is a field that has seen tremendous advances in recent years, far surpassing the knowledge reflected in the original Comets volume published as part of the Space Science Series in 1982. This new volume, with more than seventy contributing authors, represents the first complete overview of comet science in more than a decade and contains the most extensive collection of knowledge yet assembled in the field.

Comets II situates comet science in the global context of astrophysics for the first time by beginning with a series of chapters that describe the connection between stars and planets. It continues with a presentation of the formation and evolution of planetary systems, enabling the reader to clearly see the key role played in our own solar system by the icy planetesimals that were the seeds of the giant planets and transneptunian objects.

The book presents the key results obtained during the 1990s, in particular those collected during the apparition of the exceptional comets C/Hyakutake and C/Hale-Bopp in 1996-1997. The latest results obtained from the in situ exploration of comets P/Borrelly and P/Wild 2 are also discussed in detail.

Each topic of is designed to be accessible to students or young researchers looking for basic, yet detailed, complete and accurate, information on comet science. With its emphasis on the origin of theories and the future of research, Comets II will enable scientists to make connections across disciplinary boundaries and will set the stage for discovery and new understanding in the coming years.

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Comets: Nature and Culture
P. Andrew Karam
Reaktion Books, 2017

Radiating fire and ice, comets as a phenomenon seem part science, part myth. Two thousand years ago when a comet shot across the night sky, it convinced the Romans that Julius Caesar was a god. In 1066, Halley’s Comet was interpreted as a foreshadowing of the death of Harold the Second in the Battle of Hastings. Even today the arrival of a comet often feels auspicious, confirming our hopes, fears, and sense of wonder in the universe.

In Comets, P. Andrew Karam takes the reader on a far-ranging exploration of these most beautiful and dramatic objects in the skies, revealing how comets and humanity have been interwoven throughout history. He delves into the science of comets and how it has changed over time; the way comets have been depicted in art, religion, literature, and popular culture; and how comets have appeared in the heavens through the centuries. Comprehensive in scope and beautifully illustrated throughout, the book will appeal not only to the budding astronomer, but to anyone with an appreciation for these compelling and remarkable celestial bodies.

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Cosmic Winds and the Heliosphere
Edited by J. R. Jokipii, C. P. Sonett, and M. S. Giampapa
University of Arizona Press, 1997
Library of Congress QB529.C687 1997 | Dewey Decimal 523.58

Until the advent of space physics, astrophysical plasmas could be studied only using ground-based observations. Although observational methods have advanced over recent decades, the merging of heliospheric physics with astrophysics is far from complete due to the vastly different techniques employed by astronomers and space physicists. That astrophysical plasmas can be studies directly is a major advance in astrophysical research. The solar wind from the Sun is only one of many examples of solar winds, but it provides scientists with a basis for understanding how these formerly disparate disciplines are related.

Cosmic Winds and the Heliosphere is a comprehensive sourcebook on conceptually correlated topics in astrophysical winds and heliospheric physics. The contributors review the various kinds of winds, such as solar wind, winds of cataclysmic variables, and winds from pulsating stars. They then examine the physics of wind origin and physical phenomena in winds. including heliospheric shocks, magnetohydrodynamic turbulence, and kinetic phenomena. A final section considers interactions with surrounding media, with contributions ranging from studies of the interstellar cloud surrounding the solar system to considerations of solar wind interaction with comets.

Prepared to the scrupulous standards of the University of Arizona Space Science Series, Cosmic Winds and the Heliosphere is an essential volume for astronomers and space physicists.

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Cosmos: An Illustrated History of Astronomy and Cosmology
John North
University of Chicago Press, 2008
Library of Congress QB15.N67 2008 | Dewey Decimal 520.9

For millennia humans have studied the skies to help them grow crops, navigate the seas, and earn favor from their gods. We still look to the stars today for answers to fundamental questions: How did the universe begin? Will it end, and if so, how? What is our place within it? John North has been examining such questions for decades. In Cosmos, he offers a sweeping historical survey of the two sciences that help define our place in the universe: astronomy and cosmology.
            Organizing his history chronologically, North begins by examining Paleolithic cave drawings that clearly chart the phases of the moon. He then investigates scientific practices in the early civilizations of Egypt, Greece, China, and the Americas (among others), whose inhabitants developed sophisticated methods to record the movements of the planets and stars. Trade routes and religious movements, North notes, brought these ancient styles of scientific thinking to the attention of later astronomers, whose own theories—such as Copernicus’ planetary theory—led to the Scientific Revolution.
            The work of master astronomers, including Ptolemy, Galileo, Kepler, and Newton, is described in detail, as are modern-day developments in astrophysics, such as the advent of radio astronomy, the brilliant innovations of Einstein, and the many recent discoveries brought about with the help of the Hubble telescope. This new edition brings North’s seminal book right up to the present day, as North takes a closer look at last year’s reclassification of Pluto as a “dwarf” planet and gives a thorough overview of current research.
            With more than two hundred illustrations and a comprehensive bibliography, Cosmos is the definitive history of astronomy and cosmology. It is sure to find an eager audience among historians of science and astronomers alike.

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