Planetary Science: The Science of Planets Around Stars
Michael M. Woolfson (Author), George H. A. Cole (Author)
Book Description
There are many planetary systems other than our own, but
it is only through a detailed understanding of the relatively accessible
bodies in our solar system that a thorough appreciation of planetary
science can be gained. This is particularly pertinent with the recent
discovery of extra-solar planets and the desire to understand their
formation and the prospect of life on other worlds.
Planetary Science: The Science of Planets Around Stars focuses on the structure of planets and the stars they orbit and the interactions between them. The book is written in two parts, making it suitable for students at different levels and approaching planetary science from differing backgrounds. Twelve independent descriptive chapters reveal our solar system and the diverse bodies it contains, including satellites, planetary rings, asteroids, comets, meteorites, and interstellar dust. These chapters are accompanied by 42 detailed topics that discuss specialized subjects in a quantitative manner and will be essential reading for those in higher level courses. Coverage includes mineralogy, stellar formation and evolution, solar system dynamics, atmospheric physics, planetary interiors, thermodynamics, planetary astrophysics, and exobiology. Problems and answers are also included.
Planetary Science: The Science of Planets Around Stars presents a complete overview of planetary science for students of physics, astronomy, astrophysics, earth sciences, and geophysics. Assuming no prior knowledge of astrophysics or geophysics, this book is suitable for students studying planetary science for the first time.
Planetary Science: The Science of Planets Around Stars focuses on the structure of planets and the stars they orbit and the interactions between them. The book is written in two parts, making it suitable for students at different levels and approaching planetary science from differing backgrounds. Twelve independent descriptive chapters reveal our solar system and the diverse bodies it contains, including satellites, planetary rings, asteroids, comets, meteorites, and interstellar dust. These chapters are accompanied by 42 detailed topics that discuss specialized subjects in a quantitative manner and will be essential reading for those in higher level courses. Coverage includes mineralogy, stellar formation and evolution, solar system dynamics, atmospheric physics, planetary interiors, thermodynamics, planetary astrophysics, and exobiology. Problems and answers are also included.
Planetary Science: The Science of Planets Around Stars presents a complete overview of planetary science for students of physics, astronomy, astrophysics, earth sciences, and geophysics. Assuming no prior knowledge of astrophysics or geophysics, this book is suitable for students studying planetary science for the first time.
Product Details
- Paperback: 528 pages
- Publisher: Taylor & Francis; 1st edition (April 1, 2002)
- Language: English
- ISBN-10: 075030815X
- ISBN-13: 978-0750308151
- pdf 8,04 MB
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Fundamentals of Stellar Astrophysics
George W. Collins (Author)
Book Description
This textbook designed for advanced undergraduate students covers the foundations and principles in the field, and gives the necessary background for advanced courses. Beginning with a survey of some of the fundamentals of statistical mechanics, Collins builds up the physics of stellar structureProduct Details
- Hardcover: 494 pages
- Publisher: W H Freeman & Co (March 1989)
- Language: English
- ISBN-10: 0716719932
- ISBN-13: 978-0716719939
- djvu 6,46 MB
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The virial theorem in stellar astrophysics
George W Collins (Author)
Product Details
- Unknown Binding: 135 pages
- Publisher: Pachart Pub. House (1978)
- Language: English
- ISBN-10: 0912918136
- ISBN-13: 978-0912918136
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Diffuse matter in the universe
Michael A. Dopita (Author) Ralph S. Sutherland (Author)
Book Description
The reference work on astrophysics to provide a
comprehensive introduction to the physics of Interstellar Matter. The
objective of the book is to show how physics can be applied to the
understanding and diagnosis of the phase structure, the physical
conditions and the chemical make-up and evolution of the interstellar
medium. Unlike other textbooks in the field, here a more systematic
approach has been adopted based on the authors' lecture course
experience. It is aimed primarily at those undertaking post-graduate
courses, or those doing advanced projects as part of honours
undergraduate courses in physics or astrophysics.
Editorial Reviews
From the Back Cover
The book is designed as an astrophysics textbook to provide a comprehensive introduction to the physics of Interstellar Matter. It is aimed primarily at those undertaking postgraduate courses, or those doing advanced projects as part of honours undergraduate courses in physics or astrophysics. It should also provide a handy reference to the field for astrophysics faculty and other researchers who are not necessarily experts in this particular subdiscipline. The objective of the book is to show how physics can be applied to the understanding and diagnosis of the phase structure, the physical conditions and the chemical make-up and evolution of the interstellar medium. Based on the authors' lecture course experience, here a systematic approach has been adopted to assist the development of the reader's insight into the physics underlying the subject.Product Details
- Paperback: 456 pages
- Publisher: Springer (December 6, 2010)
- Language: English
- ISBN-10: 3642077714
- ISBN-13: 978-3642077715
- djvu 2,27 MB
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The Realm of the Nebulae
Edwin Hubble (Author)
Book Description
No modern astronomer made a more profound contribution to
our understanding of the cosmos than did Edwin Hubble, who first
conclusively demonstrated that the universe is expanding. Basing his
theory on the observation of the change in distanct galaxies, called red
shift, Hubble showed that this is a Doppler effect, or alteration in
the wavelength of light, resulting from the rapid motion of celestial
objects away from Earth. In 1935, Hubble described his principal
observations and conclusions in the Silliman lectures at Yale
University. These lectures were published the following year as "The
Realm of the Nebulae," which quickly became a classic work.
Product Details
- Paperback: 226 pages
- Publisher: Yale University Press (September 10, 1982)
- Language: English
- ISBN-10: 0300025009
- ISBN-13: 978-0300025002
- djvu 5,83 MB
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Large Antennas of the Deep Space Network
William A. Imbriale (Author)
Book Description
An important historical look at the space program's evolving telecommunications systems
Large Antennas of the Deep Space Network traces the development of the antennas of NASA's Deep Space Network (DSN) from the network's inception in 1958 to the present. It details the evolution of the large parabolic dish antennas, from the initial 26-m operation at L-band (960 MHz) through the current Ka-band (32 GHz) systems. Primarily used for telecommunications, these antennas also support radar and radio astronomy observations in the exploration of the solar system and the universe. In addition, the author also offers thorough treatment of the analytical and measurement techniques used in design and performance assessment.
Large Antennas of the Deep Space Network represents a vital addition to the literature in that it includes NASA-funded research that significantly impacts on deep space telecommunications. Part of the prestigious JPL Deep Space Communications and Navigation Series, it captures fundamental principles and practices developed during decades of deep space exploration, providing information that will enable antenna professionals to replicate radio frequencies and optics designs.
Large Antennas of the Deep Space Network traces the development of the antennas of NASA's Deep Space Network (DSN) from the network's inception in 1958 to the present. It details the evolution of the large parabolic dish antennas, from the initial 26-m operation at L-band (960 MHz) through the current Ka-band (32 GHz) systems. Primarily used for telecommunications, these antennas also support radar and radio astronomy observations in the exploration of the solar system and the universe. In addition, the author also offers thorough treatment of the analytical and measurement techniques used in design and performance assessment.
Large Antennas of the Deep Space Network represents a vital addition to the literature in that it includes NASA-funded research that significantly impacts on deep space telecommunications. Part of the prestigious JPL Deep Space Communications and Navigation Series, it captures fundamental principles and practices developed during decades of deep space exploration, providing information that will enable antenna professionals to replicate radio frequencies and optics designs.
Designed as an introduction for students in the field as well as a reference for advanced practitioners, the text assumes a basic familiarity with engineering and mathematical concepts and technical terms.
The Deep Space Communications and Navigation Series is authored by scientists and engineers with extensive experience in astronautics, communications, and related fields. It lays the foundation for innovation in the areas of deep space navigation and communications by disseminating state-of-the-art knowledge in key technologies.
Editorial Reviews
Review
"There is great benefit from the analysis and physical insight presented in this book." (IEEE Antennas and Propagation, February 2004)
From the Back Cover
An important historical look at the space program’s evolving telecommunications systemsLarge Antennas of the Deep Space Network traces the development of the antennas of NASA’s Deep Space Network (DSN) from the network’s inception in 1958 to the present. It details the evolution of the large parabolic dish antennas, from the initial 26-m operation at L-band (960 MHz) through the current Ka-band (32 GHz) systems. Primarily used for telecommunications, these antennas also support radar and radio astronomy observations in the exploration of the solar system and the universe. In addition, the author also offers thorough treatment of the analytical and measurement techniques used in design and performance assessment.Large Antennas of the Deep Space Network represents a vital addition to the literature in that it includes NASA-funded research that significantly impacts on deep space telecommunications. Part of the prestigious JPL Deep Space Communications and Navigation Series, it captures fundamental principles and practices developed during decades of deep space exploration, providing information that will enable antenna professionals to replicate radio frequencies and optics designs.
Designed as an introduction for students in the field as well as a reference for advanced practitioners, the text assumes a basic familiarity with engineering and mathematical concepts and technical terms.
The Deep Space Communications and Navigation Series is authored by scientists and engineers with extensive experience in astronautics, communications, and related fields. It lays the foundation for innovation in the areas of deep space navigation and communications by disseminating state-of-the-art knowledge in key technologies.
Product Details
- Hardcover: 302 pages
- Publisher: Wiley-Interscience; 1 edition (February 5, 2003)
- Language: English
- ISBN-10: 0471445371
- ISBN-13: 978-0471445371
- djvu 3,26 MB
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Introduction to Space Physics
Margaret G. Kivelson (Editor), Christopher T. Russell (Editor)
Book Description
Designed as a text for upper-level undergraduate and
first-year graduate students, this volume attempts to establish the
curriculum for the modern student entering the fledgling field of space
physics. The book provides a broad, yet selective, treatment of the
subject, covering virtually all aspects of space plasmas in the solar
system. There are sections on the sun and solar wind, the magnetized
and unmagnetized planets, and the fundamental process of space plasmas
including shocks, plasma waves, ULF waves, wave-particle interactions,
and auroral processes. In addition to emphasizing analysis, the authors
also place importance on underlying phenomenology with extensive
attention to observations.
Editorial Reviews
Review
"...contains a wealth of information in well-summarized
fashion...should be considered a valuable reference text for those who
would rather hear from the experts than from a single voice." Elmar R.
Reiter, Meteorology and Atmospheric Physics
"...Introduction to Space Physics is strong enough to form the backbone for an introductory graduate class....Because of its broad coverage, it will be an excellent addition to the library of any space physicist who occaisonally needs reminding of the issues and advances in other specialities." Michael E. Brown, Physics Today
"...Introduction to Space Physics is strong enough to form the backbone for an introductory graduate class....Because of its broad coverage, it will be an excellent addition to the library of any space physicist who occaisonally needs reminding of the issues and advances in other specialities." Michael E. Brown, Physics Today
Book Description
Designed as a text for upper-level undergraduate and first-year graduate students, this volume attempts to establish the curriculum for the modern student entering the emerging field of space physics, by covering almost all aspects of space plasmas in the solar system.Product Details
- Paperback: 588 pages
- Publisher: Cambridge University Press; 1st edition (April 28, 1995)
- Language: English
- ISBN-10: 0521457149
- ISBN-13: 978-0521457149
- djvu 7,14 MB
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The Data Book of Astronomy
Patrick Moore (Author)
Book Description
The Data Book of Astronomy is a one-stop reference for
astronomers at all levels of experience, from beginners to experienced
observers. Filled with data about the Earth, Moon, the planets, the
stars, our Galaxy, and the myriad galaxies in deep space, it also
reveals the latest scientific discoveries about black holes, quasars,
and the origins of the Universe.
Written by a premier astronomy expert, this book begins with a discussion of the Sun, from sunspots to solar eclipses. It then features over 100 tables on characteristics of the Moon, and the names, positions, sizes, and other key descriptors of all the planets and their satellites. The book tabulates solar and lunar eclipse, comets, close-approach asteroids, and significant meteor showers dates. Twenty-four maps show the surface features of the planets and their moons. The author then looks to the stars, their distances and movements, and their detailed classification and evolution. Forty-eight star charts cover both northern and southern hemispheres, enabling you to track down and name the main stars in all the constellations.
The maps are supported by detailed tables of the names, positions, magnitudes, and spectra of the main stars in each constellation, along with key data on galaxies, nebulae, and clusters. There is a useful catalogue of the world's great telescopes and observatories, a history of astronomy and of space research, and biographies of 250 astronomers who have been most influential in developing the current understanding of the subject.
Written by a premier astronomy expert, this book begins with a discussion of the Sun, from sunspots to solar eclipses. It then features over 100 tables on characteristics of the Moon, and the names, positions, sizes, and other key descriptors of all the planets and their satellites. The book tabulates solar and lunar eclipse, comets, close-approach asteroids, and significant meteor showers dates. Twenty-four maps show the surface features of the planets and their moons. The author then looks to the stars, their distances and movements, and their detailed classification and evolution. Forty-eight star charts cover both northern and southern hemispheres, enabling you to track down and name the main stars in all the constellations.
The maps are supported by detailed tables of the names, positions, magnitudes, and spectra of the main stars in each constellation, along with key data on galaxies, nebulae, and clusters. There is a useful catalogue of the world's great telescopes and observatories, a history of astronomy and of space research, and biographies of 250 astronomers who have been most influential in developing the current understanding of the subject.
Editorial Reviews
About the Author
Patrick Moore is the world's best known astronomer. He has presented BBC TV's Sky atNight for 43 years, and is the author of over 100
books. A lunar and planetary specialist, he
received the OBE in 1967 for his services to
astronomy, and in 1988 he received the OBE.
Product Details
- Hardcover: 522 pages
- Publisher: Taylor & Francis; 1 edition (January 1, 2000)
- Language: English
- ISBN-10: 0750306203
- ISBN-13: 978-0750306201
- djvu 19,4 MB
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