Fundamentals of geophysics /
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TextPublisher: CAMBRIDGE CAMBRIDGE UNIVERSITY PRESS 2020Edition: Third editionDescription: pages cmISBN: 9781108716970Subject(s): GeophysicsDDC classification: 550 Summary: "The solar system originated more than 4.5 billion years ago from a rotating cloud of molecular hydrogen and interstellar dust surrounding a star that became the Sun. Collisions and coalescence of particles in the dust cloud led to the formation of a solar system with eight planets and countless smaller bodies that has fascinated mankind since prehistoric times. Our knowledge of the solar system exploded in the recent era of space exploration, and its complete description deserves a library on its own. This chapter provides brief descriptions of the orbits and physical properties of the major planetary bodies. These exhibit natural phenomena originally studied on Earth, such as gravitational and magnetic fields, seismicity, and tidal motions. They can be understood with geophysical concepts and techniques introduced in later chapters"--
| Item type | Current location | Collection | Call number | Status | Date due | Barcode |
|---|---|---|---|---|---|---|
| Books | MES LIBRARY, PONNANI | GEOLOGY | 550 LOW/F (Browse shelf) | Available | 39179 |
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| 550 KEL/I INTRODUCTION TO ENVIRONMENTAL GEOLOGY | 550 LLI/Q QUANTITATIVE GEOPHYSICS AND GEOLOGY | 550 LLI/Q QUANTITATIVE GEOPHYSICS AND GEOLOGY | 550 LOW/F Fundamentals of geophysics / | 550 MAR/E EARTH PORTRAIT OF A PLANET | 550 MED/E EARTH SCIENCE | 550 MEN/G GEOLOGY, RESOURCES AND SOCIETY: AN INTRODUCTION TO EARTH SCIENCE |
"The solar system originated more than 4.5 billion years ago from a rotating cloud of molecular hydrogen and interstellar dust surrounding a star that became the Sun. Collisions and coalescence of particles in the dust cloud led to the formation of a solar system with eight planets and countless smaller bodies that has fascinated mankind since prehistoric times. Our knowledge of the solar system exploded in the recent era of space exploration, and its complete description deserves a library on its own. This chapter provides brief descriptions of the orbits and physical properties of the major planetary bodies. These exhibit natural phenomena originally studied on Earth, such as gravitational and magnetic fields, seismicity, and tidal motions. They can be understood with geophysical concepts and techniques introduced in later chapters"--
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