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  • 1
    Buch
    Buch
    New York, NY :Copernicus,
    UID:
    almafu_BV013135761
    Umfang: XXVIII, 333 S. : , Ill., graph. Darst.
    ISBN: 0-387-98701-0
    Inhalt: In this introduction to the emerging field of astrobiology, a distinguished paleontologist and a noted astronomer team up to provide a fascinating synthesis of what's now known about the rise of life on Earth and how it sheds light on possibilities for organic life forms elsewhere in the universe. Illustrations. First book to synthesize discoveries from astronomy & paleontology regarding the advent of life on earth, & the potential for the development of life on other planets.
    Sprache: Englisch
    Fachgebiete: Biologie
    RVK:
    Schlagwort(e): Außerirdisches Leben ; Komplexität
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
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  • 2
    Online-Ressource
    Online-Ressource
    New York, NY :Springer New York :
    UID:
    almahu_9949199313202882
    Umfang: XXXIV, 338 p. , online resource.
    Ausgabe: 1st ed. 2000.
    ISBN: 9780387218489
    Inhalt: In November 12, 2002, Dr. John Chambers of the NASA Ames Research Center gave a seminar to the Astrobiology Group at the University of Washington. The audience of about 100 listened with rapt attention as Chambers described results from a computer study of how planetary systems form. The goal of his research was to answer a deceptively simple question: How often would newly forming planetary systems produce Earth-like planets, given a star the size of our own sun? By "Earth-like" Chambers meant a rocky planet with water on its surface, orbiting within a star's "habitable zone. " This not-too-hot and not-too-cold inner region, relatively close to the star, supports the presence of liquid water on a planet surface for hundreds of million of years-the time-span probably necessary for the evolution of life. To answer the question of just how many Earth-like planets might be spawned in such a planetary system, Chambers had spent thousands of hours running highly sophisticated modeling programs through arrays of powerful computers. The results presented at the meeting were startling. The simulations showed that rocky planets orbiting at the "right" distances from the central star are easily formed, but they can end up with a wide range of water content. Earth seems to be quite a gem-a rocky planet where not only can liquid water exist for long periods of time, but where water can be found as a heathy oceanful-not too little and not too much. Our planet seems to reside in a benign region of the Galaxy, where comet and asteroid bombardment is tolerable and habitable-zone planets can commonly grow to Earth size. Such real estate in our galaxy-perhaps in any galaxy-is prime for life. And rare as well.
    Anmerkung: Why Life Might Be Widespread in the Universe -- Habitable Zones of the Universe -- Building a Habitable Earth -- Life's First Appearance on Earth -- How to Build Animals -- Snowball Earth -- The Enigma of the Cambrian Explosion -- Mass Extinctions and the Rare Earth Hypothesis -- The Surprising Importance of Plate Tectonics -- The Moon, Jupiter, and Life on Earth -- Testing the Rare Earth Hypothesis -- Assessing the Odds -- Messengers from the Stars.
    In: Springer Nature eBook
    Weitere Ausg.: Printed edition: ISBN 9780387952895
    Weitere Ausg.: Printed edition: ISBN 9781475781137
    Weitere Ausg.: Printed edition: ISBN 9780387987019
    Sprache: Englisch
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
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  • 3
    Buch
    Buch
    New York : Copernicus Books
    UID:
    kobvindex_GFZ100815
    Umfang: 333 p.
    ISBN: 0387987010
    Anmerkung: MAB0014.001: PIK N 322-01-0190
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
    BibTip Andere fanden auch interessant ...
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