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  • 1
    Monograph available for loan
    Monograph available for loan
    New Jersey : Prentice-Hall
    Call number: PIK N 421-00-0039
    Type of Medium: Monograph available for loan
    Pages: 351 p.
    ISBN: 0131773879
    Location: A 18 - must be ordered
    Branch Library: PIK Library
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  • 2
    Monograph available for loan
    Monograph available for loan
    San Francisco [u.a.] : Pearson Education International
    Call number: IASS 12.0016
    Type of Medium: Monograph available for loan
    Pages: xi, 420 S. , Ill., graph. Darst., Kt.
    Edition: 3rd ed.
    ISBN: 9780321733283
    Branch Library: IASS Library
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  • 3
    Electronic Resource
    Electronic Resource
    Palo Alto, Calif. : Annual Reviews
    Annual Review of Astronomy and Astrophysics 41 (2003), S. 429-463 
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Giant planets have now been discovered around other stars, and it is only a matter of time until Earth-sized planets are detected. Whether any of these planets are suitable for life depends on their volatile abundances, especially water, and on their climates. Only planets within the liquid-water habitable zone (HZ) can support life on their surfaces and, thus, can be analyzed remotely to determine whether they are inhabited. Fortunately, current models predict that HZs are relatively wide around main-sequence stars not too different from our sun. This conclusion is based on studies of how our own planet has evolved over time. Earth's climate has remained conducive to life for the past 3.5 billion years or more, despite a large increase in solar luminosity, probably because of previous higher concentrations of CO2 and/or CH4. Both these gases are involved in negative feedback loops that help to stabilize the climate. In addition to these topics, we also briefly discuss the rise of atmospheric O2 and O3, along with their possible significance as indicators of life on other planets.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 443 (2006), S. 643-645 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The ancient rise of atmospheric oxygen is of great interest because of its close relationship with evolution, but the geological evidence for this is indirect and subject to interpretation. The consensus for more than 30 years has been that atmospheric oxygen first reached appreciable levels around ...
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 447.2007, 7140, E1-, (1 S.) 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Arising from: F. Robert & M. Chaussidon Nature 443, 969–972 (2006); Robert & Chaussidon reply The oxygen isotopes in sedimentary cherts (siliceous sediments) have been used to argue that the Precambrian ...
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 412 (2001), S. 26-27 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] To what extent is biological evolution driven by environmental evolution? This is one of the big questions for both evolutionary biologists and geoscientists. On page 61 of this issue, Navarro-González and colleagues describe their investigation into a central innovation in the ...
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 432 (2004), S. 0 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Arising from: H. Ohmoto, Y. Watanabe & K. Kumazawa Nature 429, 395–399 (2004); see also communication from N. H. Sleep; H. Ohmoto & Y. Watanabe reply Ohmoto et al. argue that carbon ...
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 385 (1997), S. 234-236 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Moons orbiting giant planets face additional problems that an isolated Earth-like planet would not encounter. At 1 AU from a solar-type star, all moons within a jovian planet's Hill sphere (the limit for orbital stability) would become tidally locked within a few billion years of their formation. ...
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 352 (1991), S. 489-496 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Mars is believed to be lifeless, but it may be possible to transform it into a planet suitable for habitation by plants, and conceivably humans. The success of such an enterprise would depend on the abundance, distribution and form of materials on the planet that could provide carbon dioxide, ...
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    Springer
    Origins of life and evolution of the biospheres 27 (1997), S. 291-307 
    ISSN: 1573-0875
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Geosciences
    Notes: Abstract Habitable planets are likely to exist around stars nottoo different from the Sun if current theories about terrestrialclimate evolution are correct. Some of these planets may have evolved life, and some of the inhabited planets may have evolved O2-rich atmospheres. Such atmospheres could be detectedspectroscopically on planets around nearby stars using a space-based interferometer to search for the 9.6μm band of O3.Planets with O2-rich atmospheres that lie within the habitable zone around their parent star are, in all probability, inhabited.
    Type of Medium: Electronic Resource
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