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Titlebook: Astrobiology; The Quest for the Co Gerda Horneck,Christa Baumstark-Khan Book 2002 Springer-Verlag Berlin Heidelberg 2002 Habitat.astrobiolo

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31#
發(fā)表于 2025-3-26 23:47:07 | 只看該作者
32#
發(fā)表于 2025-3-27 03:38:54 | 只看該作者
Martian Atmospheric Evolution: Implications of an Ancient Intrinsic Magnetic Field00 nT during its low aerobreaking passes, resulting from remnant crustal magnetism. These magnetic anomalies strongly indicate the existence of a strong ancient intrinsic Martian magnetic moment, which corresponded to a magnetic field strength of 10% - 100% of present Earth’s.
33#
發(fā)表于 2025-3-27 05:36:38 | 只看該作者
https://doi.org/10.1007/978-3-642-59381-9Habitat; astrobiology; bioastronomy; biology; complexity; environment; evolution; exobiology; extraterrestri
34#
發(fā)表于 2025-3-27 11:05:30 | 只看該作者
978-3-642-63957-9Springer-Verlag Berlin Heidelberg 2002
35#
發(fā)表于 2025-3-27 14:51:14 | 只看該作者
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發(fā)表于 2025-3-27 20:26:00 | 只看該作者
http://image.papertrans.cn/b/image/163557.jpg
37#
發(fā)表于 2025-3-28 00:13:10 | 只看該作者
https://doi.org/10.1007/978-3-8348-9562-2e profound questions “How did life originate?”, “Are we alone in the Universe?”, and “What is the future of life on Earth and in the Universe?” The wide range in the contents of this volume indicates the rich and exciting subject matter of this field. Much of this content can be grouped into three m
38#
發(fā)表于 2025-3-28 02:11:26 | 只看該作者
https://doi.org/10.1007/978-3-8348-9562-2 can be divided in various different components with very different physical parameters, ranging from a very hot (10. K), dilute (<10. particles cm.) component heated by supernova explosions, which fills more than half of its volume, to molecular clouds with temperatures from 10 to 100 K and molecul
39#
發(fā)表于 2025-3-28 08:22:51 | 只看該作者
40#
發(fā)表于 2025-3-28 11:23:50 | 只看該作者
https://doi.org/10.1007/978-3-8348-9562-2stem. The HZ of distances between a main sequence star and an Earth-like planet is roughly defined as the range of mean orbital radii which imply moderate planetary surface temperatures suitable for the development and subsistence of carbon-based life. The latter precondition is usually taken as the
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