Water in the UniverseDue to its specific chemical and physical properties, water is essential for life on Earth. And it is assumed that this would be the case for extraterrestrial life as well. Therefore it is important to investigate where water can be found in the Universe. Although there are places that are completely dry, places where the last rainfall happened probably several 100 million years ago, surprisingly this substance is quite omnipresent. In the outer solar system the large satellites of Jupiter and Saturn are covered by a thick layer of ice that could be hiding a liquid ocean below. This of course brings up the question of whether the recently detected extrasolar planets could have some water on their surfaces and how we can detect this. Water molecules are also found in interstellar gas and dust clouds. This book begins with an introductory chapter reviewing the physical and chemical properties of water. Then it illuminates the apparent connection between water and life. This is followed by chapters dealing with our current knowledge of water in the solar system, followed by a discussion concerning the potential presence and possible detection of water on exoplanets. The signature of water in interstellar space and stars are reviewed before the origin of water in the Universe is finally discussed. The book ends with an appendix on detection methods, satellite missions and astrophysical concepts touched upon in the main parts of the book. The search for water in the Universe is related to the search for extraterrestrial life and is of fundamental importance for astrophysics, astrobiology and other related topics. This book therefore addresses students and researchers in these fields. |
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Conteúdo
| 1 | |
| 25 | |
| 37 | |
| 71 | |
| 105 | |
Water on Extrasolar Planets? | 129 |
Water in Interstellar Space and Stars | 153 |
WaterWhere Does It Come from? | 181 |
Appendix | 199 |
References | 213 |
Index | 231 |
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absorption abundance accretion albedo ammonia asteroids atoms bright burning carbon Cassini chemical cometary comets core craters Credit density detected diameter disk distance dust Earth Earth’s atmosphere electrons elements energy Europa evolution extrasolar planets flux formation galactic galaxies giant planets gravitational habitable zone heat helium Hubble Space Telescope hydrogen impact infrared interstellar medium isotopes Jupiter Jupiter’s KBOs Kuiper belt layer liquid water luminosity lunar main sequence Mars martian mass massive stars meteorites methane million mission molecular Moon NASA nebula Neptune neutrons nuclei objects observed ocean Oort cloud orbital period oxygen particles planetary systems Pluto polar pole pressure protons protostar radiation radius reactions satellite Saturn solar system solar wind spacecraft spectra Spectrometer spectrum Springer Science+Business Media stellar supernova surface temperature Table Tauri stars Titan transition universe Uranus velocity Venus volcanic water ice water maser water molecules water vapor wavelengths
