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Water on Earth, Properties of Water

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Water in the Universe

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 368))

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Abstract

Water has always played an important role for civilizations. Some ancient civilizations used complex systems to exploit the water supplies that were available to them. The role of water to civilizations like ancient Romans or Greek or ancient Egypt is reviewed in the first sections of this chapter. Water is a unique molecule and the special chemical and physical properties of it are explained. Water is a dipolar molecule which explains its special properties. Also the special phases of water are discussed amongst them the different properties of ices. Without these water would not play a substantial role for the evolution of life. Also the abundance of the constituents of water, hydrogen and oxygen in the universe is discussed.

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Notes

  1. 1.

    This value corresponds to 154 ppm, parts per million.

  2. 2.

    Because of the production of e that are also called β particles.

  3. 3.

    1 Light year ly denotes the distance that light travels within one year, 1 ly=1013 km.

  4. 4.

    Standard temperature and pressure (denoted as STP) refers to nominal conditions in the atmosphere at sea level. Standard temperature is 0°C, standard pressure denotes 760 mm in mercury barometer.

  5. 5.

    International Union of Pure and Applied Chemistry.

  6. 6.

    Benz, A., 2010, private communication.

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Correspondence to Arnold Hanslmeier .

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Hanslmeier, A. (2011). Water on Earth, Properties of Water. In: Water in the Universe. Astrophysics and Space Science Library, vol 368. Springer, Dordrecht. https://doi.org/10.1007/978-90-481-9984-6_1

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