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  2. Water cluster - Wikipedia

    en.wikipedia.org/wiki/Water_cluster

    Detailed water models predict the occurrence of water clusters, as configurations of water molecules whose total energy is a local minimum. [6] [7] [8] Of particular interest are the cyclic clusters (H 2 O) n; these have been predicted to exist for n = 3 to 60. [9] [10] [11] At low temperatures, nearly 50% of water molecules are included in ...

  3. Extraterrestrial liquid water - Wikipedia

    en.wikipedia.org/wiki/Extraterrestrial_liquid_water

    Water is one of the simplest molecules, composed of one oxygen and two hydrogen atoms, and can be found in all celestial bodies of the solar system. However, water is only useful for life in a liquid state, and extraterrestrial water is commonly found as water vapor or ice. Liquid water also has several properties that are beneficial for lifeforms.

  4. List of interstellar and circumstellar molecules - Wikipedia

    en.wikipedia.org/wiki/List_of_interstellar_and...

    For example, radio astronomy is most sensitive to small linear molecules with a high molecular dipole. [3] The most common molecule in the Universe, H 2 ( molecular hydrogen ), is completely invisible to radio telescopes because it has no dipole; [ 3 ] its electronic transitions are too energetic for optical telescopes, so detection of H 2 ...

  5. Molecules in stars - Wikipedia

    en.wikipedia.org/wiki/Molecules_in_stars

    Stellar molecules are molecules that exist or form in stars. Such formations can take place when the temperature is low enough for molecules to form – typically around 6,000 K (5,730 °C; 10,340 °F) or cooler. [1] Otherwise the stellar matter is restricted to atoms and ions in the forms of gas or – at very high temperatures – plasma.

  6. Interstellar medium - Wikipedia

    en.wikipedia.org/wiki/Interstellar_medium

    Of the gas in the ISM, by number 91% of atoms are hydrogen and 8.9% are helium, with 0.1% being atoms of elements heavier than hydrogen or helium, [3] known as "metals" in astronomical parlance. By mass this amounts to 70% hydrogen, 28% helium, and 1.5% heavier elements.

  7. Molecular cloud - Wikipedia

    en.wikipedia.org/wiki/Molecular_cloud

    The discovery of the 21 cm line was the first step towards the technology that would allow astronomers to detect compounds and molecules in interstellar space. [3] Plaque commemorating the discovery of 21-cm radiation from the Milky Way. In 1951, two research groups nearly simultaneously discovered radio emission from interstellar neutral hydrogen.

  8. Outer space - Wikipedia

    en.wikipedia.org/wiki/Outer_space

    A number of molecules exist in interstellar space, which can form dust particles as tiny as 0.1 μm. [137] The tally of molecules discovered through radio astronomy is steadily increasing at the rate of about four new species per year.

  9. Water - Wikipedia

    en.wikipedia.org/wiki/Water

    Model of hydrogen bonds (1) between molecules of water. Because of its polarity, a molecule of water in the liquid or solid state can form up to four hydrogen bonds with neighboring molecules. Hydrogen bonds are about ten times as strong as the Van der Waals force that attracts molecules to each other