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  2. Astrochemistry - Wikipedia

    en.wikipedia.org/wiki/Astrochemistry

    Astrochemistry is the study of the abundance and reactions of molecules in the universe, and their interaction with radiation. [1] The discipline is an overlap of astronomy and chemistry . The word "astrochemistry" may be applied to both the Solar System and the interstellar medium .

  3. List of interstellar and circumstellar molecules - Wikipedia

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

    The discipline of astrochemistry includes understanding how these molecules form and explaining their abundances. The extremely low density of the interstellar medium is not conducive to the formation of molecules, making conventional gas-phase reactions between neutral species (atoms or molecules) inefficient.

  4. David Williams (astrochemist) - Wikipedia

    en.wikipedia.org/wiki/David_Williams_(astrochemist)

    Professor Williams field of study is astrochemistry, involving the study of molecular line emissions in outer space to analyse and interpret the evolutionary process of the universe. He led research groups at both Manchester and London and produced more than 300 publications in journals and books.

  5. File:Map of Roblox restrictions by country.svg - Wikipedia

    en.wikipedia.org/wiki/File:Map_of_Roblox...

    This map is ineligible for copyright and therefore in the public domain, because it consists entirely of information that is common property and contains no original authorship. For more information, see Commons:Threshold of originality § Maps .

  6. Cosmochemistry - Wikipedia

    en.wikipedia.org/wiki/Cosmochemistry

    Meteorites are often studied as part of cosmochemistry. Cosmochemistry (from Ancient Greek κόσμος (kósmos) 'universe' and χημεία (khēmeía) 'chemistry') or chemical cosmology is the study of the chemical composition of matter in the universe and the processes that led to those compositions. [1]

  7. Atomic and molecular astrophysics - Wikipedia

    en.wikipedia.org/wiki/Atomic_and_molecular...

    Within a few million years the light from bright stars will have boiled away this molecular cloud of gas and dust. The cloud has broken off from the Carina Nebula.Newly formed stars are visible nearby, their images reddened by blue light being preferentially scattered by the pervasive dust.

  8. Karin Öberg - Wikipedia

    en.wikipedia.org/wiki/Karin_Öberg

    On April 9, 2015, the Öberg Astrochemistry Group published a paper stating they detected the first complex carbon molecule in a protoplanetary disk, this molecule being methyl cyanide. [ 2 ] [ 5 ] Methyl cyanide (CH 3 CN) is thought to be important for the origins of life because it contains carbon-nitrogen bonds , which make up amino acids ...

  9. Cosmic ray astronomy - Wikipedia

    en.wikipedia.org/wiki/Cosmic_ray_astronomy

    Cosmic ray astronomy is a branch of observational astronomy where scientists attempt to identify and study the potential sources of extremely high-energy (ranging from 1 MeV to more than 1 EeV) charged particles called cosmic rays coming from outer space.