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    carbon (C)

    carbon atom
    The fourth most common element in the universe (see elements, cosmic abundance) and the basis of all terrestrial life (see elements, biological abundance). Astrobiologists suspect that carbon-based life may be common through the universe. Given the unique ease with which carbon forms long, complex chains and rings, it is difficult (though not impossible) to imagine life with a different chemical basis such as silicon.


    Forms of carbon

    Carbon is found free in nature in three main allotropic forms: amorphous, graphite, and diamond. Graphite is one of the softest known materials while diamond is one of the hardest. Another recently-discovered form of carbon are fullerenes, which consist of large polyhedral molecules containing scores of carbon atoms, called buckyballs, or cylindrical molecules called carbon nanotubes. Carbon occurs as two stable isotopes, carbon-12 and carbon-13. A third isotope, carbon-14, is radioactive.


    atomic number 6
    relative atomic mass 12.0107
    electron configuration 1s22s22p4
    atomic radius 77 pm
    oxidation states 2, 4, -4
    relative density 2.25 (graphite), 3.52 (diamond)
    melting point 3,550 °C (6,422 °F)
    boiling point 3,825 °C (6,917 °F)


    Carbon and life

    Carbon is the basis of all life on Earth since it forms the backbone of DNA and proteins. The average adult human body contains about 16 kg of carbon in one form or another. Carbon is taken in by plants as carbon dioxide.


    The cosmic origins of carbon

    Carbon is manufactured inside the cores of evolved stars by a process that involves either a remarkable coincidence or a piece of cosmic tuning. In this process, two helium nuclei come together to make a nucleus of beryllium, which then has to capture a further helium nucleus to complete the synthesis of carbon. However, when the astrophysicist Fred Hoyle first looked closely at this reaction in the 1950s he realized there was a problem. According to what was then known, the capture of a helium nucleus by a beryllium nucleus was far too improbable to account for the observed cosmic abundance of carbon. He reasoned that the only way enough carbon could be made was if there existed a very specific match of nuclear energy levels, or resonance, between helium, beryllium, and carbon under precisely the conditions thought to prevail in the cores of stars at this stage in their evolution. Experiments promptly confirmed Hoyle's deduction – there was indeed a previously unsuspected resonance, very close to the energy value he gave. Crucially, for carbon-based life-forms, there is not a similar resonance at the same energy between carbon, helium, and oxygen. If there were, a large part of the carbon inside stars would quickly be changed into oxygen, and life as we know it would be impossible. These happy coincidences are cited by those who argue in favor of the anthropic principle, although Hoyle himself has put forward a more extreme interpretation:
    If you wanted to produce carbon and oxygen in roughly equal quantities by stellar nucleosynthesis, these are the two basic levels you would have to fix, and your fixing would have to be just about where these levels are actually found to be... A commonsense interpretation of the facts suggests that a superintellect has monkeyed with physics ... and that there are no blind forces worth speaking about in nature.

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    External site
    carbon (interactive periodic table)



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