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Energy and Its Biological Resources  37


           1.16  Hydrogen
           The simplest of the elements, containing a single proton and electron
           each, of mass almost unity, is the first member of the periodic table.
           Data may vary from different sources; solid at 4.2 K (d 0.089), H has
           the atomic number (AN) 1, atomic weight (AW) 1.008 g, melting point
           (mp)  259.14 C, and boiling point (bp)  252.87 C (d 0.071 at 20.4 K).
           He has a AN 2, AW 4.0026 g, mp  272.2 C (20 atm), and bp  268.93 C
           (specific gravity 0.124).
             Commercial consumption at present is mostly in synthetic fuels, say
           from coal, mineral oils, petroleum reformation (refineries), and iron and
           copper ore reductions. Hydrogen is very important because of the ver-
           satility of its physical, chemical, and biological properties. More impor-
           tantly for our purposes, is its potential as a source of energy. Hydrogen
           liquefies at 33.2 K, 12.8 atm, and 0.03 g/mL and occupies a negligible
           volume (22.4 times less), compared to its gaseous state. Solid hydrogen
           and helium are academic ideas. When hydrogen combines with oxygen
           in a volume ratio of 2:1, heat is generated and the product is water in
           a vapor state. The reaction in a vapor state occurs with a reduction of
                                               1
                     1
           volume to  / 3 and water vapor to water  / 22, which means the reaction is
           favored at a higher pressure; alternatively, the change in volume is
           compensated by utilizing some of the heat that evolves. The calculations
           are already there. Hydrogen as a combustion fuel or as a material for a
           fuel cell is less attractive than the fusion reaction such as that which
           occurs in the sun. Taking it as a model, we may be able to harness huge
           amounts of thermal and traditional energies, but we should also learn
           how to manage and handle such enormous outbursts of energy. Two
           protons fuse to yield a deuterium, a positron, and a neutrino; the last
           one is the clue to the release of energy that is not yet fully understood
           by science;

                                           1

                 1
                                     2
                                                           3
                                                3
                                                                  4
              2H → e     H     2    H   H → H            2H → He   2H   1
                                                                           2
                                                       33
                                      2
           Solar constant   1.968 cal/(cm 
 min)   3.86   10 erg/s   1.373 kW/m ;
           even at such a long distance, we are unable to use all the energies.
             Hydrogen in absence of air or oxygen, or in vacuum, will not burn, but
           may have a kind of combustion to produce ammonia in air or nitrogen.
           Combustion of hydrogen in our atmosphere does not produce simple
                                                                (nitrogen and
           water vapor, but mixture of others, i.e., ammonia and NO xS
           oxygen combine at the vicinity of high temperature generated).
             Cryogenic and space research have taught us many more lessons.
           Liquid hydrogen can be stored in special containers (cylinders), or trans-
           ported through pipes, and is almost an ideal fuel for rockets and space-
           ships, perhaps next to azides. But at higher altitudes or in space, in the
           absence of atmosphere, optimal liquid oxygen is also needed to perform
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