Reducing atmosphere

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A reducing atmosphere is an atmospheric condition in which oxidation is prevented by removal of oxygen and other oxidizing gases or vapours, and which may contain actively reducing gases such as hydrogen, carbon monoxide, and gases such as hydrogen sulfide that would be oxidized by any present oxygen.

Metal processing[edit]

In metal processing, a reducing atmosphere is used in annealing ovens for relaxation of metal stresses without corroding the metal. A non-oxidizing gas, usually nitrogen or argon, is typically used as a carrier gas so that diluted amounts of reducing gases may be used. Typically, this is achieved through using the combustion products of fuels and tailoring the ratio of CO:CO2. However, other common reducing atmospheres in the metal processing industries consist of dissociated ammonia, vacuum, and/or direct mixing of appropriately pure gases of N2, Ar, and H2.[1]

A reducing atmosphere is also used to produce specific effects on ceramic wares being fired. A reduction atmosphere is produced in a fuel fired kiln by reducing the draft and depriving the kiln of oxygen. This diminished level of oxygen causes incomplete combustion of the fuel and raises the level of carbon inside the kiln. At high temperatures the carbon will bond with and remove the oxygen in the metal oxides used as colorants in the glazes. This loss of oxygen results in a change in the color of the glazes because it allows the metals in the glaze to be seen in an unoxidized form. A reduction atmosphere can also affect the color of the clay body. If iron is present in the clay body, as it is in most stoneware, then it will be affected by the reduction atmosphere as well.

In most commercial incinerators, exactly the same conditions are created to encourage the release of carbon bearing fumes. These fumes are then oxidized in reburn tunnels where oxygen is injected progressively. The exothermic oxidation reaction maintains the temperature of the reburn tunnels. This system allows lower temperatures to be employed in the incinerator section, where the solids are volumetrically reduced.

Planetary atmospheres[edit]

The same principle applies to planets. Many scientists[weasel words] think the early Earth had a reducing atmosphere, along with Mars, Venus and Titan. This would have proven to be a good environment for cyanobacteria to evolve the first photosynthetic metabolic pathways which gradually increased the oxygen portion of the atmosphere, changing it to what is known as an oxidizing atmosphere. With increased levels of oxygen, the evolution of the more efficient aerobic respiration might have been enabled, allowing animal life to evolve and thrive.[2]

Though most scientists conceive of the early atmosphere as reducing, a 2011 article in Nature found that cerium oxidation in zircon—which comprises the oldest rocks on Earth at roughly 4.4 billion years of age—was comparable to that of present-day lava. This observation implies that Hadean atmospheric oxygen levels were similar to those of today.[3]

The research raises questions about how the jump from inorganic compounds to life-supporting amino acids and DNA occurred on earth and suggests those building blocks were delivered from elsewhere in the galaxy. The results however do not run contrary to existing theories on life's journey from anaerobic to aerobic organisms. The results quantify the nature of gas molecules containing carbon, hydrogen, and sulphur in the earliest atmosphere, but they shed no light on the much later rise of free oxygen in the air.[4]

Although a hard vacuum, interplanetary space is reducing because solar wind consists mostly of hydrogen plasma. The Moon is directly exposed to solar wind, such that sodium is reduced and evaporated to produce the sodium tail of the Moon (see atmosphere of the Moon).

See also[edit]


  1. ^ Koria, S. C. "Fuels Refractory and Furnaces" (PDF). Indian Institute of Technology Kanpur. Retrieved 28 December 2018 – via National Programme on Technology Enhanced Learning.
  2. ^ Gribbin, J. (1995-12-09). "Structure of the Earth's atmosphere". New Scientist, 2007. p. 1.
  3. ^ Trail, Dustin; Watson, E. Bruce; Tailby, Nicholas D. (2011). "The oxidation state of Hadean magmas and implications for early Earth's atmosphere". Nature. 480 (7375): 79–82. Bibcode:2011Natur.480...79T. doi:10.1038/nature10655. PMID 22129728. S2CID 4338830.
  4. ^ "Earth's Early Atmosphere: An Update". NASA Astrobiology Institute.