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Gas C 2 H 5 OH −235.3 Glucose: Solid C 6 H 12 O 6: −1271 Isopropanol: Gas C 3 H 7 OH: −318.1 Methanol (methyl alcohol) Liquid CH 3 OH −238.4 Methanol (methyl alcohol) Gas CH 3 OH −201.0 Methyl linoleate Gas C 19 H 34 O 2: −356.3 Sucrose: Solid C 12 H 22 O 11: −2226.1 Trichloromethane Liquid CHCl 3: −134.47 Trichloromethane Gas ...
Oxygen gas is the second most common component of the Earth's atmosphere, taking up 20.8% of its volume and 23.1% of its mass (some 10 15 tonnes). [19] [70] [d] Earth is unusual among the planets of the Solar System in having such a high concentration of oxygen gas in its atmosphere: Mars (with 0.1% O 2 by volume) and Venus have much less. The O
A Assuming an altitude of 194 metres above mean sea level (the worldwide median altitude of human habitation), an indoor temperature of 23 °C, a dewpoint of 9 °C (40.85% relative humidity), and 760 mmHg sea level–corrected barometric pressure (molar water vapor content = 1.16%).
The standard Gibbs free energy of formation (G f °) of a compound is the change of Gibbs free energy that accompanies the formation of 1 mole of a substance in its standard state from its constituent elements in their standard states (the most stable form of the element at 1 bar of pressure and the specified temperature, usually 298.15 K or 25 ...
By convention, the (higher) heat of combustion is defined to be the heat released for the complete combustion of a compound in its standard state to form stable products in their standard states: hydrogen is converted to water (in its liquid state), carbon is converted to carbon dioxide gas, and nitrogen is converted to nitrogen gas. That is ...
Solid oxygen forms at normal atmospheric pressure at a temperature below 54.36 K (−218.79 °C, −361.82 °F). Solid oxygen O 2 , like liquid oxygen , is a clear substance with a light sky-blue color caused by absorption in the red part of the visible light spectrum.
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The formation of O 2 occurs in the gas phase via the neutral exchange reaction between • O and • HO, which is also the main sink for • HO in dense regions. [20] We can see that atomic oxygen takes part both in the production and destruction of • HO, so the abundance of • HO depends mainly on the H + 3 abundance.