Absorption Spectrum
If one condenses O2 gas via a cooling loop immersed in a liquid nitrogen trap (-196°C), it is possible to generate liquid oxygen. Bear some thoughts toward safety in doing this as (i) liquid oxygen is a cryogenic liquid, (ii) it is a potent oxidant and (iii) in liquid form is highly concentrated at 19M. (translation:- If something burning comes in contact with the liquid oxygen there could be a large explosion!) So that warning aside, the you then need a dewared cuvette and a spectrophotometer. |
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The electronic absorption spectrum of liquid oxygen is blue due to the 2 strong absorption bands at 630 and 577 nm. The electronic bands appearing in O2 are somewhat complex. The electronic state of the ground state is |
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It is obvious in the above spectrum that there are other bands in the electronic spectrum of O2 than the ground state The electronic configurations of oxygen is then explained in terms of a molecular orbital with the following schemes. |
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The ground state The first excited state |
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Potential Energy Diagram |
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Spectra of Diatomic Molecules (1950) G. Hertzberg |
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The above figure is the potential energy diagram of oxygen showing the electronic and vibrational energies. The "Spectra of Diatomic Molecules" source book has much of the information contained in the text described herein. A solar rainbow was seen to grace my desk above this open page one morning. So I could only imagine that it was meant to be included in this page.
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At higher energy it is also possible to excite electrons from the The absorption of O3 is strongest 240-270 nm and extends a further ±40 nm. This absorption feature, the "Hartley band" is the protective UV screening layer in the atmosphere. At wavelengths longer than 300 nm the Hartley band weakens and from 310-350 nm a temperature dependent band termed the Higgins band appears . |
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Astronomy of the Middle Atmosphere (1986) G. Brasseur and S. Solomon (Ed) |
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Atomic Oxygen Emissions : AuroraThe ionization of oxygen molecules in the atmosphere by UV radiation causes dissociation to oxygen atoms: O(1S), O(3P) or O(1D). These atoms then tend to emit their absorbed radiation via fluorescence and chemiluminescence from specific electronic transitions resulting in colourfull emission in the atmosphere . The emissions of oxygen species play an important role in the emissions of the Aurora and in the airglow of the night sky. The excited states of the oxygen are also important in atmospheric chemistry of O2 and O3. The strong red and green emissions in aurora arise from oxygen (OI) emissions which can be readily seen and photographed. Many other emissions are also detectable but may be very weak.
Aurora Emission Lines |
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