Hydroxy group
In
, consist of an unbonded hydroxy group.According to IUPAC definitions, the term hydroxyl refers to the hydroxyl radical (·OH) only, while the functional group −OH is called a hydroxy group.[1]
Properties
Water, alcohols,
Occurrence
The hydroxy group is pervasive in chemistry and biochemistry. Many inorganic compounds contain hydroxyl groups, including sulfuric acid, the chemical compound produced on the largest scale industrially.[2]
Hydroxy groups participate in the dehydration reactions that link simple biological molecules into long chains. The joining of a
Hydroxyl radical
Hydroxyl radicals are highly reactive and undergo chemical reactions that make them short-lived. When biological systems are exposed to hydroxyl radicals, they can cause damage to cells, including those in humans, where they can react with DNA, lipids, and proteins.[4]
Planetary observations
Airglow of the Earth
The Earth's night sky is illuminated by diffuse light, called airglow, that is produced by radiative transitions of atoms and molecules.[5] Among the most intense such features observed in the Earth's night sky is a group of infrared transitions at wavelengths between 700 nanometers and 900 nanometers. In 1950, Aden Meinel showed that these were transitions of the hydroxyl molecule, OH.[6]
Surface of the Moon
In 2009, India's
On 26 October 2020,
The Chang'e 5 probe, which landed on the Moon on 1 December 2020, carried a mineralogical spectrometer that could measure infrared reflectance spectra of lunar rock and regolith. The reflectance spectrum of a rock sample at a wavelength of 2.85 micrometers indicated localized water/hydroxyl concentrations as high as 180 parts per million.[11]
Atmosphere of Venus
The Venus Express orbiter collected Venus science data from April 2006 until December 2014. In 2008, Piccioni, et al. reported measurements of night-side airglow emission in the atmosphere of Venus made with the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) on Venus Express. They attributed emission bands in wavelength ranges of 1.40 - 1.49 micrometers and 2.6 - 3.14 micrometers to vibrational transitions of OH.[12] This was the first evidence for OH in the atmosphere of any planet other than Earth's.[12]
Atmosphere of Mars
In 2013, OH near-infrared spectra were observed in the night glow in the polar winter atmosphere of Mars by use of the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM).[13]
Exoplanets
In 2021, evidence for OH in the dayside atmosphere of the exoplanet
See also
References
- . Retrieved 23 March 2015.
- ^ "Research Report 2012 – 2013" (PDF). Ludwig Maximilians Universität München Fakultät für Chemie und Pharmazie. 12. Archived from the original (PDF) on Dec 7, 2022.
- ^ "Peptide Bond - an overview". ScienceDirect Topics. Archived from the original on 2022-10-20. Retrieved 2022-10-20.
- PMID 22798706.
- from the original on Oct 5, 2023.
- doi:10.1086/145296. Archivedfrom the original on Oct 24, 2022.
- ^ Kerr RA (24 September 2009). "A Whiff of Water Found on the Moon". Science. Archived from the original on Dec 8, 2023. Retrieved 2016-06-01.
- ^ Dino J (13 November 2009). "LCROSS Impact Data Indicates Water on Moon". NASA. Archived from the original on 2009-11-15. Retrieved 2009-11-14.
- S2CID 228954129.
- ^ Chou F, Hawkes A (26 October 2020). "NASA's SOFIA Discovers Water on Sunlit Surface of Moon". NASA. Retrieved 2020-10-26.
- PMID 34995111.
- ^ ISSN 0004-6361.
- .
- S2CID 232110452.
- S2CID 239616465.
Further
- Reece J, Urry L, Cain M, Wasserman S, Minorsky P, Jackson R (2011). "Chapter 4&5". In Berge S, Golden B, Triglia L (eds.). Campbell Biology. Vol. Unit 1 (9th ed.). San Francisco: Pearson Benjamin Cummings. ISBN 978-0-321-55823-7.