Deuterated methanol: Difference between revisions
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{{short description|Chemical compound}} |
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{{Unreferenced|date = February 2007}} |
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{{Chembox |
{{Chembox |
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| ImageFile = Deuterovaný methanol.jpg |
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| ImageFileR1 = Methanol-d4 3D spacefill.png |
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| ImageName = Stereo skeletal formula of deuterated methanol |
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| CASNo = 811-98-3 |
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| ImageName = |
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| PubChem = 71568 |
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| OtherNames = |
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| PubChem_Ref = {{Pubchemcite|correct|pubchem}} |
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| PIN = (<sup>2</sup>H<sub>3</sub>)Methan(<sup>2</sup>H)ol |
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| SystematicName = |
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| ChemSpiderID_Ref = {{chemspidercite|correct|chemspider}} |
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| CASNo = 811-98-3 |
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| PubChem = 71568 |
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| ChEBI = 156265 |
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| ChemSpiderID_Ref = {{chemspidercite|correct|chemspider}} |
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| UNNumber = 1230 |
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| StdInChI_Ref = {{stdinchicite|correct|chemspider}} |
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| Beilstein = 1733278 |
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| Density = 0.888 g cm<sup>-3</sup> |
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| Section3 = {{Chembox Thermochemistry |
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| Section3 = {{Chembox Thermochemistry |
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| EUClass = {{Hazchem F}} {{Hazchem T}} |
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| RPhrases = {{R11}}, {{R23/24/25}}, {{R39/23/24/25}} |
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| SPhrases = {{S7}}, {{S16}}, {{S36/37}}, {{S45}} |
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| GHSPictograms = {{GHS02}}{{GHS06}}{{GHS08}} |
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| GHSSignalWord = Warning |
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| HPhrases = {{H-phrases|225|301|311|331|370}} |
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| PPhrases = {{P-phrases|210|233|240|241|242|243|260|261|264|270|271|280|301+310|302+352|303+361+353|304+340|307+311|311|312|321|322|330|361|363|370+378|403+233|403+235|405|501}} |
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| Section5 = {{Chembox Related |
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'''Deuterated methanol''' (CD<sub>3</sub>OD), is a form (called an [[isotopologue]]) of [[methanol]] (CH<sub>3</sub>OH) in which the [[hydrogen]] |
'''Deuterated methanol''' (CD<sub>3</sub>OD), is a form (called an [[isotopologue]]) of [[methanol]] (CH<sub>3</sub>OH) in which the [[hydrogen]] atoms ("H") are replaced with [[deuterium]] (heavy hydrogen) [[isotope]] ("D").<ref>{{Cite journal |last1=Bizzocchi |first1=L. |last2=Caselli |first2=P. |last3=Spezzano |first3=S. |last4=Leonardo |first4=E. |date=2014-09-01 |title=Deuterated methanol in the pre-stellar core L1544 |url=https://www.aanda.org/articles/aa/abs/2014/09/aa23858-14/aa23858-14.html |journal=Astronomy & Astrophysics |language=en |volume=569 |pages=A27 |doi=10.1051/0004-6361/201423858 |issn=0004-6361|doi-access=free |arxiv=1408.2491 |bibcode=2014A&A...569A..27B }}</ref> Deuterated methanol is a common [[solvent]] used in [[NMR spectroscopy]]. |
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Deuterated methanol was first detected in [[interstellar space]] was [[Orion-KL]] in 1988 by scientists at the [[Max Planck Institute for Radio Astronomy]].<ref>{{Cite journal |last1=Mauersberger |first1=R. |last2=Henkel |first2=C. |last3=Jacq |first3=T. |last4=Walmsley |first4=C. M. |date=1988-04-01 |title=Deuterated methanol in Orion. |url=https://ui.adsabs.harvard.edu/abs/1988A&A...194L...1M |journal=Astronomy and Astrophysics |volume=194 |pages=L1–L4 |bibcode=1988A&A...194L...1M |issn=0004-6361}}</ref> |
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== References == |
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{{Reflist}} |
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{{List of NMR solvents}} |
{{List of NMR solvents}} |
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[[Category:Deuterated |
[[Category:Deuterated solvents]] |
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[[Category:Methanol]] |
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{{NMR-stub}} |
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Latest revision as of 15:38, 2 May 2024
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Names | |||
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Preferred IUPAC name
(2H3)Methan(2H)ol | |||
Identifiers | |||
3D model (JSmol)
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1733278 | |||
ChEBI | |||
ChemSpider | |||
ECHA InfoCard | 100.011.253 | ||
EC Number |
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PubChem CID
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UN number | 1230 | ||
CompTox Dashboard (EPA)
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Properties | |||
CD4O | |||
Molar mass | 36.0665 g mol−1 | ||
Density | 0.888 g cm−3 | ||
Melting point | −98 °C (−144 °F; 175 K) | ||
Boiling point | 65 °C (149 °F; 338 K) | ||
Thermochemistry | |||
Heat capacity (C)
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87.9 J K−1 mol−1 | ||
Hazards | |||
GHS labelling: | |||
Warning | |||
H225, H301, H311, H331, H370 | |||
P210, P233, P240, P241, P242, P243, P260, P261, P264, P270, P271, P280, P301+P310, P302+P352, P303+P361+P353, P304+P340, P307+P311, P311, P312, P321, P322, P330, P361, P363, P370+P378, P403+P233, P403+P235, P405, P501 | |||
Flash point | 11 °C (52 °F; 284 K) | ||
Related compounds | |||
Related compounds
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Methanol | ||
Except where otherwise noted, data are given for materials in their standard state (at 25 °C [77 °F], 100 kPa).
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Deuterated methanol (CD3OD), is a form (called an isotopologue) of methanol (CH3OH) in which the hydrogen atoms ("H") are replaced with deuterium (heavy hydrogen) isotope ("D").[1] Deuterated methanol is a common solvent used in NMR spectroscopy.
Deuterated methanol was first detected in interstellar space was Orion-KL in 1988 by scientists at the Max Planck Institute for Radio Astronomy.[2]
References
[edit]- ^ Bizzocchi, L.; Caselli, P.; Spezzano, S.; Leonardo, E. (2014-09-01). "Deuterated methanol in the pre-stellar core L1544". Astronomy & Astrophysics. 569: A27. arXiv:1408.2491. Bibcode:2014A&A...569A..27B. doi:10.1051/0004-6361/201423858. ISSN 0004-6361.
- ^ Mauersberger, R.; Henkel, C.; Jacq, T.; Walmsley, C. M. (1988-04-01). "Deuterated methanol in Orion". Astronomy and Astrophysics. 194: L1–L4. Bibcode:1988A&A...194L...1M. ISSN 0004-6361.