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Hydrogen cyanide
Chemical compound

Hydrogen cyanide (HCN), formerly called prussic acid, is a chemical compound with the formula HCN and structural formula H−C≡N. It is a highly toxic and flammable liquid that boils just above room temperature at 25.6 °C (78.1 °F). Industrially important as a precursor to compounds like potassium cyanide and adiponitrile, it is more toxic than solid cyanides due to its volatile nature. Its aqueous form, HCN(aq), is known as hydrocyanic acid. Whether HCN is an organic compound is debated, but it belongs to the nitriles class, with hydrogen as the R group, also called methanenitrile or formonitrile.

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Structure and general properties

Hydrogen cyanide is a linear molecule, with a triple bond between carbon and nitrogen. The tautomer of HCN is HNC, hydrogen isocyanide.

Smell

Much literature has historically claimed that hydrogen cyanide smells of almonds or bitter almonds. However, there has been considerable confusion and disagreement over this, because the smell of household almond essence is due to benzaldehyde, which is released along with hydrogen cyanide from the breakdown of amygdalin present in some plant seeds, and thus is often mistaken for it.45

About half of people are unable to detect the smell of hydrogen cyanide owing to a recessive genetic trait.6

The volatile compound has been used as inhalation rodenticide and human poison, as well as for killing whales.7 Cyanide ions interfere with iron-containing respiratory enzymes.

Chemical properties

Hydrogen cyanide is weakly acidic with a pKa of 9.2. It partially ionizes in water to give the cyanide anion, CN−. HCN forms hydrogen bonds with its conjugate base, species such as (CN−)(HCN)n.8

Hydrogen cyanide reacts with alkenes to give nitriles. The conversion, which is called hydrocyanation, employs nickel complexes as catalysts.9

RCH=CH2 + HCN → RCH2−CH2CN

Four molecules of HCN will tetramerize into diaminomaleonitrile.10

Metal cyanides are typically prepared by salt metathesis from alkali metal cyanide salts, but mercuric cyanide is formed from aqueous hydrogen cyanide:11

HgO + 2 HCN → Hg(CN)2 + H2O

History of discovery and naming

Hydrogen cyanide was first isolated in 1752 by French chemist Pierre Macquer who converted Prussian blue to an iron oxide plus a volatile component and found that these could be used to reconstitute it.12 The new component was what is now known as hydrogen cyanide. It was subsequently prepared from Prussian blue by the Swedish chemist Carl Wilhelm Scheele in 1782,13 and was eventually given the German name Blausäure (lit. "Blue acid") because of its acidic nature in water and its derivation from Prussian blue. In English, it became known popularly as prussic acid.

In 1787, the French chemist Claude Louis Berthollet showed that prussic acid did not contain oxygen,14 an important contribution to acid theory, which had hitherto postulated that acids must contain oxygen15 (hence the name of oxygen itself, which is derived from Greek elements that mean "acid-former" and are likewise calqued into German as Sauerstoff).

In 1811, Joseph Louis Gay-Lussac prepared pure, liquified hydrogen cyanide,16 and in 1815 he deduced Prussic acid's chemical formula.17

Etymology

The word cyanide for the radical in hydrogen cyanide was derived from its French equivalent, cyanure, which Gay-Lussac constructed from the Ancient Greek word κύανος for dark blue enamel or lapis lazuli, again owing to the chemical’s derivation from Prussian blue. Incidentally, the Greek word is also the root of the English color name cyan.

Production and synthesis

The most important process is the Andrussow oxidation invented by Leonid Andrussow at IG Farben in which methane and ammonia react in the presence of oxygen at about 1,200 °C (2,190 °F) over a platinum catalyst:18

2 CH4 + 2 NH3 + 3 O2 → 2 HCN + 6 H2O

In 2006, between 500 million and 1 billion pounds (between 230,000 and 450,000 t) were produced in the US.19 Hydrogen cyanide is produced in large quantities by several processes and is a recovered waste product from the manufacture of acrylonitrile.20

Of lesser importance is the Degussa process (BMA process) in which no oxygen is added and the energy must be transferred indirectly through the reactor wall:21

CH4 + NH3 → HCN + 3H2

This reaction is akin to steam reforming, the reaction of methane and water to give carbon monoxide and hydrogen.

In the Shawinigan Process, hydrocarbons, e.g. propane, are reacted with ammonia.

In the laboratory, small amounts of HCN are produced by the addition of acids to cyanide salts of alkali metals:

H+ + CN− → HCN

This reaction is sometimes the basis of accidental poisonings because the acid converts a nonvolatile cyanide salt into the gaseous HCN.

Hydrogen cyanide could be obtained from potassium ferricyanide and acid:

6 H+ + [Fe(CN)6]−3 → 6 HCN + Fe+32223

Historical methods of production

The large demand for cyanides for mining operations in the 1890s was met by George Thomas Beilby, who patented a method to produce hydrogen cyanide by passing ammonia over glowing coal in 1892. This method was used until Hamilton Castner in 1894 developed a synthesis starting from coal, ammonia, and sodium yielding sodium cyanide, which reacts with acid to form gaseous HCN.

Applications

HCN is the precursor to sodium cyanide and potassium cyanide, which are used mainly in gold and silver mining and for the electroplating of those metals. Via the intermediacy of cyanohydrins, a variety of useful organic compounds are prepared from HCN including the monomer methyl methacrylate, from acetone, the amino acid methionine, via the Strecker synthesis, and the chelating agents EDTA and NTA. Via the hydrocyanation process, HCN is added to butadiene to give adiponitrile, a precursor to Nylon-6,6.24

HCN is used globally as a fumigant against many species of pest insects that infest food production facilities. Both its efficacy and method of application lead to very small amounts of the fumigant being used compared to other toxic substances used for the same purpose.25 Using HCN as a fumigant also has less environmental impact, compared to some other fumigants such as sulfuryl fluoride,26 and methyl bromide.27

Occurrence

HCN is obtainable from fruits that have a pit, such as cherries, apricots, apples, and nuts such as bitter almonds, from which almond oil and extract is made. Many of these pits contain small amounts of cyanohydrins such as mandelonitrile and amygdalin, which slowly release hydrogen cyanide.2829 One hundred grams of crushed apple seeds can yield about 70 mg of HCN.30 The roots of cassava plants contain cyanogenic glycosides such as linamarin, which decompose into HCN in yields of up to 370 mg per kilogram of fresh root.31 Some millipedes, such as Harpaphe haydeniana, Desmoxytes purpurosea, and Apheloria release hydrogen cyanide as a defense mechanism,32 as do certain insects, such as burnet moths and the larvae of Paropsisterna eucalyptus.33 Hydrogen cyanide is contained in the exhaust of vehicles, and in smoke from burning nitrogen-containing plastics.

On Titan

HCN has been measured in Titan's atmosphere by four instruments on the Cassini space probe, one instrument on Voyager, and one instrument on Earth.34 One of these measurements was in situ, where the Cassini spacecraft dipped between 1,000 and 1,100 km (620 and 680 mi) above Titan's surface to collect atmospheric gas for mass spectrometry analysis.35 HCN initially forms in Titan's atmosphere through the reaction of photochemically produced methane and nitrogen radicals which proceed through the H2CN intermediate, e.g., (CH3 + N → H2CN + H → HCN + H2).3637 Ultraviolet radiation breaks HCN up into CN + H; however, CN is efficiently recycled back into HCN via the reaction CN + CH4 → HCN + CH3.38

On the young Earth

It has been postulated that carbon from a cascade of asteroids (known as the Late Heavy Bombardment), resulting from interaction of Jupiter and Saturn, blasted the surface of young Earth and reacted with nitrogen in Earth's atmosphere to form HCN.39

In mammals

Some authors[who?] have shown that neurons can produce hydrogen cyanide upon activation of their opioid receptors by endogenous or exogenous opioids. They have also shown that neuronal production of HCN activates NMDA receptors and plays a role in signal transduction between neuronal cells (neurotransmission). Moreover, increased endogenous neuronal HCN production under opioids was seemingly needed for adequate opioid analgesia, as analgesic action of opioids was attenuated by HCN scavengers. They considered endogenous HCN to be a neuromodulator.40

It has also been shown that, while stimulating muscarinic cholinergic receptors in cultured pheochromocytoma cells increases HCN production, in a living organism (in vivo) muscarinic cholinergic stimulation actually decreases HCN production.41

Leukocytes generate HCN during phagocytosis, and can kill bacteria, fungi, and other pathogens by generating several different toxic chemicals, one of which is hydrogen cyanide.42

The vasodilatation caused by sodium nitroprusside has been shown to be mediated not only by NO generation, but also by endogenous cyanide generation, which adds not only toxicity, but also some additional antihypertensive efficacy compared to nitroglycerine and other non-cyanogenic nitrates which do not cause blood cyanide levels to rise.43

HCN is a constituent of tobacco smoke.44

HCN and the origin of life

Hydrogen cyanide has been discussed as a precursor to amino acids and nucleic acids, and is proposed to have played a part in the origin of life.45 Although the relationship of these chemical reactions to the origin of life theory remains speculative, studies in this area have led to discoveries of new pathways to organic compounds derived from the condensation of HCN (e.g. Adenine).46 Because amino acids are critical for life as we know it, and that hydrogen cyanide is a precursor for these molecules, astronomers who search for life on planets beyond Earth use spectroscopy to detect molecules like hydrogen cyanide after confirming suitable temperatures and the presence of water. 47

In space

See also: Astrochemistry

HCN has been detected in the interstellar medium48 and in the atmospheres of carbon stars.49 Since then, extensive studies have probed formation and destruction pathways of HCN in various environments and examined its use as a tracer for a variety of astronomical species and processes. HCN can be observed from ground-based telescopes through a number of atmospheric windows.50 The J=1→0, J=3→2, J= 4→3, and J=10→9 pure rotational transitions have all been observed.515253

HCN is formed in interstellar clouds through one of two major pathways:54 via a neutral-neutral reaction (CH2 + N → HCN + H) and via dissociative recombination (HCNH+ + e− → HCN + H). The dissociative recombination pathway is dominant by 30%; however, the HCNH+ must be in its linear form. Dissociative recombination with its structural isomer, H2NC+, exclusively produces hydrogen isocyanide (HNC).

HCN is destroyed in interstellar clouds through a number of mechanisms depending on the location in the cloud.55 In photon-dominated regions (PDRs), photodissociation dominates, producing CN (HCN + ν → CN + H). At further depths, photodissociation by cosmic rays dominate, producing CN (HCN + cr → CN + H). In the dark core, two competing mechanisms destroy it, forming HCN+ and HCNH+ (HCN + H+ → HCN+ + H; HCN + HCO+ → HCNH+ + CO). The reaction with HCO+ dominates by a factor of ~3.5. HCN has been used to analyze a variety of species and processes in the interstellar medium. It has been suggested as a tracer for dense molecular gas5657 and as a tracer of stellar inflow in high-mass star-forming regions.58 Further, the HNC/HCN ratio has been shown to be an excellent method for distinguishing between PDRs and X-ray-dominated regions (XDRs).59

On 11 August 2014, astronomers released studies, using the Atacama Large Millimeter/Submillimeter Array (ALMA) for the first time, that detailed the distribution of HCN, HNC, H2CO, and dust inside the comae of comets C/2012 F6 (Lemmon) and C/2012 S1 (ISON).6061

In February 2016, it was announced that traces of hydrogen cyanide were found in the atmosphere of the hot Super-Earth 55 Cancri e with NASA's Hubble Space Telescope.62

On 14 December 2023, astronomers reported the first time discovery, in the plumes of Enceladus, moon of the planet Saturn, of hydrogen cyanide, a possible chemical essential for life63 as we know it, as well as other organic molecules, some of which are yet to be better identified and understood. According to the researchers, "these [newly discovered] compounds could potentially support extant microbial communities or drive complex organic synthesis leading to the origin of life."6465

As a poison and chemical weapon

Main article: Cyanide poisoning

In World War I, hydrogen cyanide was used by the French from 1916 as a chemical weapon against the Central Powers, and by the United States and Italy in 1918. It was not found to be effective enough due to weather conditions.6667 The gas is lighter than air and rapidly disperses up into the atmosphere. Rapid dilution made its use in the field impractical. In contrast, denser agents such as phosgene or chlorine tended to remain at ground level and sank into the trenches of the Western Front's battlefields. Compared to such agents, hydrogen cyanide had to be present in higher concentrations in order to be fatal.

A hydrogen cyanide concentration of 100–200 ppm in breathing air will kill a human within 10 to 60 minutes.68 A hydrogen cyanide concentration of 2000 ppm (about 2380 mg/m3) will kill a human in about one minute.69 The toxic effect is caused by the action of the cyanide ion, which halts cellular respiration. It acts as a non-competitive inhibitor for an enzyme in mitochondria called cytochrome c oxidase. As such, hydrogen cyanide is commonly listed among chemical weapons as a blood agent.70

The Chemical Weapons Convention lists it under Schedule 3 as a potential weapon which has large-scale industrial uses. Signatory countries must declare manufacturing plants that produce more than 30 metric tons per year, and allow inspection by the Organisation for the Prohibition of Chemical Weapons.

Perhaps its most infamous use is Zyklon B (German: Cyclone B, with the B standing for Blausäure – prussic acid; also, to distinguish it from an earlier product later known as Zyklon A),71 used in the Nazi German extermination camps of Majdanek and Auschwitz-Birkenau during World War II to kill Jews and other persecuted minorities en masse as part of their Final Solution genocide program. Hydrogen cyanide was also used in the camps for delousing clothing in attempts to eradicate diseases carried by lice and other parasites. One of the original Czech producers continued making Zyklon B under the trademark "Uragan D2"72 until around 2015.73

During World War II, the US considered using it, along with cyanogen chloride, as part of Operation Downfall, the planned invasion of Japan, but President Harry Truman decided against it, instead using the atomic bombs developed by the secret Manhattan Project.74

Hydrogen cyanide was also the agent employed in judicial execution in some U.S. states, where it was produced during the execution by the action of sulfuric acid on sodium cyanide or potassium cyanide.75

Under the name prussic acid, HCN has been used as a killing agent in whaling harpoons, though it was quickly abandoned for being dangerous to the crew.76 From the middle of the 18th century it was used in a number of poisoning murders and suicides.77

Hydrogen cyanide gas in air is explosive at concentrations above 5.6%.78

References

  1. Gail, E.; Gos, S.; Kulzer, R.; Lorösch, J.; Rubo, A.; Sauer, M. "Cyano Compounds, Inorganic". Ullmann's Encyclopedia of Industrial Chemistry. Weinheim: Wiley-VCH. doi:10.1002/14356007.a08_159.pub2. ISBN 978-3-527-30673-2. 978-3-527-30673-2

  2. "Human Metabolome Database: Showing metabocard for Hydrogen cyanide (HMDB0060292)". https://hmdb.ca/metabolites/HMDB0060292

  3. "Hydrogen Cyanide". PubChem. National Center for Biotechnology Information. https://pubchem.ncbi.nlm.nih.gov/compound/768

  4. "How do people know HCN smells like almonds?". https://chemistry.stackexchange.com/questions/47204/how-do-people-know-hcn-smells-like-almonds

  5. "Do almonds smell like they do because of cyanide?". https://chemistry.stackexchange.com/questions/80564/do-almonds-smell-like-they-do-because-of-cyanide

  6. "Cyanide, inability to smell". Online Mendelian Inheritance in Man. Retrieved 2010-03-31. https://www.ncbi.nlm.nih.gov/omim/304300

  7. Lytle T. "Poison Harpoons". Whalecraft.net. Archived from the original on 2019-02-15. https://web.archive.org/web/20190215100154/http://www.whalecraft.net/Poison_Irons.html

  8. Bläsing, Kevin; Harloff, Jörg; Schulz, Axel; Stoffers, Alrik; Stoer, Philip; Villinger, Alexander (2020). "Salts of HCN-Cyanide Aggregates: [CN(HCN)2]− and [CN(HCN)3]−". Angewandte Chemie International Edition. 59 (26): 10508–10513. doi:10.1002/anie.201915206. PMC 7317722. PMID 32027458. https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7317722

  9. Leeuwen, P. W. N. M. van (2004). Homogeneous Catalysis: Understanding the Art. Dordrecht: Kluwer Academic Publishers. ISBN 1402019998. OCLC 54966334. 1402019998

  10. Ferris, J. P.; Sanchez, R. A. (1968). "Diaminomaleonitrile (Hydrogen Cyanide Tetramer)". Organic Syntheses. 48: 60. doi:10.15227/orgsyn.048.0060. /wiki/Doi_(identifier)

  11. F. Wagenknecht; R. Juza (1963). "Mercury (II) cyanide". In G. Brauer (ed.). Handbook of Preparative Inorganic Chemistry. Vol. 2 (2nd ed.). NY, NY: Academic Press.

  12. Macquer PJ (1756). "Éxamen chymique de bleu de Prusse" [Chemical examination of Prussian blue]. Mémoires de l'Académie royale des Sciences (in French): 60–77. /wiki/Pierre_Macquer

  13. Scheele CW (1782). "Försök, beträffande det färgande ämnet uti Berlinerblå" [Experiment concerning the coloring substance in Berlin blue]. Kungliga Svenska Vetenskapsakademiens Handlingar (Royal Swedish Academy of Science's Proceedings (in Swedish). 3: 264–275. Reprinted in Latin as: Scheele CW, Hebenstreit EB, eds. (1789). "De materia tingente caerulei berolinensis". Opuscula Chemica et Physica [The dark matter tingente caerulei berolinensis] (in Latin). Vol. 2. Translated by Schäfer GH. (Leipzig ("Lipsiae") (Germany): Johann Godfried Müller. pp. 148–174. https://books.google.com/books?id=mHVJAAAAcAAJ&pg=PA264

  14. Berthollet CL (1789). "Mémoire sur l'acide prussique" [Memoir on prussic acid]. Mémoires de l'Académie Royale des Sciences (in French): 148–161. Reprinted in: Berthollet CL (1789). "Extrait d'un mémoire sur l'acide prussique" [Extract of a memoir on prussic acid]. Annales de Chimie. 1: 30–39. https://books.google.com/books?id=fC5EAAAAcAAJ&pg=PA148

  15. Newbold BT (1999-11-01). "Claude Louis Berthollet: A Great Chemist in the French Tradition". Canadian Chemical News. Archived from the original on 2008-04-20. Retrieved 2010-03-31. https://web.archive.org/web/20080420175823/http://www.allbusiness.com/north-america/canada/370855-1.html

  16. Gay-Lussac JL (1811). "Note sur l'acide prussique" [Note on prussic acid]. Annales de Chimie. 44: 128–133. https://books.google.com/books?id=uJs5AAAAcAAJ&pg=PA128

  17. Gay-Lussac JL (1815). "Recherche sur l'acide prussique" [Research on prussic acid]. Annales de Chimie. 95: 136–231. https://books.google.com/books?id=m9s3AAAAMAAJ&pg=PA136

  18. Andrussow L (1935). "The catalytic oxydation of ammonia-methane-mixtures to hydrogen cyanide". Angewandte Chemie. 48 (37): 593–595. Bibcode:1935AngCh..48..593A. doi:10.1002/ange.19350483702. /wiki/Angewandte_Chemie

  19. "Non-confidential 2006 IUR Records by Chemical, including Manufacturing, Processing and Use Information". EPA. Archived from the original on 2013-05-10. Retrieved 2013-01-31. https://web.archive.org/web/20130510000856/http://cfpub.epa.gov/iursearch/2006_iur_companyinfo.cfm?chemid=6177&outchem=both

  20. Gail, E.; Gos, S.; Kulzer, R.; Lorösch, J.; Rubo, A.; Sauer, M. "Cyano Compounds, Inorganic". Ullmann's Encyclopedia of Industrial Chemistry. Weinheim: Wiley-VCH. doi:10.1002/14356007.a08_159.pub2. ISBN 978-3-527-30673-2. 978-3-527-30673-2

  21. Endter F (1958). "Die technische Synthese von Cyanwasserstoff aus Methan und Ammoniak ohne Zusatz von Sauerstoff". Chemie Ingenieur Technik. 30 (5): 305–310. doi:10.1002/cite.330300506. /wiki/Doi_(identifier)

  22. "MSDS for potassium ferricyanide" (PDF). Archived from the original (PDF) on 2016-04-18. Retrieved 2023-04-17. https://web.archive.org/web/20160418075117/http://www.labchem.com/tools/msds/msds/LC19040.pdf

  23. "Potassium ferricyanide". PubChem. National Center for Biotechnology Information. https://pubchem.ncbi.nlm.nih.gov/compound/26250

  24. Gail, E.; Gos, S.; Kulzer, R.; Lorösch, J.; Rubo, A.; Sauer, M. "Cyano Compounds, Inorganic". Ullmann's Encyclopedia of Industrial Chemistry. Weinheim: Wiley-VCH. doi:10.1002/14356007.a08_159.pub2. ISBN 978-3-527-30673-2. 978-3-527-30673-2

  25. "Manual of fumigation for insect control – Space fumigation at atmospheric pressure (Cont.)". Food and Agriculture Organization. http://www.fao.org/3/X5042E/x5042E0k.htm#Fumigation%20of%20large%20structures

  26. "New greenhouse gas identified". News.mit.edu. 11 March 2009. https://news.mit.edu/2009/prinn-greenhouse-tt0311

  27. "Chapter 10 : Methyl Bromide" (PDF). Csl.noaa.gov. Archived (PDF) from the original on 2022-10-09. https://csl.noaa.gov/assessments/ozone/1994/chapters/chapter10.pdf

  28. Vetter J (January 2000). "Plant cyanogenic glycosides". Toxicon. 38 (1): 11–36. Bibcode:2000Txcn...38...11V. doi:10.1016/S0041-0101(99)00128-2. PMID 10669009. /wiki/Bibcode_(identifier)

  29. Jones DA (January 1998). "Why are so many food plants cyanogenic?". Phytochemistry. 47 (2): 155–162. Bibcode:1998PChem..47..155J. doi:10.1016/S0031-9422(97)00425-1. PMID 9431670. /wiki/Bibcode_(identifier)

  30. "Are Apple Cores Poisonous?". The Naked Scientists. 26 September 2010. Archived from the original on 6 March 2014. Retrieved 6 March 2014. https://web.archive.org/web/20140306130316/http://www.thenakedscientists.com/HTML/index.php?id=31&tx_naksciquestions_pi1%5BshowUid%5D=2737&cHash=69220df3a3

  31. Aregheore EM, Agunbiade OO (June 1991). "The toxic effects of cassava (manihot esculenta grantz) diets on humans: a review". Veterinary and Human Toxicology. 33 (3): 274–275. PMID 1650055. /wiki/PMID_(identifier)

  32. Blum MS, Woodring JP (October 1962). "Secretion of Benzaldehyde and Hydrogen Cyanide by the Millipede Pachydesmus crassicutis (Wood)". Science. 138 (3539): 512–513. Bibcode:1962Sci...138..512B. doi:10.1126/science.138.3539.512. PMID 17753947. S2CID 40193390. /wiki/Bibcode_(identifier)

  33. Zagrobelny M, de Castro ÉC, Møller BL, Bak S (May 2018). "Cyanogenesis in Arthropods: From Chemical Warfare to Nuptial Gifts". Insects. 9 (2): 51. doi:10.3390/insects9020051. PMC 6023451. PMID 29751568. https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6023451

  34. Loison JC, Hébrard E, Dobrijevic M, Hickson KM, Caralp F, Hue V, et al. (February 2015). "The neutral photochemistry of nitriles, amines and imines in the atmosphere of Titan". Icarus. 247: 218–247. Bibcode:2015Icar..247..218L. doi:10.1016/j.icarus.2014.09.039. https://lirias.kuleuven.be/handle/123456789/486735

  35. Magee BA, Waite JH, Mandt KE, Westlake J, Bell J, Gell DA (December 2009). "INMS-derived composition of Titan's upper atmosphere: Analysis methods and model comparison". Planetary and Space Science. 57 (14–15): 1895–1916. Bibcode:2009P&SS...57.1895M. doi:10.1016/j.pss.2009.06.016. /wiki/Bibcode_(identifier)

  36. Pearce BK, Molaverdikhani K, Pudritz RE, Henning T, Hébrard E (2020). "HCN Production in Titan's Atmosphere: Coupling Quantum Chemistry and Disequilibrium Atmospheric Modeling". Astrophysical Journal. 901 (2): 110. arXiv:2008.04312. Bibcode:2020ApJ...901..110P. doi:10.3847/1538-4357/abae5c. S2CID 221095540. https://doi.org/10.3847%2F1538-4357%2Fabae5c

  37. Pearce BK, Ayers PW, Pudritz RE (March 2019). "A Consistent Reduced Network for HCN Chemistry in Early Earth and Titan Atmospheres: Quantum Calculations of Reaction Rate Coefficients". The Journal of Physical Chemistry A. 123 (9): 1861–1873. arXiv:1902.05574. Bibcode:2019JPCA..123.1861P. doi:10.1021/acs.jpca.8b11323. PMID 30721064. S2CID 73442008. /wiki/ArXiv_(identifier)

  38. Pearce BK, Molaverdikhani K, Pudritz RE, Henning T, Hébrard E (2020). "HCN Production in Titan's Atmosphere: Coupling Quantum Chemistry and Disequilibrium Atmospheric Modeling". Astrophysical Journal. 901 (2): 110. arXiv:2008.04312. Bibcode:2020ApJ...901..110P. doi:10.3847/1538-4357/abae5c. S2CID 221095540. https://doi.org/10.3847%2F1538-4357%2Fabae5c

  39. Wade N (2015-05-04). "Making Sense of the Chemistry That Led to Life on Earth". The New York Times. Retrieved 5 May 2015. https://www.nytimes.com/2015/05/05/science/making-sense-of-the-chemistry-that-led-to-life-on-earth.html

  40. Borowitz JL, Gunasekar PG, Isom GE (September 1997). "Hydrogen cyanide generation by mu-opiate receptor activation: possible neuromodulatory role of endogenous cyanide". Brain Research. 768 (1–2): 294–300. doi:10.1016/S0006-8993(97)00659-8. PMID 9369328. S2CID 12277593. /wiki/Doi_(identifier)

  41. Gunasekar PG, Prabhakaran K, Li L, Zhang L, Isom GE, Borowitz JL (May 2004). "Receptor mechanisms mediating cyanide generation in PC12 cells and rat brain". Neuroscience Research. 49 (1): 13–18. doi:10.1016/j.neures.2004.01.006. PMID 15099699. S2CID 29850349. /wiki/Doi_(identifier)

  42. Borowitz JL, Gunasekar PG, Isom GE (September 1997). "Hydrogen cyanide generation by mu-opiate receptor activation: possible neuromodulatory role of endogenous cyanide". Brain Research. 768 (1–2): 294–300. doi:10.1016/S0006-8993(97)00659-8. PMID 9369328. S2CID 12277593. /wiki/Doi_(identifier)

  43. Smith RP, Kruszyna H (January 1976). "Toxicology of some inorganic antihypertensive anions". Federation Proceedings. 35 (1): 69–72. PMID 1245233. /wiki/PMID_(identifier)

  44. Talhout R, Schulz T, Florek E, van Benthem J, Wester P, Opperhuizen A (February 2011). "Hazardous compounds in tobacco smoke". International Journal of Environmental Research and Public Health. 8 (2): 613–628. doi:10.3390/ijerph8020613. PMC 3084482. PMID 21556207. https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3084482

  45. Ruiz-Bermejo, Marta; Zorzano, María-Paz; Osuna-Esteban, Susana (2013). "Simple Organics and Biomonomers Identified in HCN Polymers: An Overview". Life. 3 (3): 421–448. Bibcode:2013Life....3..421R. doi:10.3390/life3030421. PMC 4187177. PMID 25369814. https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4187177

  46. Al-Azmi A, Elassar AZ, Booth BL (2003). "The Chemistry of Diaminomaleonitrile and its Utility in Heterocyclic Synthesis". Tetrahedron. 59 (16): 2749–2763. doi:10.1016/S0040-4020(03)00153-4. /wiki/Doi_(identifier)

  47. Öberg, Karin (2020-04-10). The galactic recipe for a living planet. Retrieved 2024-12-24 – via www.ted.com. https://www.ted.com/talks/karin_oberg_the_galactic_recipe_for_a_living_planet/transcript?subtitle=en

  48. Snyder LE, Buhl D (1971). "Observations of Radio Emission from Interstellar Hydrogen Cyanide". Astrophysical Journal. 163: L47 – L52. Bibcode:1971ApJ...163L..47S. doi:10.1086/180664. /wiki/Bibcode_(identifier)

  49. Jørgensen UG (1997). "Cool Star Models". In van Dishoeck EF (ed.). Molecules in Astrophysics: Probes and Processes. International Astronomical Union Symposia. Molecules in Astrophysics: Probes and Processes. Vol. 178. Springer Science & Business Media. p. 446. ISBN 978-0792345381. 978-0792345381

  50. Treffers RR, Larson HP, Fink U, Gautier TN (1978). "Upper limits to trace constituents in Jupiter's atmosphere from an analysis of its 5-μm spectrum". Icarus. 34 (2): 331–343. Bibcode:1978Icar...34..331T. doi:10.1016/0019-1035(78)90171-9. /wiki/Bibcode_(identifier)

  51. Snyder LE, Buhl D (1971). "Observations of Radio Emission from Interstellar Hydrogen Cyanide". Astrophysical Journal. 163: L47 – L52. Bibcode:1971ApJ...163L..47S. doi:10.1086/180664. /wiki/Bibcode_(identifier)

  52. Bieging JH, Shaked S, Gensheimer PD (2000). "Submillimeter- and Millimeter-Wavelength Observations of SiO and HCN in Circumstellar Envelopes of AGB Stars". Astrophysical Journal. 543 (2): 897–921. Bibcode:2000ApJ...543..897B. doi:10.1086/317129. https://doi.org/10.1086%2F317129

  53. Schilke P, Menten KM (2003). "Detection of a Second, Strong Sub-millimeter HCN Laser Line toward Carbon Stars". Astrophysical Journal. 583 (1): 446–450. Bibcode:2003ApJ...583..446S. doi:10.1086/345099. S2CID 122549795. https://doi.org/10.1086%2F345099

  54. Boger GI, Sternberg A (2005). "CN and HCN in Dense Interstellar Clouds". Astrophysical Journal. 632 (1): 302–315. arXiv:astro-ph/0506535. Bibcode:2005ApJ...632..302B. doi:10.1086/432864. S2CID 118958200. /wiki/ArXiv_(identifier)

  55. Boger GI, Sternberg A (2005). "CN and HCN in Dense Interstellar Clouds". Astrophysical Journal. 632 (1): 302–315. arXiv:astro-ph/0506535. Bibcode:2005ApJ...632..302B. doi:10.1086/432864. S2CID 118958200. /wiki/ArXiv_(identifier)

  56. Gao Y, Solomon PM (2004). "The Star Formation Rate and Dense Molecular Gas in Galaxies". Astrophysical Journal. 606 (1): 271–290. arXiv:astro-ph/0310339. Bibcode:2004ApJ...606..271G. doi:10.1086/382999. S2CID 11335358. /wiki/ArXiv_(identifier)

  57. Gao Y, olomon PM (2004). "HCN Survey of Normal Spiral, Infrared-luminous, and Ultraluminous Galaxies". Astrophysical Journal Supplement Series. 152 (1): 63–80. arXiv:astro-ph/0310341. Bibcode:2004ApJS..152...63G. doi:10.1086/383003. S2CID 9135663. /wiki/ArXiv_(identifier)

  58. Wu J, Evans NJ (2003). "Indications of Inflow Motions in Regions Forming Massive Stars". Astrophysical Journal. 592 (2): L79 – L82. arXiv:astro-ph/0306543. Bibcode:2003ApJ...592L..79W. doi:10.1086/377679. S2CID 8016228. /wiki/ArXiv_(identifier)

  59. Loenen AF (2007). "Molecular properties of (U)LIRGs: CO, HCN, HNC and HCO+". Proceedings IAU Symposium. 242: 462–466. arXiv:0709.3423. Bibcode:2007IAUS..242..462L. doi:10.1017/S1743921307013609. S2CID 14398456. /wiki/ArXiv_(identifier)

  60. Zubritsky E, Neal-Jones N (11 August 2014). "Release 14-038 – NASA's 3-D Study of Comets Reveals Chemical Factory at Work". NASA. Retrieved 12 August 2014. https://www.nasa.gov/press/2014/august/goddard/nasa-s-3-d-study-of-comets-reveals-chemical-factory-at-work

  61. Cordiner MA, Remijan AJ, Boissier J, Milam SN, Mumma MJ, Charnley SB, et al. (11 August 2014). "Mapping the Release of Volatiles in the Inner Comae of Comets C/2012 F6 (Lemmon) and C/2012 S1 (ISON) Using the Atacama Large Millimeter/Submillimeter Array". The Astrophysical Journal. 792 (1): L2. arXiv:1408.2458. Bibcode:2014ApJ...792L...2C. doi:10.1088/2041-8205/792/1/L2. S2CID 26277035. /wiki/The_Astrophysical_Journal

  62. "First detection of super-earth atmosphere". ESA/Hubble Information Centre. February 16, 2016. https://phys.org/news/2016-02-super-earth-atmosphere.html

  63. Green, Jaime (5 December 2023). "What Is Life? - The answer matters in space exploration. But we still don't really know". The Atlantic. Archived from the original on 5 December 2023. Retrieved 15 December 2023. https://www.theatlantic.com/science/archive/2023/12/defining-life-existentialism-scientific-theory/676238/

  64. Chang, Kenneth (14 December 2023). "Poison Gas Hints at Potential for Life on an Ocean Moon of Saturn - A researcher who has studied the icy world said "the prospects for the development of life are getting better and better on Enceladus."". The New York Times. Archived from the original on 14 December 2023. Retrieved 15 December 2023. https://www.nytimes.com/2023/12/14/science/enceladus-moon-cyanide-life-saturn.html

  65. Peter, Jonah S.; et al. (14 December 2023). "Detection of HCN and diverse redox chemistry in the plume of Enceladus". Nature Astronomy. 8 (2): 164–173. arXiv:2301.05259. Bibcode:2024NatAs...8..164P. doi:10.1038/s41550-023-02160-0. S2CID 255825649. Archived from the original on 15 December 2023. Retrieved 15 December 2023. https://www.nature.com/articles/s41550-023-02160-0

  66. Schnedlitz, Markus (2008) Chemische Kampfstoffe: Geschichte, Eigenschaften, Wirkung. GRIN Verlag. p. 13. ISBN 3640233603. /wiki/ISBN_(identifier)

  67. Weapons of War - Poison Gas. firstworldwar.com http://www.firstworldwar.com/weaponry/gas.htm

  68. Environmental and Health Effects Archived 2012-11-30 at the Wayback Machine. Cyanidecode.org. Retrieved on 2012-06-02. http://www.cyanidecode.org/cyanide_environmental.php

  69. Environmental and Health Effects Archived 2012-11-30 at the Wayback Machine. Cyanidecode.org. Retrieved on 2012-06-02. http://www.cyanidecode.org/cyanide_environmental.php

  70. "Hydrogen Cyanide". Organisation for the Prohibition of Chemical Weapons. Retrieved 2009-01-14. http://www.opcw.org/about-chemical-weapons/types-of-chemical-agent/blood-agents/hydrogen-cyanide/

  71. Van Pelt, Robert Jan; Dwork, Debórah (1996). Auschwitz, 1270 to the present. Norton. p. 443. ISBN 9780300067552. 9780300067552

  72. "Blue Fume". Chemical Factory Draslovka a.s. Retrieved 2020-07-06. https://www.draslovka.cz/about-us#products

  73. "Uragan D2". 2015-07-17. Archived from the original on 2015-07-17. Retrieved 2022-10-19. https://web.archive.org/web/20150717224853/http://www.draslovka.cz/uragan-d2

  74. Binkov's Battlegrounds (April 27, 2022). "How would have WW2 gone if the US had not used nuclear bombs on Japan?". YouTube.Com. Retrieved June 23, 2022. https://www.youtube.com/watch?v=8CFPaSH84ZU

  75. Pilkington, Ed (28 May 2021). "Arizona 'refurbishes' its gas chamber to prepare for executions, documents reveal". The Guardian. Retrieved 2022-06-14. https://www.theguardian.com/us-news/2021/may/28/arizona-gas-chamber-executions-documents

  76. Lytle T. "Poison Harpoons". Whalecraft.net. Archived from the original on 2019-02-15. https://web.archive.org/web/20190215100154/http://www.whalecraft.net/Poison_Irons.html

  77. "The Poison Garden website". Thepoisongarden.co.uk. Archived from the original on 10 February 2020. Retrieved 18 October 2014. https://web.archive.org/web/20200210022050/http://thepoisongarden.co.uk/atoz/prunus_laurocerasus.htm

  78. "Documentation for Immediately Dangerous to Life or Health Concentrations (IDLHs) – 74908". NIOSH. 2 November 2018. https://www.cdc.gov/niosh/idlh/74908.html