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. One hundred grams of crushed apple seeds can yield about 70 mg of HCN. 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. Some
millipedes, such as
Harpaphe haydeniana,
Desmoxytes purpurosea, and
Apheloria release hydrogen cyanide as a defense mechanism, as do certain insects, such as
burnet moths and the larvae of
Paropsisterna eucalyptus. Hydrogen cyanide is contained in the exhaust of vehicles, and in smoke from burning nitrogen-containing
plastics. is a giant swirling cloud of HCN (November 29, 2012)
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. One of these measurements was
in situ, where the Cassini spacecraft dipped between above Titan's surface to collect atmospheric gas for
mass spectrometry analysis. 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). Ultraviolet radiation breaks HCN up into CN + H; however, CN is efficiently recycled back into HCN via the reaction CN + CH4 → HCN + CH3.
In mammals Some authors 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. 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.
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. HCN is a constituent of
tobacco smoke.
HCN and the origin of life As a precursor to amino acids and nucleic acids, hydrogen cyanide has been proposed to have played a part in the
origin of life. Compounds of special interest are
oligomers of HCN including its trimer
aminomalononitrile and tetramer
diaminomaleonitrile, which can be described as (HCN)3 and (HCN)4, respectively. Although the relationship of these chemical reactions to the origin of life theory remains speculative, studies in this area uncovered new pathways to organic compounds derived from the condensation of HCN (e.g.
adenine).
In space Because hydrogen cyanide is a precursor to nucleic acids, which are critical for terrestrial life,
astronomers are incentivized to search for derivatives of HCN. HCN has been detected in the
interstellar medium and in the atmospheres of
carbon stars. 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. The J=1→0, J=3→2, J= 4→3, and J=10→9 pure
rotational transitions have all been observed. HCN is formed in
interstellar clouds through one of two major pathways: 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. and as a tracer of stellar inflow in high-mass star-forming regions. Further, the HNC/HCN ratio has been shown to be an excellent method for distinguishing between PDRs and X-ray-dominated regions (XDRs). 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). 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. On 14 December 2023, astronomers reported the first-time discovery, in the
plumes of
Saturn's sixth-largest moon
Enceladus, hydrogen cyanide, a possible chemical essential for
life 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." ==As a poison and chemical weapon==