Propyne

Hydrocarbon compound (HC≡C–CH3) From Wikipedia, the free encyclopedia

Propyne

Propyne (methylacetylene) is an alkyne with the chemical formula CH3C≡CH. It is a component of MAPD gas—along with its isomer propadiene (allene), which was commonly used in gas welding. Unlike acetylene, propyne can be safely condensed.[3]

Quick Facts Names, Identifiers ...
Propyne
Thumb
Methylacetylene
Thumb
Names
Preferred IUPAC name
Other names
Methylacetylene
Methyl acetylene
Allylyne
Identifiers
3D model (JSmol)
878138
ChEBI
ChEMBL
ChemSpider
ECHA InfoCard 100.000.754
EC Number
  • 200-828-4
MeSH C022030
UNII
  • InChI=1S/C3H4/c1-3-2/h1H,2H3
    Key: MWWATHDPGQKSAR-UHFFFAOYSA-N
  • InChI=1/C3H4/c1-3-2/h1H,2H3
    Key: MWWATHDPGQKSAR-UHFFFAOYAI
  • CC#C
Properties
CH3C≡CH
Molar mass 40.0639 g/mol
Appearance Colorless gas[2]
Odor Sweet[2]
Density 0.53 g/cm3
Melting point −102.7 °C (−152.9 °F; 170.5 K)
Boiling point −23.2 °C (−9.8 °F; 250.0 K)
Vapor pressure 5.2 atm (20°C)[2]
Hazards
Explosive limits 1.7%-?[2]
NIOSH (US health exposure limits):
PEL (Permissible)
TWA 1000 ppm (1650 mg/m3)[2]
REL (Recommended)
TWA 1000 ppm (1650 mg/m3)[2]
IDLH (Immediate danger)
1700 ppm[2]
Except where otherwise noted, data are given for materials in their standard state (at 25 °C [77 °F], 100 kPa).
N verify (what is YN ?)
Close

Production and equilibrium with propadiene

Propyne exists in equilibrium with propadiene, the mixture of propyne and propadiene being called MAPD:

H3C−C≡CH ⇌ H2C=C=CH2

The coefficient of equilibrium Keq is 0.22 at 270 °C or 0.1 at 5 °C. MAPD is produced as a side product, often an undesirable one, by cracking propane to produce propene, an important feedstock in the chemical industry.[3] MAPD interferes with the catalytic polymerization of propene.

Laboratory methods

Propyne can also be synthesized on laboratory scale by reducing 1-propanol,[4] allyl alcohol or acetone[5] vapors over magnesium.

Use as a rocket fuel

European space companies have researched using light hydrocarbons with liquid oxygen, a relatively high performing liquid rocket propellant combination that would also be less toxic than the commonly used MMH/NTO (monomethylhydrazine/nitrogen tetroxide). Their research showed[citation needed] that propyne would be highly advantageous as a rocket fuel for craft intended for low Earth orbital operations. They reached this conclusion based upon a specific impulse expected to reach 370 s with oxygen as the oxidizer, a high density and power density—and the moderate boiling point, which makes the chemical easier to store than cryogenic fuels that must be kept at extremely low temperatures.[6]

Organic chemistry

Propyne is a convenient three-carbon building block for organic synthesis. Deprotonation with n-butyllithium gives propynyllithium. This nucleophilic reagent adds to carbonyl groups, producing alcohols and esters.[7] Whereas purified propyne is expensive, MAPP gas could be used to cheaply generate large amounts of the reagent.[8]

Propyne, along with 2-butyne, is also used to synthesize alkylated hydroquinones in the total synthesis of vitamin E.[9]

The chemical shift of an alkynyl proton and propargylic proton generally occur in the same region of the 1H NMR spectrum. In propyne, these two signals have almost exactly the same chemical shifts, leading to overlap of the signals, and the 1H NMR spectrum of propyne, when recorded in deuteriochloroform on a 300 MHz instrument, consists of a single signal, a sharp singlet resonating at 1.8 ppm.[10]

In Astrophysics

Propyne has been detected in multiple astrophysical objects following its first observation in 1973 in the galactic center giant molecular cloud Sgr B2 using radio astronomy techniques.[11] Propyne has been proposed to act as a precursor molecule to the formation of PAHs in space, such as indene.[12]

Propyne has been detected by infrared spectroscopy in the chemically reducing atmospheres of the outer planets in our solar system, including on Jupiter in 2000 [13] and on Saturn in 1997,[14] both using the Infrared Space Observatory; on Titan in 1981 using Voyager's IRIS instrument;[15] and on the ice giants Uranus in 2006 [16] and on Neptune in 2008 [17] using the Spitzer space telescope.

Notes

  1. "Prop-1-yne" mistake fixed in the errata Archived 2019-08-01 at the Wayback Machine. The locant is omitted according to P-14.3.4.2 (d), p. 31 for propene and P-31.1.1.1, Examples, p. 374 for propyne.

References

Loading related searches...

Wikiwand - on

Seamless Wikipedia browsing. On steroids.