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Propyne ( methylacetylene) is an with the . It is a component of —along with its (allene), which was commonly used in . Unlike , propyne can be safely .Peter Pässler, Werner Hefner, Klaus Buckl, Helmut Meinass, Andreas Meiswinkel, Hans-Jürgen Wernicke, Günter Ebersberg, Richard Müller, Jürgen Bässler, Hartmut Behringer, Dieter Mayer, "Acetylene" in Ullmann's Encyclopedia of Industrial Chemistry Wiley-VCH, Weinheim 2007 ().


Production and equilibrium with propadiene
Propyne exists in equilibrium with , the mixture of propyne and propadiene being called MAPD:
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 to produce , an important in the chemical industry. MAPD interferes with the catalytic of propene.


Laboratory methods
Propyne can also be synthesized on laboratory scale by reducing 1-propanol, or vapors over magnesium.


Use as a rocket fuel
European space companies have researched using light with , 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 that propyne would be highly advantageous as a for craft intended for low Earth orbital operations. They reached this conclusion based upon a expected to reach 370 with oxygen as the oxidizer, a high and —and the moderate , which makes the chemical easier to store than that must be kept at extremely low temperatures.


Organic chemistry
Propyne is a convenient three-carbon building block for organic synthesis. Deprotonation with gives . This reagent adds to groups, producing alcohols and . Whereas purified propyne is expensive, MAPP gas could be used to cheaply generate large amounts of the reagent.

Propyne, along with 2-butyne, is also used to synthesize in the of .

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.

(2015). 9781936221349, W. H. Freeman.


In Astrophysics
Propyne has been detected in multiple astrophysical objects following its first observation in 1973 in the Sgr B2 using techniques. Propyne has been proposed to act as a precursor molecule to the formation of PAHs in space, such as .

Propyne has been detected by in the of the in the , including on in 2000 and on in 1997, both using the Infrared Space Observatory; on Titan in 1981 using IRIS instrument; and on the in 2006 and on in 2008 using the Spitzer space telescope.


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