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Ethanolamine (NH2CH2CH2OH) was detected toward the
galactic center source
G+0.693–0.027 by
Rivilla and co-workers, as reported in 2021 in
Procedings of the National Academy of Sciences. The detection utilized the
IRAM 30m telescope as well as the
Yebes 40m telescope. Of 45 rotational
transitions that fall with the wavelenth range of the observations that have sufficient brightness
to be detectable at 10-15 K, 14 were either unblended or slightly blending with transitions due to other
other molecules and serve to secure the identification. Very recently, ethanolamine has also been
detected toward the newly identified, molecule-rich galactic
center cloud G+0.633–0.0604,
providing ample confirmation for ethanolamine.
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Ethanolamine, or more properly
monoethanolamine, is well-known in terrestrial
industrial chemistry, where it represents about 40% of the entire $4 billion USD
global market of mono-,
di-, and triethanolamine compounds. (Mono)ethanolamine also plays an important role in
biochemistry,
where it is the
head group
(as Rivilla and co-workers note in their title) of
phospholipids
that are found in all cells and make up many cell membranes. Click
here to see a molecular model of a particular phospholipid
that shows how ethanolamine is connected to the other parts of the molecule (the webpahe even lets you highlight
the hydrophilic and hydrophobic parts of the molecule).
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