Monday, October 4, 2010

Anthracene band recently identified in the Perseus star formation


Image of the anthracene band recently identified in the Perseus star formation region by researchers from the IAC and the University of Texas.

This molecule is formed by three hexagonal rings of carbon atoms surrounded by hydrogen atoms. Credit: Gaby Perez and Susana Iglesias-Groth

A team of scientists from the Instituto Astrofisica de Canarias (IAC) and the University of Texas has succeeded in identifying one of the most complex organic molecules yet found in the material between the stars, the so-called interstellar medium.

The discovery of anthracene could help resolve a decades-old astrophysical mystery concerning the production of organic molecules in space. The researchers report their findings in the journal Monthly Notices of the Royal Astronomical Society.

‘We have detected the presence of anthracene molecules in a dense cloud in the direction of the star Cernis 52 in Perseus, about 700 light-years from the Sun,’ explains Susana Iglesias Groth, the IAC researcher heading the study.

In her opinion, the next step is to investigate the presence of amino acids. Molecules like anthracene are prebiotic, so when they are subjected to ultraviolet radiation and combined with water and ammonia, they could produce amino acids and other compounds essential for the development of life

‘Two years ago,’ says Iglesias, ‘we found proof of the existence of another organic molecule, naphthalene, in the same place, so everything indicates that we have discovered a star formation region rich in prebiotic chemistry.’ Until now, anthracene had been detected only in meteorites and never in the interstellar medium.

Oxidised forms of this molecule are common in living systems and are biochemically active.

The The William Herschel Telescope on the Canary Islands was inaugurated in 1987. Credit: http://www.ing.iac.es

On our planet, oxidized anthracene is a basic component of aloe and has anti-inflammatory properties.

The new finding suggests that a good part of the key components in terrestrial prebiotic chemistry could be present in interstellar matter.

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