Molecular precursors to life discovered in the Perseus Cloud

Molecular precursors to life discovered in the Perseus Cloud

Artistic composition of a “soup” of prebiotic molecules around a protoplanetary disk. Credit: Gabriel Pérez Díaz (IAC)

Susan Iglesias-Groth, of the Instituto de Astrofísica de Canarias (IAC) and Martina Marín-Dobrincicof the Polytechnic University of Cartagena have discovered the presence of numerous prebiotic molecules in the star formation region IC348 of the Perseus Molecular Cloud, a young star cluster some 2-3 million years old.

Some of these are considered essential building bricks for the construction of more complex molecules such as the , which formed the genetic code of ancient microorganisms, and brought about the flourishing of life on Earth. Getting to know the distribution and the abundances of these precursor molecules in regions where planets are very probably forming, is an important challenge for astrophysics.

The Perseus Cloud is one of the star forming regions closest to the solar system. Many of its stars are young, and have protoplanetary disks where the which give rise to planets can take place.

“It is an extraordinary laboratory of organic chemistry,” explains Iglesias-Groth, who in 2019 found fullerenes in the same cloud. “These are complex molecules of pure carbon which often occur as for the key molecules of life.”

Now new research has detected in the inner part of this region common molecules such as (H2), hydroxyl (OH), water (H2O), (CO2) and ammonia (NH3) as well as several carbon bearing molecules which could play an important role in the production of more complex hydrocarbons and prebiotic molecules, such as (HCN), acetylene (C2H2), diacetylene (C4H2), cyanoacetylene (HC3N), cyanobutadiyne (HC5N), ethane (C2H6), hexatrine (C6H2) and benzene (C6H6).

The data also show the presence of more complex molecules such as the polycyclic armoatic hydrocarbons (PAH) and the fullerenes C60 and C70. “IC 348 seems to be very rich and diverse in its molecular content,” states Iglesias-Gorth. “The novelty is that we see the molecules in the diffuse gas from which stars and protoplanetary disks are forming.”

The presence of prebiotic molecules at interstellar sites so close to this star clusters suggests the possibility that accretion processes are taking place onto young planets that could contribute to the formation of complex organic molecules. “These key molecules could have been supplied to the nascent planets in the protoplanetary disks and could in this way help to produce there a route towards the molecules of life,” says Marina-Dobrincic.

The detection by the two researchers is based on data taken wth NASA’s Spitzer satellite. The next step will be to use the powerful James Webb Space Telescope (JWST). “The spectroscopic capacity of the JWST could provide details about the of all these molecules, and extend the present search to others which are more complex, giving higher sensitivity and resolution which are essential to confirm the very probable presence of amino acids in the gas in this and in other star forming regions,” concludes Iglesias-Groth.

The study is published in the journal Monthly Notices of the Royal Astronomical Society.

More information:
Susana Iglesias-Groth et al, A rich molecular chemistry in the gas of the IC 348 star cluster of the Perseus Molecular Cloud, Monthly Notices of the Royal Astronomical Society (2023). DOI: 10.1093/mnras/stad495

Molecular precursors to life discovered in the Perseus Cloud (2023, April 3)
retrieved 23 April 2023

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