Taking into account that approximately half of these stars have orbiting material and around 120 possess disks that date back to their formation around 2 million years ago, the discovery of tryptophan in this region suggests that protein-building blocks could be ubiquitous in the gas from which stars and planets form. Dr. Susana Iglesias-Groth, the lead author of the study, notes this could be key to understanding life development in exoplanetary systems.
Tryptophan and other amino acids have previously been found in meteorites, asteroids, and comets, as well as in extreme locations like the Venusian atmosphere. Thus, their presence in interstellar space isn't entirely surprising. Moreover, their mild temperature of 7°C in the IC348 region aligns with previous observations. The discovery highlights the prevalence of amino acids and their potential role in planetary system chemistry, and ultimately, the genesis of life. These findings are published in the Monthly Notices of the Royal Astronomical Society.
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