Star Furnaces Don't Incinerate Life ⚡ экспресс
Recently, glycolamide (an isomer of the amino acid glycine) was tentatively detected in a hot protostellar core using the ALMA telescope. Seven spectral lines pointed to its abundance of about 1.7×10⁻¹⁰ relative to H₂. The similar ratios with formamide and acetamide in different environments suggest a unified amide network—like a chemical 'bridge' between interstellar matter and the stellar nursery. This confirms that molecules important for life survive the turbulent stages of star formation.
Radio telescopes detected emissions from the celestial object G358.93-0.03 MM1 — a hot cocoon inside which a massive star is igniting. Within that glow, lines of glycolamide appeared, a delicate carbon molecule.
The fragile structure didn't fall apart near the growing sun, where the heat should have erased everything down to atoms.
Half-century-old ideas of Fred Hoyle that dust between stars can nurture complex organics have gained new support. Comparison with the cold cloud G+0.693-0.027 showed: the ratio of glycolamide and its relatives — formamide and acetamide — in the hot zone is the same as in the icy one. The heat was expected to scramble all proportions, but the recipe held firm. Like a cookbook surviving a toss into a scorching oven.
This fact suggests a unified 'amide network' linking hydrogen clouds to protostellar clumps. Chemical memory survives: the birth of suns doesn't erase molecular recipes. Life's ingredients, imprinted in cosmic dust, journey through stellar furnaces and remain recognizable.
🎯 Glycolamide is an isomer of glycine: swap two atoms, and you have the amino acid that makes up our proteins. Nature seems to have mixed up just one bond, creating a molecular draft.
🎬 Fred Hoyle, mentioned above, in his novel 'The Black Cloud' described an intelligent interstellar cloud. Now, in real clouds, organics have been found that withstand stellar heat and retain their molecular signature.