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Astronomers Detect First Sugar Molecule in Milky Way’s Central Cloud

Laboratory spectral fingerprints and coordinated Yebes and Pico Veleta radio observations show the four-carbon sugar erythritulose is present in cloud G+0.693−0.027, pointing to interstellar pathways for complex organics.

Overview

  • The detection was reported Monday, July 13, 2026, in Nature Astronomy by a Spanish-led team headed by Izaskun Jiménez-Serra.
  • Researchers matched laboratory-measured spectra of erythritulose to up to 12 separate radio lines captured with the Yebes and Pico Veleta telescopes to identify the molecule.
  • Erythritulose was found in the chemically rich molecular cloud G+0.693−0.027 near the Galactic center and appears at least eight times more abundant there than comparable three-carbon sugars.
  • The team argues the sugar most likely forms on icy dust-grain surfaces from simpler two-carbon precursors such as alcohols and aldehydes, showing a plausible nonbiological route to larger organics.
  • Experts say the finding advances astrochemistry and models of prebiotic chemistry but caution it does not prove biological activity or solve origin-of-life questions and requires independent confirmation and further observations.