Astronomy & Universe

Ancient chemically primitive galaxy exhibits record-low oxygen

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Ancient chemically primitive galaxy exhibits record-low oxygen
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New insights into one of the oldest known galaxies

An international consortium of astronomers has employed the James Webb Space Telescope (JWST) together with the natural magnification provided by gravitational lensing to conduct a definitive spectroscopic study of LAP1‑B, an ultra‑faint galaxy dating back roughly 13 billion years.

The combination of JWST’s infrared spectroscopy and the lensing effect of a massive foreground galaxy amplified the faint signal, allowing researchers to determine the galaxy’s chemical makeup with unprecedented precision. The analysis revealed an oxygen abundance of just one‑two‑hundred‑and‑fortieth of the solar value, setting a new low for galaxies observed at such early epochs.

This exceptionally low metallicity indicates that LAP1‑B experienced minimal enrichment from previous generations of stars, offering a rare glimpse into the conditions prevailing shortly after the Big Bang.

  • JWST provided high‑resolution infrared spectra.
  • Gravitational lensing boosted the galaxy’s faint light.
  • Measured oxygen level is approximately 0.4 % of the Sun’s.

The findings advance our understanding of chemical evolution in the early universe and suggest that many primordial galaxies were even more primitive than current models predict.

Frequently asked questions

Was bedeutet der extrem niedrige Sauerstoffgehalt von LAP1‑B?

Er zeigt, dass die Galaxie kaum durch frühere Sternengenerationen angereichert wurde und somit sehr nahe an den ursprünglichen Bedingungen nach dem Urknall ist.

Wie hat die Gravitationslinse die Beobachtungen unterstützt?

Die massive Vordergrundgalaxie wirkt wie ein natürliches Fernrohr und verstärkt das Licht der fernen, schwachen Quelle, sodass JWST detaillierte Spektren aufnehmen kann.

Warum ist JWST für diese Messungen besonders geeignet?

Das Teleskop verfügt über empfindliche Infrarot-Instrumente, die das rotverschobene Licht sehr entfernter Galaxien erfassen und analysieren können.