Astronomers Observe the Most Chemically Primitive Galaxy in the Early Universe - Universe Today

An image of the massive galaxy cluster MACS J0416 with a three-color composite image of LAP1-B in "velocity space" (inset). Credit: NASA/ESA/CSA/K. Nakajima et al. (2026)

One of the greatest achievements of the James Webb Space Telescope is how it has allowed scientists to push the boundaries of astronomy by observing galaxies that existed during the early Universe, less than 1 billion years after the Big Bang. This period, known as the Epoch of Reionization, coincides with what astronomers have nicknamed the "Cosmic Dark Ages." During this time, 380,000 to 1 billion years after the Big Bang, the Universe was filled with neutral hydrogen, and any sources of light visible today are redshifted beyond the limits of conventional telescopes.

Thanks to Webb's advanced infrared instruments and spectrometers, scientists can now peer behind this veil and see how galaxies have evolved since the earliest cosmological epochs. In a recent discovery, an international team of astronomers used Webb and the gravitational lensing technique to capture a rare look at LAP1-B, an ultra-faint galaxy that existed 800 million years after the Big Bang. Using Webb's spectrometers, the team was able to definitively characterize this galaxy, revealing it to be the most metal-poor galaxy in the early Universe observed to date.

The team was led by Associate Professor Kimihiko Nakajima of Kanazawa University. He was joined by colleagues from the National Astronomical Observatory of Japan (NAOJ), the Institute for Cosmic Ray Research (ICRR), the Kavli Institute for the Physics and Mathematics of the Universe (IMPU), the Waseda Research Institute for Science and Engineering, the Astrophysics and Space Science Observatory Bologna (OAS), the Kavli Institute for Cosmology, the Cavendish Laboratory, and Caltech's Infrared Processing and Analysis Center (IPAC). The study describing their research appeared on May 13th in the journal Nature.

*Timeline of the Big Bang, emphasizing the early Universe and Epoch of Reionization. Credit: Big Think/Ben Gibson/NASA/Pablo Carlos Budassi*

In the immediate aftermath of the Big Bang, the Universe contained only light elements such as hydrogen and helium, while the elements necessary for life (carbon, oxygen, etc.) were absent. These elements were forged in the interiors of the first generation of stars (Population III), which were then dispersed when these stars went supernova and blew off their external layers. For decades, astronomers have been hoping to find these stars so they could witness the moment they began seeding the Universe with heavier elements. This has been problematic since the earliest galaxies that hosted Population III stars appear so small and faint.

As a result, determining their chemical makeup through spectroscopy was thought to be nearly impossible until now. The work of Nakajima builds on initial detections of LAP1-B by adding JWST spectra to the picture, revealing a record-low oxygen abundance (1/240th that of the Sun). When combined with an elevated carbon-to-oxygen ratio and a dominant dark matter halo, these findings suggest that LAP1-B is a progenitor to the fossil galaxies found near the Milky Way. Astronomers have been searching for these "ancestor" galaxies, making LAP1-B a historic window into the earliest stages of galaxy formation.

The team was assisted by the presence of an intervening galaxy cluster, which acted as a gravitational lens, magnifying the light from LAP1-B by a factor of 100. After 30 hours of observations and deep spectroscopy, the team was finally able to characterize the chemical abundance of this galaxy. In addition to being chemically primitive, the galaxy's carbon-to-oxygen ratio closely matches theoretical predictions for the material dispersed by Population III star explosions. Said Associate Professor Nakajima in a Kanazawa University press release:

I was instantly thrilled by the extreme lack of oxygen revealed in the data. Finding a galaxy in such a primitive state is astonishing. It’s a chemical signature that clearly indicates a primordial galaxy caught in the moments shortly after its formation. Usually, we act like 'cosmic archaeologists,' trying to guess the past by looking at old stars in our own neighborhood. But now, we can analyze the gas directly from the original scene 13 billion years ago. We are witnessing the moment when a galaxy first inherited the chemical building blocks created by the universe's earliest stars.

The team also discovered that LAP1-B is incredibly light (less than 3,300 Solar masses), implying that most of the galaxy consists of dark matter in the form of a halo. Along with its unique chemical makeup, this makes it a near-perfect match for the "Ultra-Faint Dwarf galaxies (UFDs)" found near the Milky Way today. Said Professor Masami Ouchi (NAOJ/University of Tokyo), a member of the research team:

UFDs are not...