Scientists have long debated the mysteries of the cosmos, and we are privileged to live in a thrilling era for galaxy research. Despite potential cutbacks in research funding in the US and UK, our comprehension of the universe continues to grow. Since its launch on Christmas Day 2021, the James Webb Space Telescope (JWST) has dramatically transformed our understanding of ancient galaxies. Contrary to previous cosmological models, these galaxies are proving to be significantly brighter and filled with hot gas and stars.

Observations from JWST are truly groundbreaking. We are now able to study galaxies that formed just 300 million years post-Big Bang. While that may sound like a vast period, in the grand timeline of the universe—approximately 14 billion years—it’s merely the infancy of cosmic evolution. For context, I am 43 years old, which correlates to 2.14% of my lifespan when I was under one year old.

Rohan P. Naidu and a team from the Massachusetts Institute of Technology identified a remarkable galaxy last year, named MoM-z14. Their research paper describes MoM-z14 as a “cosmic miracle,” brighter than anticipated for its early stage in cosmic history. Such observations have only recently been possible, as prior telescopes lacked the capability to detect these faint objects due to their incredible distance. Paradoxically, while MoM-z14 appears dim through conventional telescopes, it emits more light than anticipated based on theoretical constructs.

Nevertheless, the unexpected brightness of these galaxies raises a crucial question: how can we confirm that what we’re observing is indeed a galaxy? In April of this year, Marcia Bradaci and an international team from the University of California, Davis, meticulously analyzed the JWST data. In a paper currently pending peer review, they suggest that two of the young, bright objects identified by JWST are not galaxies at all but rather brown dwarfs within our Milky Way. In other words, what we initially thought of as distant galaxies turned out to be star-like objects much closer to home.

The findings were surprising. If one were to consider what opposes a galaxy, brown dwarfs would be a prime candidate. Too large to evolve into gas giants like Jupiter, yet too small to achieve stellar nuclear fusion, a brown dwarf occupies a unique niche—and could fit comfortably within our solar system. In other words, brown dwarfs are compact compared to a galaxy sprawling with billions of stars. Only time will tell if Bradaci’s conclusions hold true and whether observations of other ancient galaxies are marred by similar misconceptions.

However, we are well-equipped to investigate these celestial enigmas. I predict that 2026 will emerge as a landmark year for astronomy. Despite governmental obstacles, Chile’s Vera C. Rubin Observatory is set to commence a 10-year space-time legacy survey, offering detailed mapping of the Southern Hemisphere sky and imaging over 5 billion galaxies. This initiative will coincide with JWST’s operations and NASA’s upcoming flagship observatory, the Nancy Grace Roman Space Telescope. Roman will also complement the European Space Agency’s Euclid mission, projected to image hundreds of millions of galaxies. The combined efforts of JWST, Rubin, Roman, and Euclid could revolutionize our understanding of galaxy formation and evolution.