JWST Photographs Tiny Galaxies That Shaped the Early Universe

Soumyadeep Mukherjee

Soumyadeep Mukherjee is an award-winning astrophotographer from India. He has a doctorate degree in Linguistics. His work extends to the sub-genres of nightscape, deep sky, solar, lunar and optical phenomenon photography. He is also a photography educator and has conducted numerous workshops. His works have appeared in over 40 books & magazines including Astronomy, BBC Sky at Night, Sky & Telescope among others, and in various websites including National Geographic, NASA, Forbes. He was the first Indian to win “Astronomy Photographer of the Year” award in a major category.

jwst reionization cover

NASA’s James Webb Space Telescope has made a thrilling discovery. It has found a group of small but powerful galaxies that likely helped reionize the early universe. These galaxies existed just 800 million years after the Big Bang. They may have played a major role in making the universe transparent. This breakthrough comes from the UNCOVER program. UNCOVER stands for Ultra Deep NIRSpec and NIRCam Observations before the Epoch of Reionization. It is one of JWST’s first deep-field surveys. It focuses on a galaxy cluster named Abell 2744, also called Pandora’s Cluster.

What is reionization?

To understand this discovery, we need to know what reionization is. Right after the Big Bang, the universe was hot and full of charged particles. As it expanded and cooled, these particles combined into neutral hydrogen atoms. This period is called the “cosmic dark ages.” No stars had formed yet. Light couldn’t travel far.

Then, the first stars and galaxies were born. Their radiation started breaking apart those neutral hydrogen atoms. The universe became ionized again. This process is called “reionization.” It allowed light to travel freely. That’s how the universe became clear. But scientists didn’t know what caused reionization. Were they big galaxies? Quasars? Or tiny galaxies we hadn’t seen yet? Now, JWST has brought us closer to the answer.

White diamonds show the locations of 20 of the 83 young, low-mass, starburst galaxies found in infrared images of the giant galaxy cluster Abell 2744. Credit: NASA/ESA/CSA/Bezanson et al. 2024 and Wold et al. 2025
White diamonds show the locations of 20 of the 83 young, low-mass, starburst galaxies found in infrared images of the giant galaxy cluster Abell 2744. Credit: NASA/ESA/CSA/Bezanson et al. 2024 and Wold et al. 2025

The power of gravitational lensing

The UNCOVER program used a powerful trick, gravitational lensing. That’s when a massive galaxy cluster, like Abell 2744, bends and magnifies the light of objects behind it. Abell 2744 lies 3.5 billion light-years away. Its mass acts like a cosmic magnifying glass. It allows JWST to see extremely faint galaxies far in the background, galaxies that would otherwise be invisible. This method helped astronomers peer deeper into the universe than ever before.

What did JWST find?

JWST used two instruments: NIRCam and NIRSpec. NIRCam captured deep images of the field. NIRSpec then observed 83 distant galaxies in detail. Among them, 33 existed within the first 1 billion years of the universe. This includes 17 galaxies from a redshift of about 7.9, meaning their light took over 13 billion years to reach us.

Scientists focused on 20 galaxies. All of them were extremely small. They had stellar masses 100 times smaller than the Milky Way. But they were intense. They produced huge amounts of light and energy, considering their size. Their light was filled with ionizing radiation. That’s the kind of light that can break hydrogen atoms apart, exactly what’s needed for reionization.

Why weren’t these galaxies seen before?

Before JWST, we couldn’t see these galaxies. They were too small and too faint. Even the Hubble Space Telescope couldn’t detect them. But JWST’s large mirror and sensitive instruments made it possible. The key was combining JWST’s power with gravitational lensing. That allowed astronomers to spot extremely faint galaxies magnified by the foreground cluster. Also, JWST’s spectrograph, NIRSpec, helped measure their light with precision. It confirmed their distance, age, and chemical makeup.

One of the most interesting galaxies of the study, dubbed 41028 (the green oval at center), has an estimated stellar mass of just 2 million Suns, comparable to the masses of the largest star clusters in our own Milky Way galaxy. Credit: NASA/ESA/CSA/Bezanson et al. 2024 and Wold et al. 2025
One of the most interesting galaxies of the study, dubbed 41028 (the green oval at center), has an estimated stellar mass of just 2 million Suns, comparable to the masses of the largest star clusters in our own Milky Way galaxy. Credit: NASA/ESA/CSA/Bezanson et al. 2024 and Wold et al. 2025

This discovery is a huge step forward. It solves a major puzzle of cosmic history. For decades, scientists asked: Who reionized the universe? Now, we have a strong answer. A group of tiny galaxies, too faint to see until now, may have lit up the early cosmos. They worked together, like countless fireflies in the dark, to push back the cosmic fog. JWST has shown us that size doesn’t always matter. Even the smallest galaxies can shape the universe in big ways. JWST’s mission will continue to peel back the layers of time, one light-year at a time.

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Soumyadeep Mukherjee

Soumyadeep Mukherjee

Soumyadeep Mukherjee is an award-winning astrophotographer from India. He has a doctorate degree in Linguistics. His work extends to the sub-genres of nightscape, deep sky, solar, lunar and optical phenomenon photography. He is also a photography educator and has conducted numerous workshops. His works have appeared in over 40 books & magazines including Astronomy, BBC Sky at Night, Sky & Telescope among others, and in various websites including National Geographic, NASA, Forbes. He was the first Indian to win “Astronomy Photographer of the Year” award in a major category.

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