Webb Telescope Sees Through Dust in Galaxy NGC 5134

On February 20, 2026, the James Webb Space Telescope took a sharp picture of a spiral galaxy. Scientists call this galaxy NGC 5134. It is about 65 million light-years away from Earth. This distance is very far, but NGC 5134 is close in space terms. Usually, thick dust blocks our view of stars inside spiral arms. The new image shows stars clearly because it uses infrared light. Infrared light can pass through dark dust clouds that hide stars. This helps scientists see the true shape of the galaxy.

Two special cameras helped the telescope take this clear photo. The first camera is called MIRI. It collects mid-infrared light from warm dust. This dust is made of tiny solid particles floating between stars. Warm dust often means new stars are forming there. The second camera is called NIRCam. It records near-infrared light from the stars themselves. This light shows us groups of stars in the spiral arms. Using both cameras gave scientists two different views at once. They could separate the glow of dust from the light of stars. This mix creates a complete map of the galaxy's inside parts.

Studying close galaxies like NGC 5134 helps us understand distant ones. Faraway galaxies look like blurry dots because they are too far. We cannot see their shapes or how stars form there. NGC 5134 acts like a template or a guide. Scientists use its clear details to guess what blurry distant galaxies look like. This helps them learn how galaxies grow over billions of years. Galaxies change shape and make new stars all the time. The data from this study makes our models more accurate. It turns guesses into facts based on real evidence.