JWST has captured Centaurus A in unprecedented mid-infrared detail, piercing dust to expose the active galaxy’s core, warm dust filaments and structures left by an ancient collision.
11 million light-years away, Centaurus A is close enough for Webb to resolve features earlier visible-light and near-infrared images from ESO, Hubble and Spitzer largely left obscured.
Scientists say the galaxy merged with another roughly 2 billion years ago, a crash whose warped central structure and S-shaped ribbons show how mergers rearrange gas and dust over time.
The image also highlights the role of Centaurus A’s feeding supermassive black hole, whose energy and jets can both trigger and suppress star formation in surrounding material.
Released on July 6, the observation arrives near the end of Webb’s fourth science year, underscoring the telescope’s ability to probe how galaxies grow and evolve.
What theories explain the mysterious S-shaped dust cloud Webb discovered at the heart of Centaurus A?
How will this new image shape the fierce global competition for Webb's limited observation time in the next cycle?
How can a single black hole act as both a creator and a destroyer of stars within the same galaxy?
JWST Resolves Millions of Stars in Centaurus A: Unveiling the Aftermath of a Galactic Collision and Black Hole Activity
Overview
In July 2026, the James Webb Space Telescope (JWST) used its NIRCam to capture highly detailed infrared images of Centaurus A, delivering groundbreaking insights into this galaxy. These new observations offer an unprecedented view, revealing intricate details that were previously hidden by dust and gas. Thanks to JWST’s advanced infrared capabilities, astronomers can now see a dense field of millions of individual stars within Centaurus A. This allows them to peer through obscuring material and gain a much clearer understanding of the galaxy’s stellar composition and distribution, marking a major step forward in galactic research.