NASA's Hubble Space Telescope has captured a stunning image of the spiral galaxy NGC 1792, revealing a chaotic and highly active storm of new stars. The galaxy, located over 50 million light-years from Earth in the constellation Columba, appears to be in turmoil, with bright patches of star-forming regions scattered throughout its disk.
The new image, which includes data collected by Hubble in 2025, provides a deeper look at the tumultuous activity taking place within the galaxy. The galaxy's arms are adorned with numerous sparkling blue and glowing red regions - star clusters and star-forming nebulae - that are thought to be the result of strong gravitational interactions between NGC 1792 and its larger neighbor, NGC 1808.
The Hubble Space Telescope image shows the galaxy in a state of constant transformation. The swirling clouds of dark reddish dust within the arms give way to bright patches of light where stars are being born at an incredible rate. These newly formed stars shine powerfully with ultraviolet radiation, which causes hydrogen gas to emit a distinctive red light known as H-alpha.
This image not only provides astronomers with valuable insights into the complex interactions between gas and star clusters in galaxies but also underscores the enduring importance of the Hubble Space Telescope in advancing our understanding of the universe.
The new image, which includes data collected by Hubble in 2025, provides a deeper look at the tumultuous activity taking place within the galaxy. The galaxy's arms are adorned with numerous sparkling blue and glowing red regions - star clusters and star-forming nebulae - that are thought to be the result of strong gravitational interactions between NGC 1792 and its larger neighbor, NGC 1808.
The Hubble Space Telescope image shows the galaxy in a state of constant transformation. The swirling clouds of dark reddish dust within the arms give way to bright patches of light where stars are being born at an incredible rate. These newly formed stars shine powerfully with ultraviolet radiation, which causes hydrogen gas to emit a distinctive red light known as H-alpha.
This image not only provides astronomers with valuable insights into the complex interactions between gas and star clusters in galaxies but also underscores the enduring importance of the Hubble Space Telescope in advancing our understanding of the universe.