Located in the southern part of the constellation Columba, NGC 1792 is a tempestuous and highly energetic spiral galaxy.

NGC 1792 is approximately 36.4 million light-years away from Earth, positioned to the south of the constellation Columba, bordering Caelum.

This galaxy, also known as AGC 24019 or LEDA 16709, was identified by Scottish astronomer James Dunlop on October 4, 1826.

The chaotic appearance of NGC 1792 features dust interspersed throughout its disk.

This galaxy is abundant in neutral hydrogen gas, leading to a high rate of new star formation.

“Astronomers find NGC 1792 intriguing, as its tumultuous appearance implies,” stated Hubble astronomers.

“Classified as a starburst galaxy, it serves as a dynamic site for star formation, with spiral arms rich in star-forming regions.”

“Surprisingly, it is quite luminous for its mass,” they added.

“This galaxy is approaching its larger neighbor, NGC 1808. The intense gravitational interaction between the two is believed to have stirred the gas reserves of the galaxy.”

“Consequently, star formation is more concentrated on the side where the gravitational pull is stronger.”

“This makes NGC 1792 an ideal subject for astronomers aiming to comprehend the intricate interactions among gas, star clusters, and supernovae within galaxies.”

In 2020, astronomers utilized Hubble’s Wide Field Camera 3 (WFC3) to observe NGC 1792.

The recent images incorporate additional WFC3 data collected in 2025, enriching our understanding of the turbulent astrophysical activity in the galaxy.

“The red light radiating in the arms signals H-alpha emission from a dense cloud of hydrogen molecules,” remarked the astronomers.

“Stars are born within these clouds and emit strong ultraviolet light.”

“This process ionizes the surrounding gas, causing it to emit light at a distinctive red wavelength, a clear indicator of a new star.”