Astronomers utilizing the NASA/ESA Hubble Space Telescope have captured breathtaking new images of sections of the spiral galaxy known as NGC 45.
This Hubble image depicts the outer arm of the NGC 45, a spiral galaxy approximately 22 million light-years distant in the Cetus constellation. This color image was generated from individual exposures taken in both visible and near-infrared light using Hubble’s Wide Field Camera 3 (WFC3). The colors have been produced by assigning different hues to each monochromatic image captured through various filters. Image credits: NASA/ESA/Hubble/D. Calzetti/R. Chandar/Mhözsaraç.
NGC 45 is located about 22 million light-years away within the constellation of Cetus.
Also referred to as DDO 223, ESO 473-1, or Leda 930, this galaxy spans roughly 81,000 light-years in diameter.
The discovery of NGC 45 dates back to November 11, 1835, by British astronomer John Herschel.
“The data from Hubble utilized to create this portrait of NGC 45 was obtained from two complementary observational programs,” stated Hubble astronomers.
“Initially, we leveraged Hubble’s capability to capture light from ultraviolet to near-infrared ranges to broadly observe galaxies and examine star formation within them.”
“In the second program, we focused on many of the same nearby galaxies as the first, narrowing down to a specific wavelength of red light known as H-alpha.”
“Star-forming nebulae emit strong H-alpha light, and several of these areas can be identified by their bright pink red color throughout NGC 45.”
“These observational programs aim to investigate star formation across galaxies of varying sizes, structures, and separations, making NGC 45 a particularly compelling target.”
Though it may appear to be an ordinary spiral galaxy, NGC 45 is actually a remarkable low surface brightness galaxy.
“Low surface brightness galaxies are more intriguing than the evening sky and are incredibly challenging to detect,” articulated the researchers.
“They possess relatively fewer stars in relation to the amount of gas and dark matter they contain, making them appear unexpectedly faint.”
“Since the accidental discovery of the first low-surface brightness galaxies in 1986, scientists have learned that 30-60% of all galaxies may fall within this category.”
“Investigating these elusive galaxies is crucial for understanding the formation and evolution of galaxies, and Hubble’s sensitive instruments are well-suited for this task.”
Source: www.sci.news
