Hubble Telescope Captures New Image of Distant Spiral Galaxy NGC 3137
Similar Articles
Hubble Telescope Captures Detailed Image of Distant Spiral Galaxy NGC 3137
Hubble Telescope Captures Image of Distant Barred Spiral Galaxy IC 486
Hubble Telescope Marks 36th Anniversary with Detailed Image of Trifid Nebula
NASA's Chandra Observatory Discovers Distant 'X-Ray Dot' Object
Gravitational Lens Reveals Distant Supernova, Aiding Measurement of Universe's Expansion
NASA's Hubble Space Telescope has captured a new image of the spiral galaxy NGC 3137, located 53 million light-years away. The galaxy is part of the NGC 3175 group, which contains more than 500 dwarf galaxy candidates alongside its two large spiral galaxies.
Facts First
- Hubble Space Telescope captured a new image of the spiral galaxy NGC 3137
- Galaxy is located 53 million light-years away in the constellation Antlia
- NGC 3137 is part of the NGC 3175 group, which contains two large spiral galaxies
- Researchers have found more than 500 dwarf galaxy candidates within the NGC 3175 group
- Both the NGC 3175 group and our Local Group contain a number of smaller dwarf galaxies
What Happened
NASA's Hubble Space Telescope captured a new image of the spiral galaxy NGC 3137. The galaxy is located 53 million light-years away in the constellation Antlia (the Air Pump). NGC 3137 is part of the NGC 3175 group of galaxies, which contains two large spiral galaxies: NGC 3137 and NGC 3175.
Why this Matters to You
This observation contributes to our understanding of galaxy formation and structure. The discovery of more than 500 dwarf galaxy candidates within the NGC 3175 group may help scientists better understand how galaxy groups, including our own Local Group that contains the Milky Way, form and evolve.
What's Next
The Hubble Space Telescope has also observed the other large spiral galaxy in the group, NGC 3175. Further analysis of these images and data could provide more insights into the composition and dynamics of the NGC 3175 group and its many dwarf galaxy candidates.