(NGC 4548) M91 Galaxy
What is M91 Galaxy - NGC 4548
M91 Galaxy (NGC 4548) is a spiral galaxy located in the constellation Coma Berenices. It is part of the Virgo Cluster, a rich cluster of galaxies in the Virgo Supercluster.
What Type of Galaxy is M91 Galaxy - NGC 4548
M91 Galaxy (NGC 4548) is classified as a spiral galaxy. It exhibits a well-defined spiral structure with a central bulge, spiral arms, and a disk.
How old is M91 Galaxy - NGC 4548
Determining the exact age of M91 Galaxy (NGC 4548) is challenging, but it is estimated to be approximately around 9 to 10 billion years. Age estimation involves studying the galaxy's stellar populations and the history of star formation.
M91 Galaxy - NGC 4548 Size in Light Years
The size of M91 Galaxy (NGC 4548) encompasses an extensive region of approximately about 80,000 to 90,000 light-years.
M91 Galaxy - NGC 4548 Diameter in Light Years and Compared to Milky Way
The diameter of M91 Galaxy (NGC 4548) is approximately about 80,000 to 90,000 light-years. Compared to the Milky Way, M91 is slightly smaller in size, making it a galaxy of considerable dimensions.
M91 Galaxy - NGC 4548 Mass in Solar Masses
Estimates suggest that the mass of M91 Galaxy (NGC 4548) is approximately about 60 billion to 80 billion solar masses. The galaxy's mass influences its gravitational interactions and internal processes, placing it within the range of spiral galaxies.
M91 Galaxy - NGC 4548 Location
M91 Galaxy (NGC 4548) is located in the constellation Coma Berenices. Positioned in the northern celestial hemisphere, Coma Berenices is home to a cluster of galaxies, and M91 is one of its notable members.
10 Interesting Fun Facts about M91 Galaxy - NGC 4548
- M91 was discovered by Charles Messier in 1781, making it the 91st entry in his catalog.
- It is part of the Virgo Cluster, a massive collection of galaxies in close proximity.
- The galaxy's spiral arms contain regions of active star formation and bright, young stars.
- M91 has been studied to understand the dynamics and interactions within galaxy clusters.
- It is part of the larger Coma I Group, a collection of galaxies associated with the Coma Cluster.
- Observations of M91 contribute to our understanding of the formation and evolution of spiral galaxies.
- The galaxy's location in the Virgo Cluster provides insights into the large-scale structure of the universe.
- M91 has been observed in various wavelengths, including radio and infrared, revealing different aspects of its properties.
- Studies of the Virgo Cluster, including M91, contribute to the understanding of galaxy evolution in dense environments.
- The galaxy's proximity to other Virgo Cluster members makes it a valuable target for comparative studies.
M91 Galaxy - NGC 4548 Distance from Earth in Light Years and Miles / Km
M91 Galaxy (NGC 4548) is situated at an approximate distance of about 60 million light-years from Earth. Converting this distance, it is approximately 3.52e+20 miles (5.66e+20 km) away. This distance places it in the realm of relatively distant galaxies, and observations of M91 contribute to our understanding of spiral galaxy properties and their interactions within galaxy clusters.