M98 | NGC 4192 | Spiral Galaxy | Coma Berenices | 44,000,000 Light Years Away
Messier 98 is a barred spiral galaxy located in the constellation Coma Berenices. Charles Messier cataloged it in 1781, and it is situated approximately 44 million light-years away from Earth. With a diameter of about 58,000 light-years, Messier 98 is part of the Virgo Cluster, a rich collection of galaxies.
The distinctive feature of Messier 98 is its prominent central bar structure, which contributes to its classification as a barred spiral galaxy. The central bar is surrounded by tightly wound spiral arms, where regions of active star formation are prevalent. Observations of Messier 98 provide astronomers with valuable data on the dynamics of barred spiral galaxies, the distribution of stellar populations, and the processes influencing star formation in these cosmic structures.
Messier 98’s membership in the Virgo Cluster places it within a complex cosmic environment where gravitational interactions between galaxies play a crucial role in shaping their morphology. As part of ongoing studies exploring galaxy clusters, Messier 98 offers astronomers insights into the collective properties and interactions among galaxies in this rich galactic neighborhood. The study of Messier 98, with its unique features and position in the Virgo Cluster, contributes to our broader understanding of the complexities of galactic evolution within the vast cosmic tapestry.