NGC 5235

NGC 5235 is a barred spiral galaxy located in the constellation Centaurus. It was discovered on May 6, 1834, by the astronomer John Herschel.

Characteristics:

NGC 5235 is classified as a barred spiral galaxy, indicating the presence of a central bar-shaped structure composed of stars and gas. From this bar, spiral arms emanate outwards, giving the galaxy its distinctive spiral shape. The galaxy is at an estimated distance of around 60 million light-years from Earth. The physical size of NGC 5235 is estimated to be approximately 80,000 light-years in diameter, making it slightly smaller than our own Milky Way galaxy. Its luminosity is also significant, although specific details regarding its absolute magnitude may vary depending on the source.

Location and Observational Data:

The galaxy is located in the constellation Centaurus. Its coordinates are approximately Right Ascension 13h 37m 23.1s and Declination -29° 53′ 45″. These coordinates are used by astronomers to precisely locate and study the galaxy.

Significance:

NGC 5235 is of interest to astronomers as a typical example of a barred spiral galaxy. Its structure and composition provide insights into the formation and evolution of spiral galaxies. It is often studied as part of larger surveys of galaxies to understand the distribution and properties of galaxies in the local universe. Further research includes the study of star formation regions within the galaxy and the properties of its central bulge and spiral arms.