Classification of Galaxy

Classification of Galaxy What is Galaxy? A galaxy is a large collection of stars, gas, dust, and other celestial objects held together by gravity. Galaxies come in a variety of shapes and sizes, ranging from small irregularly shaped galaxies with just a few hundred million stars to massive spiral and elliptical galaxies with trillions of stars. The stars within a galaxy are organized into various structures, such as spiral arms, bulges, and halos. Galaxies also contain supermassive black holes at their centers, as well as clouds of gas and dust that form new stars. The study of galaxies and their properties is an important area of research in astronomy and astrophysics, providing insight into the formation and evolution of the universe. Classification of Galaxy Galaxies are classified based on their morphology or structure. The most common classification system was developed by Edwin Hubble in 1926, known as the Hubble sequence, which divides galaxies into three main catego...