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The Galaxy is part of the Local Group, a collection of galaxies of comparable size, including the Milky Way and the M31. The Group also contains the Triangulum Galaxy and the Magellanic Clouds. The Milky Way and the Galaxy are a part of the Virgo Supercluster and the Centaurus-A/Cen-A supercluster. The Local Group is considered to be a part of a larger group of galaxies called the Local Supercluster. The Virgo Supercluster contains a number of massive galaxy clusters, such as Virgo, Fornax, and the Coma cluster.
The Galaxy is classified as a spiral galaxy. Spiral galaxies contain a flat, disk-shaped main body, or “spiral disk,” that includes a central bulge. The spiral disk has the shape of a logarithmic spiral and contains many spiral arms. The Galaxy has a central bulge about 1,500 light years across. The bulge is a flattened central part of the disk that contains old stars. The stars in the bulge are about three times more massive than the stars in the rest of the galaxy.
Several spiral galaxies are classified as “grand design” or “flocculent” galaxies. The term “grand design” was coined by Sir James Jeans to describe galaxies with bright spiral arms that are free of dust and gas and are bright in the visible wavelengths. Grand design galaxies are symmetrical, meaning they are similar on opposite sides of the galaxy. Flocculent galaxies have broken-up spiral arms, and are less symmetrical than grand design galaxies.
Since the advent of star-mapping techniques, it has been discovered that many spiral galaxies are not symmetrical, but have irregularities in the spiral arms and “transition 0b46394aab