The Andromeda Galaxy, also known as Messier 31, M31, or NGC 224, is a spiral galaxy located about 2.537 million light-years from Earth in the constellation of Andromeda. It is the nearest spiral galaxy to the Milky Way, making it a prominent and well-studied object in the night sky.
The Andromeda Galaxy is approximately 220,000 light-years in diameter, making it the largest galaxy in the Local Group, which also includes the Milky Way, the Triangulum Galaxy, and about 54 other smaller galaxies. It is estimated to contain about one trillion stars, dwarfing the estimated 100 billion stars in the Milky Way.
The Andromeda Galaxy has a prominent bulge at its center, surrounded by a large, flat disk of stars, gas, and dust. It exhibits spiral arms that wrap around its nucleus, giving it a classic spiral galaxy appearance. The galaxy also contains a number of satellite galaxies, including M32, M110, and others.
The Andromeda Galaxy is visible to the naked eye under dark sky conditions and is a popular target for amateur and professional astronomers. It appears as a faint, elongated smudge in the night sky and can be best observed during the late summer and fall months in the Northern Hemisphere.
The formation and evolution of the Andromeda Galaxy are of great interest to astronomers. It is believed to have formed from the gravitational collapse of a protogalactic cloud of gas and dust, eventually forming stars and the structures seen today. Andromeda is on a collision course with the Milky Way and is predicted to collide with our galaxy in about 4.5 billion years, forming a new galaxy often referred to as "Milkomeda."