M32, also known as Messier 32 or NGC 221, is a fascinating galaxy located in the constellation Andromeda. Spanning approximately 8,000 light-years in diameter, M32 is one of the many satellite galaxies orbiting the famous Andromeda Galaxy (M31). In this review, we will explore the characteristics of M32 and determine its classification among the different galaxy types, including spiral, barred spiral, elliptical, or irregular.
To determine the type of galaxy M32 belongs to, we must carefully analyze its structure, shape, and other defining features. Unlike spiral galaxies that exhibit prominent arms or barred spiral galaxies with a central bar structure, M32 possesses a distinct elliptical shape. Elliptical galaxies are characterized by their smooth, oval-shaped appearance and lack of defined spiral arms.
M32's elliptical shape is indicative of its classification as an elliptical galaxy. These galaxies are often found in dense regions of the universe, such as galactic clusters, where gravitational interactions between galaxies lead to mergers and the formation of elliptical shapes. M32's proximity to the massive Andromeda Galaxy also supports the idea that it is an elliptical galaxy, as these types of galaxies are frequently found in close proximity to larger galaxies
Why does an elliptical galaxy have few young stars?
There is very little gas and dust. Because there is not much gas and dust, there's not enough material to make new stars. In general, the stars in elliptical galaxies are old, red stars.
Why do elliptical galaxies contain only population II stars?
Elliptical galaxies, such as M87 (left), have very little gas and dust. Because gas and dust are found in the clouds that are the birthplaces of stars, we should expect to see very few young stars in elliptical galaxies. In fact, elliptical galaxies contain primarily old, red stars (also known as Population II stars).
Why are elliptical galaxies hot?
As a consequence of their formation and galactic dynamics, big elliptical galaxies are often found near the centers of groups and rich clusters. It is natural that the diffuse thermal gas contained in these hot stellar systems is also hot.
How does this difference explain the lack of hot young stars in elliptical galaxies?
How does this difference explain the lack of hot, young stars in elliptical galaxies. Like the halos of spiral galaxies, elliptical galaxies lack cool gas and so do not have much star formation. As a result, we see few hot, young stars in these galaxies.
Why do elliptical galaxies not produce new young stars?
Unlike spirals, elliptical galaxies usually contain little gas and dust and show very little organization or structure. The stars orbit around the core in random directions and are generally older than those in spiral galaxies since little of the gas needed to form new stars remains.