Chapter 15 Part 2

More About Galaxies

The Local Group

The Local Group is an association (cluster) of galaxies that includes the Milky Way. The two other large members are M31 (Andromeda) and M33 (Triangulum). The rest are smaller dwarf galaxies. The illustrations of page 401 show you how the Local Group looks.

Galaxy Clusters

Galaxies are found to be in clusters. The Milky Way Galaxy is part of a cluster called the Local Group; it consists of three large spirals and about 42 dwarf elliptical and irregular galaxies. Figure 15.14 will show you the Virgo Cluster (recognize that from lab??). Figure 15.1 shows the Coma Cluster.

Superclusters

Clusters of galaxies exist in superclusters, or clusters of clusters. We are located in the Local Supercluster, and you shouldn't be surprised to find out that we aren't in the center of that; we're sitting about 20 Mpc from the center of it.

Seeing VERY FAR Out

Before we had a fully functioning Hubble Space Telescope, the detection limit for galaxies and such was about magnitude 25 (m=25). Hubble extended that in the 1990's. The Director of the Hubble Space Telescope Science Institute has 5% of Hubble's observing to use as he wishes. He doesn't have to go through the process of applying for time on the telescope. This means that he can take some scientific risks, performing observations whose outcome is really unknown. In the mid 90's, Director Bob Williams had Hubble aimed at a spot just north of the Big Dipper. Over 100 hours of exposure were taken and combined into the Hubble Deep Field (see page 435, Figure 16.18). This was an area of sky where previous survey images showed nothing! That "nothing" turned out to be full of galaxies. Some of the nearest ones in the image are over 1,000 mpc away. The faintest ones are too far and too faint for spectroscopic study. The magnitude limit was pushed down to near 30 (m=30). The newer Hubble ultra Deep Field goes about one magnitude deeper.