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Stars and Galaxies
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have a disk but no arms

have little or no excess gas and dust

Slide 62

Irregular Galaxies

Irregular Galaxies

any galaxy that isn’t a Spiral, Elliptical, or Lenticular

usually have lots of gas and dust and young stars

may have a distorted shape from interaction with another galaxy

Slide 63

Irregular Galaxies

Irregular Galaxies

Slide 64

Collisions!

Collisions!

We now think that galaxies in groups and clusters often collide

The Milky Way is moving at 300,000 mph toward the Andromeda Galaxy

They may collide in about 5 billion years

Stars don’t usually collide

New orbits, gas piles up to form new stars

Slide 65

Interacting

Interacting

Slide 66

the Antennae or Mice

the Antennae or Mice

Slide 67

The occasional results of two galaxies colliding: ringed galaxies

The occasional results of two galaxies colliding: ringed galaxies

Slide 68

Various galaxies (can you identify types?)

Various galaxies (can you identify types?)

Slide 69

Supermassive black holes

Supermassive black holes

almost every medium to large galaxy we’ve check has a supermassive black hole at the center

the larger the galaxy, the more massive the black hole

we don’t know which comes first, the galaxy or the black hole

we think that these black holes are responsible for some of the galaxies with jets and lobes which give off radio waves, x-rays, etc.

Slide 70

Active galaxy

Active galaxy

Slide 71

at the center of a large galaxy

at the center of a large galaxy

Slide 72

Galaxy Clusters

Galaxy Clusters

the Local Group

includes the Milky Way, the Andromeda, and over 30 other smaller galaxies

the Virgo Cluster

hundreds to thousands of galaxies, 60 million light-years away

giant elliptical at center, formed by galactic cannibalism

the Local Group is “falling” toward the Virgo Cluster at 60 to 250 miles per second!

Slide 73

Coma Cluster

Coma Cluster

Slide 74

Superclusters!

Superclusters!

clusters are bound together in larger structures, called superclusters

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