Historical background Until the 1920's it was believed that our Milky Way was all there was to the...

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Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher Immanuel Kant (1724-1804) suggested that some of the nebulae might be other star systems Using the 100 inch telescope on Mount Wilson, Edwin Hubble was able to resolve individual stars in several bright spiral-shaped "nebulae" including the Andromeda Galaxy (M31).

Transcript of Historical background Until the 1920's it was believed that our Milky Way was all there was to the...

Page 1: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

Historical background

• Until the 1920's it was believed that our Milky Way was all there was to the universe.

• As early as the 18th century, the philosopher Immanuel Kant (1724-1804) suggested that some of the nebulae might be other star systems

• Using the 100 inch telescope on Mount Wilson, Edwin Hubble was able to resolve individual stars in several bright spiral-shaped "nebulae" including the Andromeda Galaxy (M31).

Page 2: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

What is a galaxy ?

• A galaxy is a large assembly of stars, gas, dust, and dark matter, held together by gravity.

• Galaxies can be classified in several ways. The most common is a system developed by Edwin Hubble, which is based on the shape of galaxies.

Page 3: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

types of galaxies

there are four main classes (as classified by Hubble)

1) Spiral galaxies • Disk + central bulge 2 ) A ‘subspecies’ of

spiral galaxy is the class of barred spirals.

• Disk + central bulge with bar

Page 4: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

3) Elliptical galaxies • All bulge, elliptical shape,

no disk; stars but little or no gas

4) Irregular galaxies • Irregular shape

Page 5: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

• The class of spiral galaxies is further divided into classes Sa, Sb, & Sc.

• Sa galaxies have big central bulges, tightly wound spiral arms, & relatively small amount of interstellar gas.

• Sc Galaxies have small bulges, loosely wound spiral arms, & relatively large amount of gas.

• Sb Galaxies are intermediate between Sa & Sc. • our own galaxy is an Sb galaxy, as is M31 & M51

Page 6: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

M51 whirlpool galaxy (Sc type) M31 Andromeda Galaxy (Sb type)

Sombrero galaxy (Sa type)M85 a ‘lenticular’ galaxy (on left) mostly bulge, a little disk (type S0)

Page 7: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

M91 in Virgo Cluster (type SBb)

M95 (type SBb)

Page 8: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

• Elliptical galaxies contain very little gas and dust, and the gas that is present is very hot & diffuse. Consequently, there is no current star formation in elliptical galaxies. These galaxies are not disks, but flattened spheres called ellipsoids. Astronomers classify them as E0 for nearly spherical galaxies through E7 for very elongated ones.

• The largest galaxies in the Universe are giant Ellipticals. They can contain trillion stars or more, and span as much as one million light years – about 10 times the diameter of the Milky Way.

Page 9: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

M32 dwarf elliptical galaxy, satellite of M31

M60 giant elliptical galaxy in Virgo Cluster (on right)

M87 giant elliptical galaxy, the dominant Galaxy in Virgo Cluster

Page 10: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

• Irregular galaxies have no obvious spiral or elliptical

structure. • Irregular galaxies tend to

contain lots of gasses and dust.

NGC 1569 is a dwarf irregular galaxy

Large Magellanic Cloud, best known irregular galaxy

Page 11: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

Astronomers also categorize galaxies by how much energy they produce in their cores. A particular class is called "active" galaxies, because they produce much more energy than "normal" galaxies.

The most powerful active galaxies are quasars.

Page 12: Historical background Until the 1920's it was believed that our Milky Way was all there was to the universe. As early as the 18th century, the philosopher.

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