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Galaxies
The
Galaxies
5/12/2010
 On a clear and moonless night, away
from city lights, you can see a
marvelous sight; our own Milky Way
Galaxy.
 Galaxies are large groups of stars,
dust, and gases held together by
gravity.
 There may be 400 billion stars in our
Milky Way galaxy alone.
 Our galaxy looks milky because the
stars of the solar system are
concentrated within a flat disk; the
galactic disk.
5/12/2010
The Milky Way Galaxy:
 Imagine you are hiking in a forest.
You look around and see trees in
every direction and it seems like
you are in the center of the
forest.
 When astronomers began to
survey stars located along the
plane of the Milky Way, it seemed
like the forest; stars lay in every
direction and it seemed we were
at the center of it all.
 This is not the case however;
Earth and our solar system are
located on one of many arms of a
spinning
galaxy.
5/12/2010
Size of the Milky Way:
 It’s hard to study the Milky Way
galaxy with optical telescopes
because large quantities of
interstellar matter block our
vision.
 With the aid of radio telescopes,
scientists have partly determined
the structure of the galaxy.
 The Milky Way is a large spiral
whose disk is about 100,000 light
years wide and about 10,000 light
years thick at it’s center.
5/12/2010
Structure of the Milky Way:
 Radio telescopes reveal that the
Milky Way has at least three
distinct spiral arms, with some
signs of splintering.
 Our sun is positioned in one of
these arms about two thirds of
the way from the center, or about
30,000 light years from the
galactic nucleus.
 The stars on these arms rotate
around the galactic nucleus.
5/12/2010
 The most outward arms move the
slowest, and the ends of the arms
appear to trail.
 Our solar system makes one
revolution around the galactic
center about once every 230 million
years.
 Surrounding the galactic disk is a
nearly round halo made of thin gas
and numerous clusters of stars.
 These star clusters do not rotate as
the arms in the galaxy do.
 Although some of the star clusters
are dense space is so large that the
rotating arms pass through these
star cluster with no chance of
colliding.
5/12/2010
Types of Galaxies:
 In the mid 1700s, German
philosopher Immanuel Kant
proposed that fuzzy patches of
light scattered among the stars
were actually distant galaxies like
our Milky Way.
 Today we know that the universe
includes hundreds of billions of
galaxies, each containing hundreds
of billions of stars.
 From these hundreds of billions of
galaxies, scientists have identified
several basic types.
5/12/2010
Spiral Galaxies:
 Spiral galaxies are usually disk
shaped, with a greater
concentration of stars near their
centers.
 There are numerous variations of
them however. Viewed broadside,
the arms are often seen extending
from the center nucleus and
sweeping gracefully away.
 The outermost arms of these
stars rotate the slowest, giving
the galaxy the appearance of a
pinwheel.
5/12/2010
Types of spiral galaxies
 One type of spiral galaxy,
however, has it’s arms arranged
in the shape of a bar, which
rotates as a rigid system.
 This type is called a barred
spiral galaxy.
 Recent evidence indicates our
Milky way may be a barred spiral
galaxy.
 Spiral galaxies are generally
quite large.
 About 10 percent of all galaxies
are thought to be barred spirals
and another 20 percent are
spiral
5/12/2010galaxies.
Elliptical Galaxies:
 About 60 percent of galaxies are
classified as elliptical galaxies.
 Elliptical galaxies range in shape
from round to oval.
 Although most are small, the
very largest known galaxies;
200,000 light years in diameter,
are elliptical.
 This type of galaxy does not
have spiral arms.
5/12/2010
Earth Science 25.3 The Universe
Irregular Galaxies:
 Only 10 percent of the known
galaxies have irregular shapes
and are classified as irregular
galaxies.
 The best known irregular
galaxies, the large and small
Magellanic Clouds, are easily
visible from the Southern
Hemisphere with the unaided
eye.
 These clouds are our nearest
neighbors; only 150,000 light
years away.
5/12/2010
Earth Science 25.3 The Universe
Irregular Galaxies:
 In addition to shape and size,
one of the major differences
among different types of
galaxies is the age of their
stars.
 Irregular galaxies are
composed mostly of young
stars, while elliptical galaxies
contain old stars.
 The Milky way and other spiral
galaxies have both young and
old stars, with the youngest
stars located in the arms.
5/12/2010
Earth Science 25.3 The Universe
Galaxy Clusters:
 Once astronomers discovered
that stars were found in
groups, they wondered
whether galaxies also were
grouped or just randomly
distributed among the
universe.
 They found that, like stars,
galaxies are grouped in
clusters.
 Some clusters may contain
thousands of galaxies. Our own
galaxy, called the Local Group,
contains at least 28 galaxies.
5/12/2010
Earth Science 25.3 The Universe
Galaxy Clusters:
 Of these 28 galaxies
located in our cluster; 3 are
spiral galaxies, 11 are
irregular galaxies, and 14
are elliptical galaxies.
 Galaxy clusters also make
up huge groups called
superclusters, which in turn
make up vast threadlike
structures called filaments.
 These filaments are the
largest known structures in
the universe.
5/12/2010
superclusters
Earth Science 25.3 The Universe
Quasars:
 In the 1960s, astronomers
discovered objects that
were very bright and very
far away.
 They called them quasistellar objects, or quasars,
since they looked like stars.
 Because it takes their light
billions of years to reach
Earth, quasars must have
existed when the universe
was very young.
5/12/2010
Earth Science 25.3 The Universe
Quasars:
 Quasars must emit huge
amounts of radiation, or
they would be too dim for
us to detect.
 The leading theory at
present is that they are
massive black holes in the
centers of very young
galaxies.
5/12/2010
5/12/2010
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