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Telescopes

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Telescopes Characteristics of Stars Lives of Stars Star Systems and Galaxies The Expanding Universe Electromagnetic Radiation The electromagnetic spectrum includes ... – PowerPoint PPT presentation

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Title: Telescopes


1
Table of Contents
  • Telescopes
  • Characteristics of Stars
  • Lives of Stars
  • Star Systems and Galaxies
  • The Expanding Universe

2
Electromagnetic Radiation
- Telescopes
  • The electromagnetic spectrum includes the entire
    range of radio waves, infrared radiation, visible
    light, ultraviolet radiation, X-rays, and gamma
    rays.

3
Types of Telescopes
- Telescopes
  • A refracting telescope uses convex lenses to
    focus light. A reflecting telescope has a curved
    mirror in place of an objective lens.

4
Four Views of the Crab Nebula
- Telescopes
  • Different type of telescopes collect
    electromagnetic radiation at different
    wavelengths. Astronomers are able to learn a
    great deal about the Crab Nebula by examining
    these different images. The images are shown at
    different scales.

5
Building Vocabulary
- Telescopes
  • Carefully read the definition of each Key Term.
    Also read the neighboring sentences. Then write a
    definition of each Key Term in your own words.

Key Terms
Examples
A telescope that uses lenses or mirrors to
collect and focus visible light is called an
optical telescope.
telescope
A telescope helps to make faraway objects look
closer. It is a very valuable tool in astronomy.
A refracting telescope uses convex lenses to
gather and focus light.
electromagnetic radiation
Electromagnetic radiation is a type of energy
that travels as waves through space. It includes
visible light.
A convex lens is a piece of transparent glass,
curved so that the middle is thicker than the
edges.
visible light
Scientists call the light you can see visible
light.
A reflecting telescope uses a curved mirror to
collect and focus light.
wavelength
The distance between the crest of one wave and
the crest of the next wave is called wavelength.
Devices used to detect radio waves from objects
in space are called radio telescopes.
spectrum
If you shine white light through a prism, the
light spreads out to make a range of different
colors with different wavelengths, called a
spectrum.
An observatory is a building that contains one or
more telescopes.
6
Links on Telescopes
- Telescopes
  • Click the SciLinks button for links on telescopes.

7
Telescopes
- Telescopes
  • Click the Video button to watch a movie about
    telescopes.

8
The Hubble Space Telescope
- Telescopes
  • Click the Video button to watch a movie aboutthe
    Hubble Space Telescope.

9
End of SectionTelescopes
10
Star Size
- Characteristics of Stars
  • Stars vary greatly in size. Giant stars are
    typically 10 to 100 times larger than the sun and
    more than 1,000 times the size of a white dwarf.

11
Star Spectrums
- Characteristics of Stars
  • Astronomers use line spectrums to identify the
    chemical elements in a star. Each element
    produces a characteristic pattern of spectral
    lines.

12
Parallax
- Characteristics of Stars
  • Parallax is the apparent change in position of an
    object when you look at it from different places.

13
Measuring Distances to Stars
- Characteristics of Stars
  • Astronomers often use parallax to measure
    distances to nearby stars.

14
The Hertzsprung-Russell Diagram
- Characteristics of Stars
  • Astronomers use H-R diagrams to classify stars
    and to understand how stars change over time.

15
Using Prior Knowledge
- Characteristics of Stars
  • Before you read, write what you know about the
    characteristics of stars in a graphic organizer
    like the one below. As you read, write what you
    learn.

What You Know
  1. Stars are bright and hot.
  2. Distances between stars are often measured in
    light-years.
  3. The sun is a yellow star.

What You Learned
  1. Stars are classified by color, temperature, size,
    composition, and brightness.
  2. Light travels 9.5 million million kilometers in
    one year.
  3. The sun has a surface temperature of about
    5,800ºC.

16
More on Types of Stars
- Characteristics of Stars
  • Click the PHSchool.com button for an
    activityabout types of stars.

17
End of SectionCharacteristics of Stars
18
The Lives of Stars
- Lives of Stars
  • A stars life history depends on its mass. After
    a star runs out of fuel, it becomes a white
    dwarf, a neutron star, or a black hole.

19
The Lives of Stars Activity
- Lives of Stars
  • Click the Active Art button to open a browser
    window and access Active Art about the lives of
    stars.

20
Black Holes
- Lives of Stars
  • The remains of the most massive stars collapse
    into black holes. Here, a black hole is shown
    pulling matter from a companion star.

21
Sequencing
- Lives of Stars
  • As you read, make a flowchart that shows the
    stages in the life of a star like the sun. Write
    each step of the process in a separate box in the
    flowchart in the order that it occurs.

Life Cycle of a Sun-Like Star
Protostar forms from a nebula.
A star is born as fusion begins.
The star stays on the main sequence for billions
of years.
The star begins to run out of fuel.
The star becomes a red giant, then a white dwarf,
then a black dwarf.
22
End of SectionLives of Stars
23
Structure of the Milky Way
- Star Systems and Galaxies
  • Our solar system is located in a spiral galaxy
    called the Milky Way. From the side, the Milky
    Way appears to be a narrow disk with a bulge in
    the middle. The galaxys spiral structure is
    visible only from above or below.

24
Scientific Notation
- Star Systems and Galaxies
  • The bright star Deneb is about 3,230 light years
    from Earth. To express this number in scientific
    notation, first insert a decimal point in the
    original number so that you have a number between
    one and ten. In this case, the numberis 3.23.
  • To determine the power of 10, count the number of
    places that the decimal point moved. Here the
    decimal point moved three places.
  • 3,230 light-years 3.23 X 103 light-years

25
Scientific Notation
- Star Systems and Galaxies
  • Practice Problem
  • The sun takes about 220,000,000 years to revolve
    once around the center of the galaxy. Express
    this length of time in scientific notation.
  • 2.2 X 108 years

26
Building Vocabulary
- Star Systems and Galaxies
  • Carefully read the definition of each Key Term.
    Also read the neighboring sentences. Then write a
    definition of each Key Term in your own words.

Key Terms
Examples
binary star
Star systems that have two stars are called
double stars or binary stars.
A galaxy is a huge group of single stars, star
systems, star clusters, dust, and gas bound
together by gravity.
Astronomers define the universe as all of space
and everything in it.
eclipsing binary
An eclipsing binary is a star system in which one
star cannot be seen at times because the other
star blocks the light.
Scientific notation uses powers of ten to write
very large or very small numbers in shorter form.
Spiral galaxies appear to have a bulge in the
middle and arms that spiral outward, like
pinwheels.
open cluster
Open clusters have a loose, disorganized
appearance and contain no more than a few
thousand stars.
Elliptical galaxies look like round or flattened
balls.
Irregular galaxies do not have regular shapes.
Since quasi means something like in Latin,
these objects were given the name quasi-stellar
objects, or quasars.
globular cluster
Globular clusters are large groupings of older
stars.
27
Links on Galaxies
- Star Systems and Galaxies
  • Click the SciLinks button for links on galaxies.

28
End of SectionStar Systems and Galaxies
29
Retreating Galaxies
- The Expanding Universe
  • All distant galaxies are moving rapidly away from
    our galaxy and from each other.

30
Speeding Galaxies
- The Expanding Universe
  • Use the graph to answer the questions about
    moving clusters of galaxies.

31
Speeding Galaxies
- The Expanding Universe
  • Reading Graphs
  • How far away is the Bootes cluster? How fast is
    it moving?
  • About 2.5 billion light-years about 39,000 km/sec

32
Speeding Galaxies
- The Expanding Universe
  • Reading Graphs
  • Which galaxy is moving away the fastest? Which
    galaxy is closest to Earth?
  • Hydra Virgo

33
Speeding Galaxies
- The Expanding Universe
  • Drawing Conclusions
  • How are the distance and speed of a galaxy
    related?
  • The greater the distance from Earth, the greater
    the speed of the galaxy.

34
Speeding Galaxies
- The Expanding Universe
  • Predicting
  • Predict the speed of a galaxy that is 5 billion
    light-years from Earth.
  • Its speed would be about 80,000 km/s.

35
Moving Galaxies
- The Expanding Universe
  • The galaxies in the universe are like the raisins
    in rising bread dough.

36
Formation of the Solar System
- The Expanding Universe
  • The solar system formed from a collapsing
    cloudof gas and dust.

37
Identifying Supporting Evidence
- The Expanding Universe
  • As you read, identify the evidence that supports
    the big bang theory. Write the evidence in a
    graphic organizer like the one below.

Evidence
Moving galaxies Allgalaxies are moving
awayfrom us and from one other.
Theory
Big Bang
Cosmic backgroundradiation This glow comesfrom
thermal energy leftover from the big bang.
38
Links on the Expanding Universe
- The Expanding Universe
  • Click the SciLinks button for links on the
    expanding universe.

39
End of SectionThe Expanding Universe
40
Graphic Organizer

Telescopes
can be
In space only
On Earth
collect types of radiation
collect types of radiation
Visible light
Gamma rays
Radio waves
X-rays
Infrared
Ultraviolet
41
End of SectionGraphic Organizer
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