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Using Telescopes to Observe Electromagnetic Radiation in Space

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Presentation on theme: "Using Telescopes to Observe Electromagnetic Radiation in Space"— Presentation transcript:

1 Using Telescopes to Observe Electromagnetic Radiation in Space
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2 This is a telescope:

3 So is this:

4 And this:

5 Even this:

6 What are Telescopes Telescopes are instruments that collect electromagnetic radiation and bring it into focus.

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8 Collects: Visible Light Wavelengths: 350-800 nm
Optical Telescopes Collects: Visible Light Wavelengths: nm Where Located: on Earth and in space

9 What we look at: Stars, Planets, nebula, galaxies
Optical Telescopes What we look at: Stars, Planets, nebula, galaxies What information is provided: Distances using light years, Composition of stars

10 Optical Telescope Images

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12 Best of Hubble

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14 Collects: Radio waves and Microwaves Wavelengths: 1,000 km- 1m
Radio Telescopes Collects: Radio waves and Microwaves Wavelengths: 1,000 km- 1m Where Located: on Earth

15 What we look at: any space in the sky
Radio Telescopes What we look at: any space in the sky What information is provided: discovered Pulsars and cosmic background radiation

16 Radio telescope images

17 This is an array of telescopes.

18 Radio telescope data:

19 Spitzer Space telescope
Collects: Infrared Wavelengths: 3.6 to 160 micrometers Where Located: Space

20 Spitzer Space Telescope
What we look at: Stars, galaxies What information is provided: discovered extrasolar planets, youngest star ever found

21 Spitzer Images Andromeda Galaxy

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23 Collects: X-rays Wavelengths: 0.01-10 nm Where Located: Space
Chandra Observatory Collects: X-rays Wavelengths: nm Where Located: Space

24 Chandra Observatory What we look at: exploded stars, clusters of galaxies, and matter around black holes. What information is provided: x-rays emitted from hot gasses leaving black holes has been recorded

25 Chandra Images

26 Cygnus X-1, first strong black hole discovered.

27 SNR 0519-69.0 - remains of an exploding star in the Large Magellanic Cloud.

28 Compton and Fermi Gamma-Ray Observatories
Collects: Gamma-rays Wavelengths: 20 keV to 30 GeV Where Located: Space

29 Compton and Fermi Gamma-Ray Observatories
What we look at: deep space, Gamma bursts What information is provided: exploding stars that become black holes as their cores collapse.

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33 Video review


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