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TELESCOPES. Where do we put telescopes to have the best viewing conditions? 1. On Earth: CLEARHIGHDRYCOLDDARK.

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Presentation on theme: "TELESCOPES. Where do we put telescopes to have the best viewing conditions? 1. On Earth: CLEARHIGHDRYCOLDDARK."— Presentation transcript:

1 TELESCOPES

2 Where do we put telescopes to have the best viewing conditions? 1. On Earth: CLEARHIGHDRYCOLDDARK

3 Problem with Telescopes on Earth? Problem: Particles of all sorts in the atmosphere block and cloud the view Particles of all sorts in the atmosphere block and cloud the view

4 2. In Space Solves atmosphere problem – CLEAR VIEW! Examples: Hubble, Cobe, Iras

5 Problem with telescopes in space? They’re in space! Hard to get to Hard to repair EXPENSIVE!!!

6 Functions of a Telescope 1. C ollect Light 2. M agnify Images 3. S eparate Distant Objects 4. U se as a Camera

7 OPTICAL TELESCOPES (USE VISIBLE LIGHT) Two types: 1. Refractor – BENDS LIGHT Invented by Hans Lippershey in 1608 Refined by Galileo in 1609

8 Galileo demonstrating his telescope

9 2. Reflector – USES MIRRORS

10 Tololo Observatory - Chile

11 TYPE 1 – REFRACTING TELESCOPE How does it work? a. It bends light to create an image b. It uses two lenses 1. eyepiece (ocular) lens - small 2. objective lens - large

12 Draw it!

13 Type 2 – Reflecting Telescope a. Invented by Isaac Newton in 1668 b. Uses two mirrors Objective Mirror – Large Secondary (flat) mirror – Small Secondary (flat) mirror – Small c. Can be VERY LARGE 40 ft - 50 ft diameter objective mirror!

14 Draw It!

15 Advantages of a reflector 1. You only need to prepare one side of the mirror. (on a refractor the lens has two sides) – cheaper and distortion is less of a problem. 2. The whole back of the mirror can be supported, therefore can be made very LARGE

16

17 Non-optical Telescopes 1. Radio Telescopes a. Location – Earth (atmosphere does not affect radio waves) b. Structure – Large metal dish

18 c. Size – very large because radio waves have a very long wavelength

19 d. Arrays – sets of multiple radio telescopes that allow for more data to be gathered.

20 Ex – VLA (very large array) in Socorro, New Mexico 27 dishes. SETI– Search for Extra-Terrestrial Intelligence looking for intelligent radio signals looking for intelligent radio signals

21 Other Non-Optical Telescopes (all are satellites) a. Infrared – IRAS launched 1983

22

23 b. Microwaves – COBE Cosmic Background explorer. Discovered evidence of the Big Bang. Launched 1981

24 COBE Image of CBR

25 c. X-Rays – Chandra Launched 1999

26 Cassiopeia Super Nova

27 Black Hole

28 Crab Nebula

29 Saturn

30 d. Gamma Rays – GRO Gamma Ray Observatory

31 Milky Way


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