24
Unit 3 Telescopes

Unit 3

  • Upload
    rowena

  • View
    29

  • Download
    0

Embed Size (px)

DESCRIPTION

Unit 3. Telescopes. Optical Telescopes. Two basic types Refractors Reflectors. Refractors. Uses lenses to gather and concentrate light. Refractors. Advantages: Refractor telescopes are rugged Lenses inside the tube is sealed so it rarely needs cleaning images are steadier and sharper - PowerPoint PPT Presentation

Citation preview

Page 1: Unit 3

Unit 3

Telescopes

Page 2: Unit 3

Optical Telescopes

• Two basic types– Refractors– Reflectors

Page 3: Unit 3

Refractors

• Uses lenses to gather and concentrate light

Page 4: Unit 3

Refractors• Advantages:– Refractor telescopes are rugged– Lenses inside the tube is sealed so it rarely needs

cleaning– images are steadier and sharper

• Disadvantages:– chromatic aberration – Lens supported only at the ends, lens will sag – Expensive, heavy

Page 5: Unit 3

Refractor

Page 6: Unit 3

Reflectors

• Uses a curved mirror to focus incoming light

Page 7: Unit 3

Reflectors• Advantages:– Do not suffer from chromatic aberration – Can be made very BIG!– Less expensive, lighter

• Disadvantages:– Optics need more frequent alignment– Open to the outside, need frequent cleaning– Secondary mirror can produce diffraction effects

Page 8: Unit 3

Reflector

Page 9: Unit 3

Types of Reflectors• Gregorian

• Newtonian

• Cassegrain

Page 10: Unit 3

Schmidt-Cassegrain

Page 11: Unit 3

Telescope magnificationMagnification = focal length of telescope / focal length eyepiece

e.g. focal length of telescope = 1000 mm focal length of eyepiece = 30 mm

magnification = 1000 mm/ 30 mm

= 33

Page 12: Unit 3

Brightness• The observed brightness of an object is

directly proportional to the area of the telescope mirror, e.g. a 5 meter telescope will have a light gathering capacity 25 times (52) greater than a 1 meter telescope

Page 13: Unit 3

History of Large Telescopes

• William Herschel (late 1700s)

Page 14: Unit 3

• Mt. Wilson (1917)– 100 inch

Page 15: Unit 3

• Hale (1948)– 200 inch

Page 16: Unit 3

Space Telescopes

• outside the distortion of Earth's atmosphere• extremely sharp images • almost no background light

Page 17: Unit 3

Space Telescopes

• Hubble

• Spitzer

• Chandra

Page 18: Unit 3

Kepler Space Telescope

• Designed to discover Earth-like planets

Page 19: Unit 3

Herschel Space Observatory

•Launched in 2009 by the European Space Agency•Sensitive to Infrared radiation

Page 20: Unit 3

Image Acquisition & Processing

• Charge-coupled devices (CCDs) computer (very efficient)

Page 21: Unit 3

Radio Astronomy

Page 22: Unit 3

How to pick a telescope

• Start by using your bare eyes • Next, move up to binoculars• When you’re ready for a telescope, read/

research

Page 23: Unit 3

Choosing the right telescope

• Performance• Purpose• Portability• Light Pollution• Price

Page 24: Unit 3

• All other things being equal, the greater the mirror/ lens diameter the greater the light gathering ability

• Primary Mirror Size Square Inches of Aperture

4" 12 6 28 8 50 10 78 12 113

• http://www.astronomics.com/main/category.asp/catalog_name/Astronomics/category_name/How%20to%20pick%20a%20telescope/Page/1