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Astronomical Instruments

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Title: Chapter 1 Author: Robert Harr Last modified by: Robert Harr Created Date: 9/8/2003 10:52:05 PM Document presentation format: On-screen Show Company – PowerPoint PPT presentation

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Title: Astronomical Instruments


1
Chapter 5
  • Astronomical Instruments

How do we learn about objects too far away for
spacecraft? How do telescopes work? Do all
telescopes use light? Why are telescopes located
on mountains? Why are some telescopes in orbit
around the Earth?
2
5.1 Telescopes
  • Telescopes are devices for seeing distant
    objects.
  • To see faint objects, collect more light by using
    a bigger aperture.
  • Magnification is much, much less important.
  • Two types of optical telescopes
  • Refracting
  • Reflecting

3
Refracting Telescopes
  • Use a large lens as the primary light collecting
    element.
  • Common in older telescopes.
  • Chromatic aberrations and ultraviolet cutoff.

4
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5
Reflecting Telescopes
  • Use a large mirror as the primary light
    collecting element.
  • Easier to make a large mirror than a large lens.
  • Modern telescopes are reflectors.
  • Reduced chromaticity problems.

6
Refracting versus Reflecting
7
Prime, Newton, and Cassegrain
8
5.2 Optical Detectors and Instruments
  • Second greatest advance in astronomy was the use
    of photographic film
  • Longer integration time than the eye.
  • Images available for later (re)inspection.
  • The 3 uses of telescopes
  • Imaging
  • Measuring brightness and color
  • Spectroscopy
  • All benefit from longer integration time.

9
Charge-Coupled Device
  • A modern advance is the use of charge-coupled
    devices or CCDs.
  • These are the digital film of digital cameras.

10
5.3 Optical and Infrared Observatories
  • Ground based telescopes are housed in domes or
    other structures to protect them when not in use.
  • They are often located on remote mountains, away
    from lights, and smog, and above humid and
    turbulent air.

11
NOAO on Kitt Peak, AZ
12
South African Large Telescope
13
European Southern Observatory
14
Choice of Telescope Sites
  • Weather clouds, wind, and rain limit observing
    time.
  • Water vapor water vapor in the atmosphere
    filters out infrared wavelengths.
  • Darkness city light can overwhelm faint stars.
  • Turbulence turbulent air blurs images.

15
Observatory Sites
  • Newest telescopes are sited in the Chilean Andes,
    desert peaks of Arizona, Canary Islands, and
    Mauna Kea in Hawaii.
  • Modern telescopes can use segmented mirrors,
    adaptive optics, and interferometry.

16
Observing Other Radiation
  • To learn the most about planets, stars, and
    galaxies, astronomers use as many types of
    radiations as possible.
  • Radio
  • Infrared and ultraviolet
  • X-rays
  • Gamma rays

17
5.4 Radio Telescopes
  • Many objects emit radio waves, from long wave to
    microwaves.
  • Radio telescopes generally look like large
    satellite dishes.
  • They can operate during the day and night.
  • Large facilities in Puerto Rico, West Virginia,
    and New Mexico.

18
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19
The Very Large Array (VLA)
20
The VLBA Spans A Continent
21
Radio Image of Quasar Jets
22
5.5 Observatories Outside the Earths Atmosphere
  • Some wavelengths of radiation are absorbed by
    Earths atmosphere (gamma rays, x-rays, and
    ultraviolet).
  • Telescopes for these wavelengths must be put in
    space.
  • The Hubble telescope demonstrates the advantages
    for an optical telescope to be above the
    atmosphere.

23
The Hubble Space Telescope
24
The Swift Satellite (GRBs)
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