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Telescopes & Light. The Powers of a Telescope. Light Gathering Power : Astronomers prefer *large* telescopes. A large telescope can intercept and focus more starlight than does a small telescope. A larger telescope will produce brighter images and will be able to detect fainter objects. .

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Presentation Transcript
the powers of a telescope
The Powers of a Telescope

Light Gathering Power: Astronomers prefer *large* telescopes. A large telescope can intercept and focus more starlight than does a small telescope. A larger telescope will produce brighter images and will be able to detect fainter objects.

Resolving Power: A large telescope also increases the sharpness of the image and the extent to which fine details can be distinguished.

Magnification: The magnifying power is the ability of the telescope to make the image appear large in the field of view.

size does matter
Size Does Matter

Light-Gathering Power:

Depends on the surface area (A) of the primary lens and is proportional to the telescopes diameter.

D

the powers of a telescope1
The Powers of a Telescope

Resolving Power: Wave nature of light: The telescope aperture produces fringe rings that set a limit to the resolution of the telescope.

the powers of a telescope2
The Powers of a Telescope

Magnifying Power

The ability of the telescope to make the object’s optical image appear bigger while being observed

A larger magnification does not improve the resolving power of the telescope!

types of telescopes
Types of Telescopes
  • Refracting Telescopes: Use lenses as the optics to focus and bend light.
    • Galileo used a refracting telescope.
    • The human-eye is partly a refracting telescope.
refracting telescope

Objective Lens

Eyepiece Lens

Focal Length Objective

Focal Length of Eyepiece

Refracting Telescope

Refracting Telescope:Lens focuses light onto the focal plane

Focal length

disadvantages

Blue Focus

Red Focus

Disadvantages

Refracting telescopes suffer from Chromatic Aberration. As light passes through a lens, just as a prism will disperse light, the lens will focus bluer wavelengths differently than the redder wavelengths.

disadvantages1
Disadvantages
  • Cannot be made very large for a multitude of reasons.
  • Get to be very expensive to maintain.
  • Lenses can grow “cloudy” over time.
  • Lenses can distort over time.
types of telescopes1
Types of Telescopes
  • Reflecting Telescopes: Use mirrors as the optics to focus and bounce light.
    • The rear view mirror on your car is a simple reflecting telescope.

Reflecting Telescope: Concave Mirror focuses light onto the focal plane

Focal length

Most modern telescopes are reflecting telescopes.

advantages
Advantages

Reflecting telescopes do not suffer from Chromatic Aberration. All wavelengths will reflect off the mirror in the same way.

Reflecting telescopes can be made very large because the mirrored surfaces have plenty of support. Thus, reflecting telescopes can greatly increase in light gathering and resolving power.

Reflecting telescopes are often cheaper ($$$) to make than similarly sized refracting telescopes.

hey where are you going
Hey! Where are you going?

The Doppler Effect

The wavelength of light is effected by the relative motion between the source and the observer. Christian Doppler (1803-1853), a professor of mathematics in Prague, pointed out in 1842 that the observed wavelength of light is affected by motion.

The frequency increases when the source and observer are approaching each other, and decreases when they are moving away from each other.

the doppler effect

Observer

Stationary

Towards

The Doppler Effect

Blueshift

Away

Redshift

slide17

Observer

Observer

how does this help
How does this help?

Star moving towards from us

Stationary Star

Star moving away from us

Strength of the Light with this Wavelength

Wavelength

where to put a telescope
Where to put a Telescope?

Far away from civilization – to avoid light pollution

slide21

Where to put a Telescope?

On high mountain-tops – to avoid atmospheric turbulence and other weather effects

seeing
“Seeing”

Weather conditions and turbulence in the atmosphere set further limits to the quality of astronomical images.

Bad seeing

Good seeing

x ray astronomy
X-Ray Astronomy

X-rays are completely absorbed in the atmosphere.

X-ray astronomy has to be done from satellites.

NASA’s Chandra X-ray Observatory

gamma ray astronomy
Gamma-Ray Astronomy

Gamma-rays: most energetic electromagnetic radiation; traces the most violent processes in the Universe

The Compton Gamma-Ray Observatory

radio interferometry1
Radio Interferometry

The Very Large Array (VLA): 27 dishes are combined to simulate a large dish of 36 km in diameter.

Even larger arrays consist of dishes spread out over the entire U.S. (VLBA = Very Long Baseline Array) or even the whole Earth (VLBI = Very Long Baseline Interferometry)!

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