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Midterm Distribution31 A’s, 37 B’s, 26 C’s, 21 D’s, 17 F’s
Common Mistakes
Do the algebra first! Units, Units, Units Does your answer make sense? Using ratios
Lecture 18:
Telescopes and
Observational Astronomy
There are two kinds of telescopes
RefractingRefracting: a lens is used to focus the light from distant objects.
ReflectingReflecting: a primary mirror is used to gather and focus light.
A Refracting Telescope
A Reflecting Telescope
Alternative designs for reflecting telescopes
Charge Coupled Devices (CCD)
Fundamental Telescope Properties
Light collecting area (diameter of primary mirror or lens)
angular resolution (smallest angular distance that can be resolved clearly) limited by effects of Earth’s atmosphere
Angular Separation
= 360o . s /(2d) “small angle formula”
Angular Resolution
Diffraction
The Diffraction Limitdiffraction limit = 2.5 x 105 x wavelength of light(arcsec) diameter of telescope
Find the diffraction limit of the 2.4 m Hubble Space Telescope for visible light (500 nm).
d.l. = 2.5 x 105 (500 x 10-9 m/2.4 m) = 0.05 arcsec
Where to put your telescope high and dry – to minimize the blurring
effects of the Earth’s atmosphere and emission/absorption from water vapor
away from light pollution with roads, electricity, and other support
systems nearby
The Summit of Mauna Kea
The Keck Telescopes
The Magellan Telescopes
Basic Functions of Telescopes
Imaging/photometryaccurate measurement of light intensity filters can be used to separate into different
colors spectroscopy
light spread out using a diffraction grating time sequence
how an object’s brightness changes with time
A Basic Spectrograph
Spectral Resolution
Telescopes across the spectrum
Hubble Space Telescope
Infra-red Telescopes
SOFIA
SIRTF
Radio Telescopes
Arecibo
Very Large Array (VLA)
Interferometry An array of smaller
telescopes can be used together
the light gathering power is equal to the sum of all the areas
the angular resolution is greatly improved
X-ray Telescopes
grazing incidence mirror
Chandra X-ray Observatory
Compton Gamma-ray Observatory
Images of non-visible light
Radio
CO
FIR
NIR
vis.
X-ray
gammaray