Telescopes Flashcards
The amount of light a telescope can gather determines the —- of the image it can form and the —- of objects it can detect
Brightness, dimness
Light gathering power determined by
A=pir^2
Use Lena’s to focus light
Refracting telescope
Use mirrors to focus the light
Reflecting telescope
Cheaper, lighter, and do not have an aberration of lenses, used more often
Reflectors
Direct focus
Prime
All over focus
Newtonian
Bouncing focus
Cassegrian
The bending of light around obstacles
Diffraction
1/60 of an acrminute
Arc second
Simultaneous observations are made from widely space, telescopes, and sent to a common detector where they are analyzed by computer to form an image
Interferometer
Detects, approximately 4% of photons recorded
Photographic film
Semi conductor surface that is broken down into millions of picture elements
Charges coupled devices
Picture elements
Pixels
How many protons recorded
75%
Astronomical objects, ready, energy at 
All wavelengths 
Stingless absorbed by atmosphere
In in frayed ultraviolet, x-rays and gamma radiation 
From ground-based light sources interferes with astronomical observations
Light pollution 
The twinkling of astronomical objects due to refraction of light through the atmosphere 
Scintillation
Telescopes in orbit
Hubble and James webb