Panic Flashcards
CCD
Charge coupled devices
Silicone chips divided into a grid of millions of identical pixels
That can capture images digitally
How DO CCDs work
Photons hit silicon in pixel
Creates free electrons confined to the pixel
Causes charge to accumulate
Which can be measured to create digital signal
Describes where light hits an the intensity
Charge varies depending on how many photons hit
CCD vs eye
C: quantum efficiency of 80%
E: 1%
C: detect wider spectrum of light (UV and infrared) than E which can only detect visible
C: less convenient, more equipment needed than just looking down telescope
C: creates digital images which can be stored, copied and shared
What can limit resolution
Diffraction
Diffraction pattern forms with airy disc at centre and maxima and minima around
Air bubbles or impurities in glass
Absorb and scatter some light so faint objects seen
Difficult to build them large
Issue with focal length of refracting telescope
Mustbe large to get large magnification
So need large expensive buildings
Benefit of reflecting mirrors
No chromatic aberration
Supported from underneath so distort less than lenses
Casssegrain arrangement
Uses convex secondary mirror so the user doesn’t block incoming light
Radio telescope benefit
Making a dish out of wire mesh makes construction easier and cheaper
Longer wavelength of radiation being detected so less affected by imperfections in shape of dish so dish doesn’t have to be as perfect to avoid spherical aberration
Collecting power
Proportional to diameter squared
Parallax
Apparent change in motion
Distance of a nearby star
d=r/tantheta
For small angles, tan theta is approximately theta
0.77 arc seconds
0.77×1/3600
Parallax
Half the angle by which a nearby star appears to move in relation to the background stars in 6 months as earth moves from one end of its orbit to the other
What objects emit EM radiation
Any above absolute zero