Astrophysics Flashcards
(49 cards)
What are disadvantages of refracting telescopes?
Chromatic and spherical aberration.
Distortion due to warping of glass.
Expensive.
What is chromatic aberration?
Different wavelengths focus at different points causing blurred image.
What is spherical aberration?
Spherical lens means rays focus at different points.
Closer to centre of lens = focuses further away.
Which colour of light focuses furthest from lens due to chromatic aberration?
Red.
What is resolving power / Rayleigh criterion?
Minimum angle at which two objects are able to be differentiated between.
Central maximum of one sits over the first minimum of the other.
What is quantum efficiency?
Number of photons detected / Number of photons incident x 100
What is a CCD and how does it work?
Silicon chip divided into pixels.
Incident light liberates electrons which are trapped in potential wells.
Number of electrons liberated is proportional to intensity of light.
Pattern built up by electrons forms image.
What is the quantum efficiency of a CCD?
Around 70%
What is the gathering power?
Energy / photons collected per second.
What is brightness of a telescope proportional to?
d^2
What is luminosity
Total energy emitted per second (power).
What number is used to compare the brightness of stars?
2.512
What is a parsec?
Distance an object must be to have a parallax of one arcsecond when observed from Earth.
What is a light year?
Distance an EM wave travels in a year.
What is apparent magnitude?
Magnitude of a star as seen from Earth.
What is spacial resolution?
How far apart objects need to be to be distinguishable.
What is a blackbody?
Absorbs and can emit all wavelengths of EM radiation.
What is the area under a black body curve?
Intensity.
Which telescopes cannot be grounded on Earth?
Infrared
UV
X-Ray
Gamma
What do lines on absorption spectrum refer to?
Photons absorbed by gases.
What do lines on an emission spectrum refer to?
Photons emitted from energy levels.
Where do electrons with a high temp reside in for Balmer series?
n=2 level, so strong lines.
Where do electrons with a low temp reside in for Balmer series?
n=1 level, so weak lines.
Where do electrons with a very high temp reside in for Balmer series?
n=3 level, so less strong lines.