ASTROPHYSICS Flashcards
(41 cards)
Apparent Magnitude
brightness of an object as seen from earth
Absolute magnitude
Brightness seen from 10pc (parsec)
light year
distance traveled by light in one year
parsec
distance to an object subtending 1 second of arc to earths orbit
State meaning of T in Stefan-Boltzmann law
Kelvin temperature of surface
Unit of luminosity
watts
convex/ converging lens
focuses incident light
concave/ diverging lens
spreads out light
focal length
distance between centre of a lens and principle focus
the shorter the focal length the stronger the lens
real image
formed when light rays cross before refraction
virtual image
formed on same side as lens, light rays do not cross
lens formula
1/u + 1/v = 1/f
u - distance of object to centre of lens
v - distance of image to centre of lens
f - focal length
power of a lens
shorter focal length, more powerful the lens
measured in D (dioptres)
converging (positive)
diverging (negative)
P = 1/u + 1/v = 1/f
normal adjustment
sum of focal lengths of objective and eyepiece lens
Quantum efficiency equation
(#electrons released) divided by
(#incident photons)
Quantum efficiency of human eye
1%
CCD advantages
store more images
better resolution
wider range of wavelengths detected
What is the minimum resolving angle of the human eye
3.2 x 10^-4 rad or 0.02 degrees
For us to just be able to distinguish between two diffraction patterns…
The central maxima of one pattern has to coincide with the other patterns first minimum
Astronomical unit
1 AU is the mean distance between the Earth and the Sun.
number of brightest star in hipparcos scale
1
number of dimmest star in hippacros scale
6
apparent magnitude scale based on…
intensity
A stars total power output known as its…
luminosity