Astrophysics Flashcards
Principal focus
Where rays meet
Focal length
Distance between lens axis and principal focus
Power equation
Power = 1/ focal length
Real image
Image that can be projected
Magnification
How many time’s it has been enlarged
Problems with refracting telescopes
Spherical aberration: not all rays focus at the same point
Chromatic aberration: different frequencies refract by different amounts
Angular resolution
Smallest angle the telescope is able to detect and analyse
Rayleigh criterion
To be able to resolve 2 stars they need to be separated by more than the radius of the airy disk
Quantum efficiency
N.o. Of electrons detected/ n.o. Detected
Collecting power
How much light it can gather
Pid^2/4
AU
The mean distance between the earth and sun
Light year
Distance that light can travel in a year
Parsec
The distance to a nearby star when the angle subtended is 1 arcsecond
Apparent magnitude
How bright the star appears to be from Earth
Absolute magnitude
The brightness of a star from 10pc
Black body
Absorbs the same energy it emits
Plasma
Ionised gas