Astro-Physics Flashcards
Give two equations for magnification of a refracting telescope.
1) M = α / β
2) M = Fo / Fe (Focal Objective / Focal Eyepiece)
Define 1 arc minute.
1/60 of a degree
What is 1 degree in arc minutes
60 arc minutes
What’s the equation for angular size of an object
Diameter of object / Distance to eye or lense
List two “aberrations” of refracting telescopes
1) Chromatic Aberration
2) Spherical Aberration
What is meant by Chromatic Aberration
The refractive index of a lens is different for different wavelengths so different colours are brought to focus at different points. SHORTER WAVELENGTH => SMALLER FOCAL LENGTH
What is meant by Spherical Aberration
Due to manufacturing difficulties, imperfections in a lens cause rays further from the principle axis to be brought to focus closer to the lens.
What criteria must be met for a a refracting telescope to be in “normal adjustment”
- Objective and eyepiece lenses share a principle focus (separation = Fo + Fe)
- Must be focused at infinity (meaning everything in frame is in focus)
What is meant by the term Collecting power of a telescope
How much light enters the telescope hence determining the brightness of the observed image
What is the relationship between collecting power and telescope aperture
Collecting power is directly proportional to (Diameter of Aperture)^2
What is meant by the term Resolving Power of a telescope
How well the telescope can distinguish between two nearby objects
What is an airy disc
It’s a circular diffraction patter around stars caused by diffraction at the telescopes aperture.
What is the Rayleigh Criterion
The minimum angular separation for two object to be resolved
When will the minimum angular separation for the Rayleigh Criterion occour
When the central maximum of one airy disc coincides with the first minimum of the second airy disc.
List 4 disadvantages of refracting telescopes
- Very difficult to create large lenses
- Large lenses can deform under their own weight
- Very difficult to manoeuvre quickly
- Suffer from chromatic and spherical aberration
List 4 advantages of reflecting telescopes
- Can be made of smaller composite mirrors
- Large single mirrors can be made fairly easily
- No chromatic or spherical aberration when using parabolic mirrors
- Light weight allows quick response to astronomical events