Yr 13 - Astrophysics & Cosmology (Cosmology) Flashcards
What is the unit for angles in astronomy? And how many In 1 degrees?
Arc seconds
- 3600 Arc seconds in 1degree
- 60 Arc minutes in 1 degree
Parsec
Distance from SOL to astronomical object which has angle of 1 arc second between SOL and Earth (Parallax angle)
Tan(P) = 1/d
What can we assume and use?
What are the limitations for the small angle approximation?
Small angle approximation
P = 1/d
P (Parallax angle)
1 = Astronomical unit
d (distance in Parsecs)
Limitations - Distance Must be < 100 Parsecs
What is Stella parallax
- And what happens to stars that are close?
Difference due to change in position of earth
- Close stars change apparent position as earth orbits whereas further (background) stars don’t.
Parallax angle
Angle of apparent shift when a close star is observed from 2 different positions against background stars.
What is the cosmological principle?
Universe is Isotropic & Homogenous & laws of physics apply everywhere (on a large scale)
What are absorption Klines?
Lines missing on absorption spectra due to certain elements in stars atmosphere absorbing certain wavelengths of em radiation.
Label each end of the colour spectra in terms of wavelength length and frequency
R - Long λ - Low F
O
Y
G
B
I
V - Short λ - High F
Explain the doppler effect in terms of wavelengths
Object is moving forward you - Shorter wavelengths - Higher frequency
Object moving away from you - Longer wavelengths - lower frequency
What is red shift?
When the wavelength is shifted towards the red section of the spectrum
- Longer wavelengths
- Occurs when object moving away (recessional velocity)
What is Blue Shift?
When the wavelength is shifted towards the blue section of the spectrum
- Shorter wavelengths
- Occurs when the object is moving towards
The equation that is given is
△λ/λ = △f/f = v/c
What is the other equation using the observed wavelength and true wavelength
△λ = λobs - λ
△f = fobs - f
λ/fobs = λ/f when there is relative motion (Observed wavelength) From earth!
λ/f = λ/f with no relative motion (Source wavelength) As perceived from source!
λ/f is λ or f not λ divide f
Using the equation △λ = λobs - λ
- When is the object moving away?
- When is the object moving toward?
- When (+) observer and source moving apart
- When (-) observer and source moving together
What is meant by ‘doppler shifted wavelength’ or ‘doppler shifter frequency’?
△λ or △f