Yr 13 - Astrophysics & Cosmology (5.5.3 - 5.5.5) Flashcards
Colour of a star depends on.
The luminosity of the star.
A Black Body
Body that absorbs all wavelengths of EM radiation.
- Can emit all wavelengths of EM radiation
Wien’s Displacement law
Peak intensity of radiation is related to surface temperature of star.
Wavelength ∝ 1 / T (inversely proportional)
K = Wien’s Constant (m.K) / Peak wavelength
Spectral Class Types for stars
O - Blue - 25,000/50,000 (K)
B - Blue/White - 12,000/25,000 (K)
A - White - 7,500/12,000 (K)
F - Yellow/White - 6,000/7,500 (K)
G - Yellow - 4,500/6,000 (K)
K - Yellow/Red - 3,000/4,500 (K)
M - Red - 2,000/3,000 (K)
Relationship between Kinetic energy and Temperature
Ke ∝ Temperature
What do hydrogen nuclei fuse to make?
Helium nuclei
Size of low mass star (in terms of solar masses)
0.5 - 10 solar masses
Whats a continuous spectrum? (Atomic Spectrum)
What are they used to show?
Superimposed image of both absorption & emission line spectrum.
- No visible dark lines because the colour lines from Emission spectrum cover the dark Lines on Absorption spectrum.
- Used to show black body radiation.
What is a line spectrum? (Molecular spectrum)
Either Absorption or Emission line spectrum.
Absorption line spectrum
Produced by atoms absorbing energy.
- Dark lines on bright background
- Exited atom
Emission line spectrum
Produced by atoms releasing energy
- Bright lines on dark background
- Relaxing atom
Whats a transmission diffraction grating?
Glass surface with very fine parallel grooves and slits used to produce optical spectra by diffracting transmitted light.
What is maxima and minima?
Maxima - Point where 2 crests of troughs off 2 different waves collide to reinforce one-another.
Minima - Point where crest and trough meet and cancel each other out.
Ionisation
Where an atom acquires a positive/negative charge by gaining/loosing electrons.
Equation including:
- n
- 𝝺
- d
- Sin 𝞡
n 𝝺 = d Sin𝞡
n = Order of maximum
𝝺 = Wavelength of incident light
d = Slit Seperation
Sin𝞡 = angle beam makes with diffraction grating