Yr 13 - Astrophysics & Cosmology (5.5.3 - 5.5.5) Flashcards

1
Q

Colour of a star depends on.

A

The luminosity of the star.

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2
Q

A Black Body

A

Body that absorbs all wavelengths of EM radiation.
- Can emit all wavelengths of EM radiation

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3
Q

Wien’s Displacement law

A

Peak intensity of radiation is related to surface temperature of star.

Wavelength ∝ 1 / T (inversely proportional)

K = Wien’s Constant (m.K) / Peak wavelength

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4
Q

Spectral Class Types for stars

A

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)

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5
Q

Relationship between Kinetic energy and Temperature

A

Ke ∝ Temperature

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6
Q

What do hydrogen nuclei fuse to make?

A

Helium nuclei

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7
Q

Size of low mass star (in terms of solar masses)

A

0.5 - 10 solar masses

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8
Q

Whats a continuous spectrum? (Atomic Spectrum)

What are they used to show?

A

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.
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9
Q

What is a line spectrum? (Molecular spectrum)

A

Either Absorption or Emission line spectrum.

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10
Q

Absorption line spectrum

A

Produced by atoms absorbing energy.

  • Dark lines on bright background
  • Exited atom
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11
Q

Emission line spectrum

A

Produced by atoms releasing energy

  • Bright lines on dark background
  • Relaxing atom
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12
Q

Whats a transmission diffraction grating?

A

Glass surface with very fine parallel grooves and slits used to produce optical spectra by diffracting transmitted light.

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13
Q

What is maxima and minima?

A

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.

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14
Q

Ionisation

A

Where an atom acquires a positive/negative charge by gaining/loosing electrons.

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15
Q

Equation including:

  • n
  • 𝝺
  • d
  • Sin 𝞡
A

n 𝝺 = d Sin𝞡

n = Order of maximum
𝝺 = Wavelength of incident light
d = Slit Seperation
Sin𝞡 = angle beam makes with diffraction grating

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16
Q

Wien’s displacement law

A

Maximum wavelength is inversely proportional to temperature (Kelvin)

17
Q

Stefans Law

A

Relates luminosity of a star with its absolute temperature.
Known as Stefans constant.

18
Q

One solar mass

A

1.99 x 10^30 kg

19
Q

Low mass star

A

0.5 - 10 solar masses

20
Q

How to elements heavier than iron get created?

A

Supernova Explosions due to high amounts of energy being released.

21
Q

What range of masses can a core be for it to become a neutron star?

A

Between Chandrasekhar limit and 3 solar masses

22
Q

What range of masses can a core be for it to become a black hole?

A

Greater than 3 solar masses