1.1 Recap on Stars Flashcards

1
Q

Define a galaxy

A

A group of stars bounded by gravity

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2
Q

What are the two observational characteristics of stars?

A

Brightness and colours as measured by us

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3
Q

What are the two physical characteristics of stars?

A

Luminosity (J/s)
Flux (W/m^2)
Can also get flux densities

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4
Q

What is important about the apparent magnitude equation?

A

m = - 2.5 logF constant

  • Logarithmic so matches our vision
  • Negative scale (brighter stars have a lower magnitude)
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5
Q

What is colour?

A

The difference between two magnitudes measured in 2 regions of the spectrum
c = -2.5log(F1 / F2)

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6
Q

What is absolute magnitude?

A

Magnitude of source if placed at 10pc

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7
Q

What is the distance modulus?

A

The apparent magnitude - the absolute magnitude

DM = 5log(d/10pc)

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8
Q

Is the spectrum of a star a black body?

A

No

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9
Q

How do we deal with spectra that aren’t radiating as a BB?

A

Aproximate it as a BB then modify it by accounting for absorption/emission by molecules and atoms in the atmosphere

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10
Q

What is Wein’s law a relation between, and state the equation

A

Relationship between the wavelength at which a black body peaks and its temperature
Hotter the star, the bluer the spectrum
λ = 2900 / T

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11
Q

State the properties of a HR diagram

A

Axes are Luminosity and surface temp(right to left)
Most stars align on main sequence
Different diagram regions equal different stages of star lifetime

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12
Q

When are stars a main sequence star?

A

During Hydrogen burning

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13
Q

What is the relationship between luminosity and mass?

A

L is prop. to M^3.5

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14
Q

What is the equation for the lifetime of a star, and what is significant about this?

A

τ = Fuel available / Rate of consumption = M / M^3.5 = M^-2.5
- More massive stars have shorter lifetimes

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15
Q

What does the colour of a galaxy depend on?

A

The balance between the old, red, faint stars and the young, blue, luminous stars

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16
Q

What is the initial mass function, and what does it describe?

A

n(M) prop. to M^-2.35

- Shows smaller stars are more likely to form