The Milky Way and Other Galaxies Flashcards

1
Q

What are the main properties of the milky way?

A

Mainly a disc with spiral arms. Also with a bulge and halo.

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2
Q

About how many stars are in the milky way?

A

~3*10^11 stars

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3
Q

Name some properties of the milky way.

A
  • Perseus arm at far left
  • Orion arm at top
  • Sun near orion arm
  • ~8500pc across
  • ~500pc deep
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4
Q

What is the distribution of globular clusters like in the milky way?

A

Roughly spherical. Not centred at Sun though.

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5
Q

What radius does the sun orbit the centre of the galaxy? What velocity?

A
R0 = 8.5kpc
v0 = 220 km s^-1
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6
Q

How do you work out an equation for the mass of a star?

A

Set gravitational force equal to centripetal acceleration and rearrange for mass.

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7
Q

What does a galaxy rotation curve show us?

A

That stellar count rapidly drops as a function of distance to the centre.

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8
Q

What is the Milky way rotation curve like and what does this suggest?

A

Is flat - suggests there is something else other than stars mass, otherwise it would decrease with radius.

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9
Q

What is dark matter?

A

Unknown mass surrounding galaxies which is seen through gravity but does not appear to emit light.

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10
Q

How do we know there are black holes at the centre of galaxies?

A

Because from the equation for mass, we can see that the central mass is way to large to be a cluster of stars.

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11
Q

How can we estimate how far other galaxies are?

A

Need something bright which we can estimate the absolute magnitude of and then use the magnitude equation to find out distance.

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12
Q

What are Cepheid variables?

A
  • Cepheids undergo oscillations in their envelopes - they are in the giant star phase
  • Their oscillations are visible as changes of brightness with periods of ~10 days
  • Was discovered that the pulsation period is related to the luminosity of the star
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13
Q

What is the equation relating luminosity and period?

A

Mv = -2.81*log P(d) - 1.43

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14
Q

What are the requirements for standard candles?

A
  • Bright
  • Recognisable
  • Can be calibrated (need a luminosity)
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15
Q

What absolute magnitude do we find for Cepheids of approximate periods of 10-100days?

A

Mv ~ -2 to -7 or L = 500-50000 L(sun)

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16
Q

What is the distance to the Andromeda galaxy?

A

770 pc

17
Q

What is the net velocity of the Milky way and where is it heading?

A

110 km s^-1 and is heading for the Andromeda galaxy

18
Q

How long will it take for the milky way to reach andromeda?

A

4 billion years

19
Q

What is the equation for fractional redshift?

A

z = (λ’-λ0)/λ0 = v/c

20
Q

What did Vesto Slipher find about near/far galaxies?

A

The near galaxies are getting close but the far galaxies are moving away from us and eachother

21
Q

What is Hubble’s law of universal expansion?

A

Galaxies recede from us with a velocity v that is proportional to the distance d: v = H0d, where H0 is the Hubble constant

22
Q

What is the modern value of the Hubble constant?

A

68-72 km s^-1 Mpc^-1

23
Q

What are the two main types of supernovae?

A

Type 2 - core collapse

Type 1a - white dwarfs pushed over the Chandrasekhar limit

24
Q

What does the light curve for a type 1a supernova look like?

A

Increases and then peaks and then decreases, levelling out at the end

25
Q

How can we use type 1a supernova?

A

Can use them to find distance as they are very bright and can be calibrated to give luminosity (Mv ~ -19)