astrophisc Flashcards

1
Q

Hubble’s law

A

recession speed of galaxies is proportional to their distance from earth

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

constellation

A
  • a group of stars that form a pattern in the sky
  • but they are not necessarily close to each other
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

stellar cluster

A

a group of stars (gas and dust) that are held together by gravity

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

apparent brightness

A

the power per square metre received by an observer on earth

is the amount of ENERGY received per second per unit area by an observer”

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

two different ways in which atomic spectra can be used to deduce physical data for stars

A
  • absorption spectra give information on the element that make up the star
  • the peak of wavelength gives information on the temperature of the star
    doppler shift gives information on the stars motion relative to earth
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

parallax angle measured

A
  • relative position of the star to distant background stars is received at two times 6 months apart
  • half of the angular shift = parallax angle
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

parallax angle less than 100 pc

A

beyond this distance the parallax angle is too small to be measured accurately/is less than the uncertainty of the measurement

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

property determine wether a star ends its life as a white dwarf or as a neutron star

A

mass of the star’s remnant core

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Chandrasekhar limit - difference between a white dwarf and neutron star

A
  • defines the maximum mass of a white dwarf
  • up to this limit electron degeneracy pressure prevents further gravitational collapse
  • above this, gravity overcomes this forming a neutron star
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

pulsar

A

rotating neutron star

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

red super giant star

A

red in colour
large luminosity
low temperature
large mass
large surface area

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

many regions of the universe that do not contain any stars why this contradicts newton’s model of the universe

A
  • newton’s model states that universe is infinite and uniform
  • so there must be a star along every line of light from earth making the sky bright at night
  • but as there are regions without stars newton’s model is incorrect
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

big bang model is consistent

A
  • space and time originated with the big bang
  • universe is expanding
  • due to expansion light from distant stars has not yet reached / or has been redshifted to infrared and is not visible
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

observed redshift of light from many distant galaxies is explained

A

the universe is expanding

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

lendamaxT and big bang model

relationship between those two
or how does lenda max supports big bang theory

A
  • the neutral temperature of the universe was very high after the big bang
  • due to expansion and time, the temperature has now fallen to 2.7k
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

experimental evidence that support big bang

A
  • Hubble showed that galaxies are moving away from each other
  • showing that the universe is expanding from an originated single point
17
Q

distinguish between solar system and galaxy

A
  • a galaxy is much larger in size then a solar system
  • a galaxy is more luminous
  • a galaxy contains many solar systems
18
Q

distinguish between planet and comet

A
  • a comet is a small icy body whereas a planet is made of rock and gas
  • comets have larger orbits then planets
  • comets often have tails, planets do not
19
Q

main sequence star

A
  • absorption lines in the spectrum correspond to the h emission spectrum
  • main sequence stars are rich in hydrogen
20
Q

radius of a white dwarf reaches a stable value

A
  • the star collapses until gravitational force inwards is balance by electron degeneracy pressure outwards
21
Q

international collaboration has helped to refine this value

A
  • data collection is expensive so cost can be shared
  • data from around the world can be collected
22
Q

main sequence star are in equilibrium under the action of forces - equilibrium is achieved

A
  • gravitational force inwards balanced by radiation pressure outwards
23
Q

star from main sequence to final stable phase

A
  • main sequence to red giant
  • the planetary nebula carries a core of mass <1.4mo
  • so becomes a white dwarf
24
Q

hubble’s law assumption

A

rate of expansion of universe has been constant
- universe expand at a constant rate

25
Q

constellation / cluster

A
  • stars in a cluster are close together, these in a constellation are not
  • stars in a cluster are held together by gravity, those in a constellation are not
  • stars in a cluster are the same age these in a constellation are not
26
Q

composition of star can be determined

A
  • absorption spectrum of the star is observed
  • absorption line give an indication of the elements that make up the star
27
Q

main sequence to final stage

A

red giant -> planetary -> white dwarf

28
Q

Hubble measured the recessional velocity of galaxies

A

measured the redshift of the galaxies
used z = v/c to find v

29
Q

prevents star from collapsing further

A

electron degeneracy pressure

30
Q

origin of EM radiation

A

thermal energy

31
Q

red shift

A

observed wavelength is greater than that emitted

32
Q

CMB evidence for big bang model

A
  • the CMB comes from all regions of space it is uniform
  • the wavelength of the CMB matches that predicted by coding of the universe after the big bang / or by expansion of the universe
  • coding the wavelength of CMB matches the prediction that universe is expanding
33
Q

observation of spectra from distant galaxies provide evidence that the universe is expanding

A

distant galaxies have their spectra red shifted

34
Q

sun become a red giant

A
  • fusion of hydrogen in the core stops and the core contract helium fusion now begins in the core causing the sun to expand and become more luminous.
35
Q

sun maintain a constant radius after it becomes a white dwarf

A

electron degeneracy pressure prevents further contraction

36
Q

light spectra of distant galaxies confirm hypotheses about the expansion of the universe

A
  • spectra are redshifted
  • galaxies are moving away from us
37
Q

Hubble unlikely to predict the age of the universe

A

assumes the universe has a constant rate of expansion
there is uncertainty in the value of Ho

38
Q

asteroids

A

lump rock
between mars and Jupiter in the asteroid belt