11B.2 Stellar classification Flashcards

1
Q

what have Astronomers done with stars

A

they have classified stars into groups according to their temperature, as it determines the spectral output of the star, and it can also suggest its chemical composition and age

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2
Q

what is the order of spectral star classes from hottest to coolest

A

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3
Q

the hotter the stars are

A

the more mass and more luminous they are, and that is because their is a large gravitational pressure at the centre of a massive star which makes the nuclear fission within the star very fast, producing loads of energy and using the hydrogen fuel in the star at a very high rate (so luminosity). In addition the massive stars and very large large. (so mass)

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4
Q

what do the white lines in the light spectra show

A

the position of absorption lines, which give us information about the chemical composition of the star, and the doppler shift which tells us their velocity

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5
Q

if we combine light with equal intensity of thee visible spectrum we will make

A

white light

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6
Q

what is the Hertzsprung-Russel diagram

A

a plot of stars, showing luminosity(or absolute magnitude) on the y-axis, and the temp(or spectral class) on the X-axis

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7
Q

the temp measurements of stars from the Hertzsprung-Russel diagram is considered to be

A

that the star is considered to be a black body

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8
Q

the luminosity measurements form the Hertzsprung-Russel diagram are

A

not that accurate since measuring distances if from the star to earth isn’t completely accurate

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9
Q

what is the main sequence

A

a diagonal line form the top left to bottom right of a Hertzsprung-Russel diagram which marks stars that are in a generally stable phase of their existence

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10
Q

what is also seen on the Hertzsprung-Russel diagram

A

white dwarfs bottom right, red gaint on the top left with red supergiant on tope of it

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11
Q

what is also seen on the Hertzsprung-Russel diagram

A

white dwarfs bottom right, red giant on the top left with red supergiant on top of it

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12
Q

why are some stars more polluted in the Hertzsprung-Russel diagram compared to others

A

because some stars have a very shorter life spam so their isn’t many of them to see, that’s why the tope left and the bottom right of the main sequence isn’t as populated as the middle

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13
Q

what are the two elements that stars are originally made form

A

hydrogen, and helium

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14
Q

what is a protostar

A

a mass of dust and gas clumping together under the force of gravity prior to the start of nuclear fission within its core, which will go on to become a star

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15
Q

what is a neutron star

A

one of the possible conclusions to the life of a large mass star. it is a very small and dense, and it is composed of neutrons

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16
Q

what is a black hole

A

one of the possible conclusion to the life of a large mass star. a region of space-time in which gravity is so strong preventing anything from escaping it including EM radiation

17
Q

how does nuclear fission release energy

A

the energy difference between the nuclei before and after fusion means energy release often as EM radiation to heat the star

18
Q

how does a star not collapse on it self due to gravity

A

the force of gravity is going against the outward pressure made from nuclear fission (EM radiation)

19
Q

What is the low mass star life cycle

A

so first is the protostar, after that the hydrogen atoms start boning to form helium atoms forming a main squence

20
Q

What is the low mass star life cycle

A

so first is the protostar, after that the hydrogen atoms start boning to form helium atoms forming a main sequence, at this stage the radiation pressure outward, and the gravity force inward are at equilibrium, eventually the star will run low of hydrogen fuel, but will have produced so much more energy that it will slightly expand, this expansion will cause the temp to fall and to form a red giant, then after most of the hydrogen fuel has been used and the star will start fussing helium nuclei, this complex process can cause an explosion which throws materials from the star into space, then this will form a planetary nebula, as the fuel runs out the outward pressure drop causing the star to collapse on its self forming a white dwarf as heat would increase. as time continues the white dwarfs energy will will run out and it will die making it pass through a red drawf then a black dwarf

21
Q

what is a planetary nebula

A

the remains of an explosion at the end of a low-mass star. materials that may eventually join together into new planets

22
Q

what is a black dwarf

A

it is the final stage of a low-mass star, when nuclear fission has ceased and it cooled down so it no longer emits visible light

23
Q

what is the massive stars life cycle

A

so first is the protostar then the hydrogen would react together to form a blue super giant at this point the outward radiation and the force of gravity inward are at eq, once most of the hydrogen as been used up a lot of energy releases at that expands the star causing it to form a red super giant dropping the energy down, but since the massive starts have much more larger energies fusion between nuclei larger than He starts forming elements which are multiple of fours like carbon, oxygen and silicon, once all of the nuclei has fused to form iron(which is the highest nuclei that can be made with the energy provided) the outward radiation would drop causing the star to collapse on its own, this sudden large collapse produces a large burst of energy in the supernova explosion, this releases so much energy that all the elements within our universe are produced, after the supernova the entire star may be completely shattered, but if there is a central core of stellar matter it would form a neutron star or if big enough a black hole

24
Q

why is neither the black dwarf nor the neutron star, nor the black hole plotted on the Hertzsprung-Russel diagram

A

because they are hard to spot since they emit to light as will as the black dwarf so far is only theoretical as there hasn’t been time for any to develope