Astrophysics - Stellar evolution Flashcards

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1
Q

What colour are the coolest stars?

A

red - M

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2
Q

What colour are the hottest stars?

A

blue - O

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3
Q

What is the luminosity of a star?

A

this measures how much energy is given out by a star and will depend on the size and temperature of the star

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4
Q

What is the brightness of a star?

A

how bright a star appears from earth, depends on the luminosity of the star and the distance

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5
Q

What is absolute magnitude?

A

This is the brightness of the star if it was at a standard distance from earth. It allows us to make better comparisons between stars.

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6
Q

Spectral Class types for Stars

A
O - blue
B - blue/white
A - white
F - yellow/white
G - yellow
K - yellow/orange
M - red
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7
Q

Different stages in the evolution of stars

A
  • nebula
  • protostar
  • average star
  • red giant
  • planetary
  • white dwarf
  • massive star
  • red supergiant
  • supernova
  • neutron statr
  • black hole
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8
Q

stellar nebular

A

mostly hydrogen, forms from clouds of gas and dust in the galaxy

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9
Q

Protostar

A
  • as the mass falls together it gets hot
  • a star is formed when it is hot enough for the hydrogen nuclei to fuse together to make helium
  • this is known as nuclear fusion
  • the fusion process releases energy, which keeps the core of the star hot
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10
Q

main sequence star

A
  • the force of gravity holding the star together is balanced by higher pressure due to the high temperatures
  • this phase in a star’s life usually lasts for around 10 billion years
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11
Q

red giant star

A

when the hydrogen has been completely used up in the fusion process, larger nuclei begin to form and the star may even expand to become a red giant

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12
Q

white dwarf

A
  • average mass star will throw off the outer layers, but the centre will cool and contract into a white dwarf
  • as the light then fades it will become a black dwarf
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13
Q

planetary nebula

A
  • cloudy remnants of smaller stars that have shed their outer layers of gas, but haven’t exploded into supernovas
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14
Q

red supergiant

A
  • eventually the hydrogen at the core of the star will run out as it has all been used up in nuclear fusion
  • the star will then expand into a red supergiant
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15
Q

supernova

A
  • the red supergiant will eventually explode, causing a supernova, which throws out gas and dust into space
  • this type of explosion is so strong that it would be too dangerous to stimulate on earth
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16
Q

neutron star/black hole

A
  • the force of the supernova will cause the star’s core to collapse
  • this then either forms a neutron star, a small star with a diameter of a few km made solely of neutrons, or a black hole, a region of space with a gravitational field so strong that not even light can escape it
17
Q

What is the Hertzsprung-Russel diagram?

A

A graph relating to the surface temperatures and absolute brightness of stars

18
Q

What are the four key components of the hertz sprung-russel diagram group?

A
  • supergiants (top right)
  • giants (below supergiants, off to the right)
  • main sequence (central, diagonal S shape)
  • white dwarf (bottom left)