Astrophysics Flashcards

1
Q

Universe

A

Collection of billions of galaxies

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2
Q

Galaxy

A

Collection of billions of stars

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3
Q

Fusion

A

When two small nuclei join together to make one large nucleus

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4
Q

What is fusion the energy source for

A

Stars

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5
Q

Why does it need to be hot for fusion

A

The nuclei move very quickly because there is lots of KE, and it can overcome the electrostatic repulsive force

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6
Q

Why does fusion need high pressure

A

It forces the nuclei closer together which increases the probability of collision

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7
Q

Evolution of low mass stars (like the sun)

A

Nebula, protostar, main sequence, red giant, white dwarf, red dwarf

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8
Q

Evolution of high mass starts

A

Nebula, protostar, main sequence, red supergiant, supernova, EITHER neutron star, OR black hole

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9
Q

Nebula formation

A

Gravitational force causes cloud of dust and gas to attract together

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10
Q

Protostar formation

A

When there is enough mass in the nebula

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11
Q

Main sequence formation

A

The gravitational forces are balanced by the radiation pressure, so the star is stable (there is fusion)

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12
Q

Red giant formation

A

They are very hot in the centre so the star swells because the energy and radiation pressure increases, surface temp gets cooler.

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13
Q

White Dwarf formation

A

The star collapses from the gravitational forces, surface heats up (no fusion because no energy)

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14
Q

Red dwarf formation

A

Cools down and turns red (no fusion because no energy)

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15
Q

Supernova

A

Occurs when fusion stops abruptly, huge explosion radiating energy out into the universe

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16
Q

Neutron star

A

All neutrons, low mass, no fusion

17
Q

Black hole

A

A rip in the universe that nothing can escape from, no fusion

18
Q

Why would a supernova become a black hole

A

Higher mass

19
Q

Why would a supernova become a neutron star

A

Lower mass

20
Q

What does a low absolute magnitude of a star mean

A

A brighter star

21
Q

Apparent magnitude

A

A measurement of the brightness of a star as we measure it on earth

22
Q

Absolute magnitude

A

A measurement of the brightness of a star if all stars are the same distance away

23
Q

Why is absolute magnitude useful

A

Allows us to compare stars

24
Q

Speed of light

A

3 x 10^8 m/s

25
y-axis of HR diagram
Absolute magnitude
26
x-axis of HR diagram
Surface temperature
27
Line spectra
Where each element has a particular light that it emits. The different colours are based on the frequency
28
Doppler effect
moving towards: wavelength decreases and frequency increases moving away: wavelength increases and frequency decreases
29
Red shift
When an object emitting light moves away from us, the wavelength increases and appears more red
30
CMBR
Microwave radiation that is found to exist everywhere in the universe, in all directions
31
CMBR evidence
As the universe expanded, the wavelength of the radiation also expanded. There had to have been a huge release of energy to produce the radiation
32
Red shift of galaxies evidence
The galaxies furthest away from us have the greatest red shift, so they are travelling the fastest.