Stars (C19) Flashcards

(39 cards)

1
Q

3 stages in star formation

A

nebula
Protostar
Star

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2
Q

Difference between star and protostar

A

star there is fusion

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3
Q

Describe energy changes in star formation

A

GPE –> Kinetic energy
causes heating up
leads to high pressure and fusion

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4
Q

Describe the equilibrium in a main sequence star

A

outward gas and radiation pressure

Inwards gravitational pressure

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5
Q

Name 8 space objects

A
Star
Planet
dwarf planet
asteroid
comet
Solar system
Galaxy
Universe
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6
Q

To form a red giant what size?

A

0.5 solar masses to 10 molar masses

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7
Q

To form a super red giant what size?

A

above 10 solar masses

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8
Q

Describe how a red giant forms

A

Hydrogen fuel runs low, so radiation pressure falls, causing the sun the have excessive inward pressure
this causes fusion of hydrogen in the outer layers to occur
So the outer layers drift apart and the star swells

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9
Q

Describe the life cycle of a small star

A
Nebula
Protostar
Main-sequence star
Red giant
White dwarf and nebula
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10
Q

Describe the life cycle of a large star

A
nebula
protostar
Main-sequence
Super red giant
Neutron star or black hole
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11
Q

What is the Chandrasekhar limit

A

core of 1.44 solar masses or more will result in a neutron star/black hole

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12
Q

Conditions for neutron star

A

core between 1.44 solar masses and 3

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13
Q

Conditions for blackhole

A

core greater than 3 solar masses

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14
Q

What stops a black hole/neutron star in smaller stars from forming

A

the electron degeneracy pressure resists the gravitational force

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15
Q

why is there electron degeneracy pressure

A

Pauli exclusion principle

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16
Q

What is the difference between super red giant and red giant

A

in super, heavier elements up to iron can be fused

17
Q

What causes a supernova

A

super red giant starts to fuse iron, which takes more energy than it releases, causing the rapid collapse of the star and explosion

18
Q

When are elements heavier than iron fused?

A

in supernova explosions

19
Q

Where do electrons want to exist

A

at the lowest energy state (most negative)

20
Q

Key thing with energy levels

A

Only discrete, certain jumps are possible, therefore only certain frequencies are emitted/absorbed

21
Q

What is an excited electron

A

an electron that has been moved to a higher energy state

22
Q

What does 0 represent on the electron level diagrams

A

a free elctron

23
Q

why is the energy levels for electrons negative

A

energy is required to remove the electrons

24
Q

Things that are excited…

A

quickly move down to lower energy states

25
What is spectroscopy
Analysis of light to determine the elements within a substance
26
What are the 3 types of spectrum
Continuous emission absorption
27
Why does a sun emit an absorption spectra
as the sun is a hot body so emits all wavelengths but the gasses on the surface absorb certain wavelengths
28
what is an emission spectra
unique set of lines for each element due to the specific photons it gives off
29
What is a diffraction grating
a device with has many slits designed to diffract light
30
Why are diffraction gratings used
has it seperates different wavelengths of light so reduces blurriness
31
What colour diffracts most in a diffraction grating
red
32
What colour diffracts least in a diffraction grating
violet
33
Why does different colours of light diffract different amounts
Depends on wavelength
34
What is a blackbody
an abject which absorbs (and therefore emits) a full spectrum of wavelengths
35
Why do hotter stars have lower peak wavelengths
Energy is inversely proportional to wavelength and energy is proportional to temp
36
What is Weins displacement constant
2.9 x 10^-3 Km
37
what is luminosity
total power radiated by a star
38
What two laws are needed to calculate the size of stars
Wiens and stefans
39
What is Stefan's Law
Luminosity is proportional to the radius squared and the temperature to the power of 4