Stars And Cosmology Flashcards

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1
Q

How heavy are low mass stars?

A

0.5 Mo - 10 Mo

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2
Q

What stops gravitational collapse in a white dwarf?

A

Electron Degeneracy Pressure, two electrons can or exist in the same energy state, can support Fromm gravitational collapse a maximum mass of 1.44 Mo, this is the Chandrasekhar limit

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3
Q

In red supergiants there are layers where fusion occurs, where are the heaviest elements found?

A

In the core (up to iron) then layers of lighter elements near the outer surface

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4
Q

What prevents the nuetron star from collapse?

A

Nuetron degeneracy pressure ( they cannot occupy the same energy state)

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5
Q

What stars are located at the top of the HR diagram?

A

Supergiants

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6
Q

What stars are located at the bottom left of the HR diagram?

A

White Dwarfs

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7
Q

What are absorption spectra?

A

Some wavelengths of light are absorbed by the gas

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8
Q

What is theta in the diffraction grating equation?

A

the angle between the central maximum and the order of interest

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9
Q

Red is diffracted….

A

more than blue (higher wavelength)

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10
Q

What is Weins displacement law?

A

Maximum llamada is inversely proportional to T (in kelvin)

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11
Q

The peak wavelength corresponds too…

A

colour ( lower peak wavelength = more blue)

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12
Q

What is Stefans Law?

A

The total power radiated per unit surface area of a black body is directly proportional to the fourth power of the absolute temperature of the black body

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13
Q

If the object moves away from you then you have…

A

Red shift

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14
Q

What is the cosmological principle?

A

The Universe is isotropic and homogeneous

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15
Q

What does homogeneous mean?

A

Matter is uniformly distributed (the density of the universe is the same everywhere)

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16
Q

What does isotropic mean?

A

Looks the same in every direction to every observer

17
Q

How does CMB support the Big Bang theory?

A

the Big Bang theory predicts there were high energy gamma photons present when the universe was very young and hot, the expansion of the universe caused these to become red shifted, such that we now observe this primordial radiation as microwaves