Stellar Physics Flashcards

1
Q

What is the symbol and units of luminosity?

A

L
( J/s or watts)

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2
Q

What is b the symbol of?

A

Apparent brightness

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3
Q

How are stars formed?

A

They’re formed in interstellar clouds when gravitational forces overcome thermal pressure and cause a molecular cloud to contract until the core becomes hot enough to sustain nuclear fusion, which then provides a thermal pressure that balanced the gravitational force

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4
Q

What do the proton-proton chains in stellar fusion reactions do?

A

Convert hydrogen to helium

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5
Q

How do stars maintain their outward thermal pressure to balance inwards gravitational forces?

A

Hydrogen fusion in the core of a star supplies energy to balance forces

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6
Q

What happens when the hydrogen in the core of a star becomes depleted?

A

Nuclear fusion in the core ceases and gravitational forces cause both the core and the shell (still containing hydrogen) surrounding the core to shrink.

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7
Q

In a star like the sun what happens when the hydrogen shell around the stars core becomes hot enough for hydrogen fusion?

A

Hydrogen fusion leads to an increase in pressure which pushed the surface f the star outwards causing it to cool -> at this stage the star will be a giant or supergiant.

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8
Q

When does a star such as the sun become hot enough for helium in the core to begin fusion?

A

When the core shrinks

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9
Q

What determines the lifetime of a star?

A

The mass of the star

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10
Q

Ultimately what does every star become?

A

A white dwarf, a neuron star or a black hole. The mass if a star determines its eventual fate

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