W9 L1 - Life cycle of stars Flashcards

1
Q

Up to what size are low mass stars

A

Equal to or less than 8 solar masses

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2
Q

Protostars evolve into what type of stars on the HR diagram?

A

Main sequence stars

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3
Q

What does the position of a star on the HR diagram depend on?

A

Its initial mass

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4
Q

Roughly how long does it take for a star the size of the sun to condense and enter the main sequence?

A

30 million years

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5
Q

Do stars of higher mass form faster or slower than the sun?

A

Faster

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6
Q

Do low mass stars form faster or slower than the sun?

A

Slower

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7
Q

What are the three categories of stars?

A

High mass, solar mass or sun-like, and low mass

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8
Q

What proportion of their life do stars spend on the main sequence?

A

90%

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9
Q

Which zone dominates in high mass and low mass stars respectively?

A

High mass = conduction, low mass = convection

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10
Q

What part of their mass do high mass stars have access to for fuel?

A

Only the part at their core

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11
Q

What is the rough equation for lifetime of a star?

A

Lifetime = mass / luminosity

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12
Q

How long can the lifetime of an M-type star be?

A

10^11 years

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13
Q

What proportion of the gas in a nebula might usually be converted to stars?

A

About 30%

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14
Q

Which stars form most commonly from a nebula?

A

Small stars

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15
Q

What are the two types of star clusters?

A

Open and globular

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16
Q

Which are older: open clusters or globular clusters?

A

Globular clusters

17
Q

what type of star cluster did our sun form within?

A

Open cluster

18
Q

What is an isochrone diagram used for?

A

Dating a cluster by working out the position of the stars on the HR diagram

19
Q

Where are most of the stars on the HR diagram for the Matariki cluster?

A

On the main sequence

20
Q

What age is the Matariki open cluster?

A

Roughly 100 million years

21
Q

What are the 3 steps for a low mass star when it leaves the main sequence?

A

Red giant, planetary nebula, white dwarf

22
Q

What are the 3 potential steps in the fork of the life of a high mass star when it leaves the main sequence?

A

Supergiant, supernova, then either neutron star or black hole

23
Q

What is the upper limit on how big stars can get?

A

Roughly 150 solar masses

24
Q

Roughly how long will the sun spend in the main sequence?

A

10 billion years

25
Q

Roughly how long will our sun spend as a red giant?

A

1 billion years

26
Q

How long will the sun spend as a planetary nebula?

A

A few thousand years

27
Q

What happens to the core of our sun at “core exhaustion” as it transforms to a red giant?

A

1) core H runs out, 2) inert helium core contracts from gravity, 3) H shell around core contracts, 4) H fusion occurs faster

28
Q

What is the Helium flash?

A

Core gets hot enough to fuse helium to carbon

29
Q

Will the Sun fuse beyond carbon and oxygen?

A

No

30
Q

Roughly what size will the sun be as a white dwarf?

A

The size of the earth

31
Q

At roughly what size do Type 1A Supernovae occur?

A

About 1.4 x the mass of the Sun

32
Q

Where do most of the fused elements accrete?

A

At the core