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
Roughly how long will our sun spend as a red giant?
1 billion years
26
How long will the sun spend as a planetary nebula?
A few thousand years
27
What happens to the core of our sun at "core exhaustion" as it transforms to a red giant?
1) core H runs out, 2) inert helium core contracts from gravity, 3) H shell around core contracts, 4) H fusion occurs faster
28
What is the Helium flash?
Core gets hot enough to fuse helium to carbon
29
Will the Sun fuse beyond carbon and oxygen?
No
30
Roughly what size will the sun be as a white dwarf?
The size of the earth
31
At roughly what size do Type 1A Supernovae occur?
About 1.4 x the mass of the Sun
32
Where do most of the fused elements accrete?
At the core