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Stellar Evolution

Authored by Isabel Perez

Physics

University

Used 22+ times

Stellar Evolution
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10 questions

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1.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Stars can take different evolutionary paths due to their initial:

Brightness

Mass

Temperature

Color

2.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Helium flash occurs:

In very massive stars

When the helium nucleus breaks its degeneracy

At the Asymptotic Giant Branch phase

when the nucleus burns helium

3.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Which following states regarding the main sequence is wrong?

Main sequence undergo fusion hydrogen within their cores.

Mass is the key factor to determine the lifespan of the star

The energy is transported via radiation or convection

Hydrogen burns in a shell

4.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Which following evolutionary sequence is correct?

PMS-AGB-RGB-BH

MS-HB-RGB-AGB-SN-WD

MS-RGB-HB-AGB-PN-WD

MS-RGB-HB-AGB-SN-WD

5.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

When a red giant's outer atmosphere drifts away, it becomes:

Expanding nebula

Planetary nebula

White dwarf cloud

Planetary cloud

6.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Why will a low/medium mass star will never create a Black Hole

Collapse is too slow

Collapse is too fast

Electron degeneracy

Proton degeneracy

7.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Stars like the Sun probably do not form iron cores during their evolution because

All the iron is ejected when they become planetary nebulas.

Their cores never get hot enough.

Their strong magnetic fields keep their iron in their atmospheres.

The iron converted in heavier elements through proton capture

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