Stellar Evolution

Stellar Evolution

University

10 Qs

quiz-placeholder

Similar activities

ZIP Class - Circuit SMP/SMA #1

ZIP Class - Circuit SMP/SMA #1

7th Grade - University

10 Qs

PENGENALAN BOLA JARING

PENGENALAN BOLA JARING

University

10 Qs

Universe Review

Universe Review

6th Grade - University

12 Qs

Astrophysics

Astrophysics

University

10 Qs

Failure of CM

Failure of CM

University

10 Qs

Hard Math

Hard Math

KG - Professional Development

7 Qs

Astronomy Quiz- Equinox

Astronomy Quiz- Equinox

University - Professional Development

15 Qs

Stars and stellar evolution

Stars and stellar evolution

11th Grade - University

15 Qs

Stellar Evolution

Stellar Evolution

Assessment

Quiz

Physics

University

Medium

Created by

Isabel Perez

Used 22+ times

FREE Resource

10 questions

Show all answers

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

Create a free account and access millions of resources

Create resources
Host any resource
Get auto-graded reports
or continue with
Microsoft
Apple
Others
By signing up, you agree to our Terms of Service & Privacy Policy
Already have an account?