Stellar Evolution of Low Mass Stars

Stellar Evolution of Low Mass Stars

9th - 12th Grade

26 Qs

quiz-placeholder

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Stellar Evolution of Low Mass Stars

Stellar Evolution of Low Mass Stars

Assessment

Quiz

Physics

9th - 12th Grade

Medium

NGSS
HS-ESS1-1, HS-ESS1-3, HS-PS1-8

+1

Standards-aligned

Created by

Mary Hing

Used 14+ times

FREE Resource

26 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following occurs in stage 8, subgiant branch?

The core contracts

The surface cools

the core temperature decreases

the surface temperature is around 10000K

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What are the properties of black dwarfs?

Is is seen at the right side of the HR diagram

they have been observed in our galaxy

they are very large and cold

they are cold cores of low mass stars

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following is NOT a planetary nebula?

Dumbbell nebula

Orion nebula

Ring nebula

Cat eye nebula

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following is NOT a property of a white dwarf?

They are located in the lower left side of the HR diagram

They are very hot cores of low mass stars

They have ejected all the gas and only the core remains

They continue to fuse helium to carbon and hydrogen to helium in shells around the core

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Hydrogen shell burning is:

helium continues to fuse into carbon in the core

hydrogen continues to fuse into carbon in a shell around the core

carbon fuses to helium in the core

hydrogen fuses to helium in a shell around the core

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following does NOT happen during Stage 10?

helium continues burning

carbon ash forms in the core

80% of the mass is lost

the brightness decreases

Tags

NGSS.HS-ESS1-1

NGSS.HS-ESS1-3

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following does NOT occur in stage 12?

hydrogen and helium continue to burn in shells

radius oscillates more and more violently

burning remains stable

Envelope of gas is ejected

Tags

NGSS.HS-ESS1-3

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