5.2 Life Cycle of Stars Quiz

5.2 Life Cycle of Stars Quiz

9th Grade

7 Qs

quiz-placeholder

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5.2 Life Cycle of Stars Quiz

5.2 Life Cycle of Stars Quiz

Assessment

Quiz

Science

9th Grade

Practice Problem

Easy

NGSS
HS-ESS1-1, HS-ESS1-3, HS-PS2-4

Standards-aligned

Created by

Kristopher Knutson

Used 14+ times

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7 questions

Show all answers

1.

DRAG AND DROP QUESTION

1 min • 1 pt

Low mass stars will burn through their fuel ​ (a)   high mass stars.

slower than
faster than
at the same rate as

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

When is a star considered a main-sequence star?

When it is no longer fusing any elements in its core

When it is in the final stages of its life and is about ready to die

When it is fusing hydrogen into helium in its core and is in a stable phase of its life cycle

When it has exhausted its hydrogen fuel and is starting to fuse heavier elements

Tags

NGSS.HS-ESS1-1

3.

MATCH QUESTION

1 min • 4 pts

Match the correct phase of a low mass star’s life cycle to the proper description.

White Dwarf

Has begun fusion and is in stellar equilibrium.

Protostar

Spinning region that will develop into a star, no fusion yet.

Main Sequence

A small, dense remnant of a star that has used its nuclear fuel and no longer undergoes fusion.

Red Giant

A low-mass star that has expanded and cooled.

Tags

NGSS.HS-ESS1-3

4.

REORDER QUESTION

1 min • 5 pts

Put the stages of a high-mass star's life in order with "1" being the earliest stage:

Black Hole

Main Sequence

Solar Nebula

Protostar

Supergiant

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

An older main sequence star would have a greater percentage of helium than a younger main sequence star because...

the older star has had more time to fuse hydrogen into helium in its core.

the older star is larger and hotter, causing it to fuse helium faster.

the older star's core has more mass and has more fuel to burn.

the older star is fusing elements other an hydrogen into helium.

Tags

NGSS.HS-ESS1-1

NGSS.HS-ESS1-3

6.

DRAG AND DROP QUESTION

1 min • 2 pts

Stellar equilibrium is the balance between the inward force of​ (a)   trying to crush the star, ​and outward pressure caused by​ (b)   which keeps a star stable in size and shape.

gravity
nuclear fusion
nuclear fission
magnetism
solar wind

Tags

NGSS.HS-ESS1-1

NGSS.HS-PS2-4

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Media Image

Which star(s) would have a shorter lifespan than the Sun?

A

B

Both A & B

D

Tags

NGSS.HS-ESS1-1

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