Exploring the Interstellar Medium  (ISM)

Exploring the Interstellar Medium (ISM)

11th Grade

10 Qs

quiz-placeholder

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Exploring the Interstellar Medium  (ISM)

Exploring the Interstellar Medium (ISM)

Assessment

Quiz

Science

11th Grade

Hard

NGSS
HS-PS4-4, HS-PS4-3

Standards-aligned

Created by

Jennifer Low

FREE Resource

10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

What is the interstellar medium (ISM) primarily composed of?

99% gas and 1% dust

90% hydrogen and 10% helium

50% gas and 50% dust

75% hydrogen and 25% helium

2.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

What is the typical temperature of the dust in the interstellar medium (ISM)?

10 K

100 K

273 K

1000 K

3.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Why is it necessary to use telescopes that detect light at wavelengths longer than visible light to observe the ISM?

Because the ISM is very hot

Because the ISM is very cold

Because the ISM is very dense

Because the ISM is very bright

Tags

NGSS.HS-PS4-4

4.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

What effect does dust in the ISM have on light at optical wavelengths?

It amplifies the light

It blocks the light

It changes the color of the light to blue

It makes the light brighter

Tags

NGSS.HS-PS4-4

5.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

What is the phenomenon called when dust absorbs and scatters blue light more than red light, making a star look redder than it really is?

Optical extinction

Interstellar reddening

Light amplification

Blue shift

Tags

NGSS.HS-PS4-4

6.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Why is the sky blue?

Because the atmosphere absorbs all colors except blue

Because blue light is more scattered than red light

Because the Sun emits more blue light

Because blue light is absorbed by the atmosphere

Tags

NGSS.HS-PS4-3

7.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Why do sunsets appear red?

Because the Sun emits more red light at sunset

Because red light is absorbed by the atmosphere

Because the light has to travel further through the atmosphere, leaving more red light after the blue is scattered away

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