Earth Moon and Sun

Earth Moon and Sun

6th Grade

25 Qs

quiz-placeholder

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Earth Moon and Sun

Earth Moon and Sun

Assessment

Quiz

Science

6th Grade

Hard

NGSS
MS-ESS1-1, MS-ESS1-2

Standards-aligned

Created by

Lisa Thompson

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25 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Because the Moon moves to different positions around Earth, we see different amounts of the ______________ half of the Moon. This is why we see different phases of the Moon.

pattern

illuminated

shadow

model

Tags

NGSS.MS-ESS1-1

2.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

There is a pattern to the position of the Moon because ___________________.

the Moon orbits around the Earth.

the Earth orbits around the Moon.

the Moon orbits around the Sun.

the Sun orbits around the Moon.

Tags

NGSS.MS-ESS1-1

3.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

How many days for one complete cycle of Moon Phases to occur?

25 days

27.3 days

29.5 days

31 days

Tags

NGSS.MS-ESS1-1

4.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Media Image

What phase of the moon is shown on the picture below?

waxing crescent

waxing gibbous

waning crescent

waning gibbous

Tags

NGSS.MS-ESS1-1

5.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

During a total lunar eclipse the moon is in Earth’s

corona.

penumbra.

umbra.

orbit.

Tags

NGSS.MS-ESS1-1

6.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Media Image

What phase of the moon is shown on the picture below?

new moon

full moon

first quarter

third quarter

Tags

NGSS.MS-ESS1-1

7.

MULTIPLE CHOICE QUESTION

1 min • 1 pt

Media Image

Astronomers made two observations of the Moon that were several days apart. Their observations are shown in the diagram above. The light part of the Moon appeared to get larger over time. Why did this happen?

Between the first observation and the second observation, the Moon rotated so that more of the light-colored rock on the Moon’s surface faced Earth.

Between the first observation and the second observation, the Moon moved so that the astronomers were able to see more of the half that faces the sun.

Between the first observation and the second observation, the Moon moved closer to the sun so more sunlight reached the Moon’s surface.

Between the first observation and the second observation, Earth moved so its shadow was blocking less of the Moon so the astronomers were able to see more of it

Tags

NGSS.MS-ESS1-1

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