
The Moon Features
Presentation
•
Science
•
9th - 12th Grade
•
Practice Problem
•
Easy
+7
Standards-aligned
Tom Temple
Used 5+ times
FREE Resource
12 Slides • 9 Questions
1
27-2
The Moon
2
•Gravity is one sixth of
earth’s (divide your weight
by six)
•No atmosphere as a result
•Up to 127* C during day and
down to –173* C at night
* Slow rotation - due to "Sychronous
Tidal Lock with Earth
3
Fill in the Blank
4
Multiple Choice
The Moon lacks and atmosphere because
It never had time to form.
There are no plants there to form one.
There is not enough gravity to hold onto one.
5
Dropdown
6
• Large, dark areas on the Moon are termed Maria meaning sea.
• Represent volcanic flows that occurred before 3 billion years ago.
They average 3km lower in elevation.
• Lighter colored, heavily cratered, areas are known as Highlands
are composed of regolith (broken rock)
7
Multiple Choice
The lowland areas of the moon are called Mare which is latin for
lake
valley
sea
ocean
8
Fill in the Blank
9
Moon rock is similar to Earth rock
•Mare Basalt -- This sample
of mare basalt, ~3.7 billion
years old, was collected by
Apollo 17 astronauts. The
small holes in the sample are
vesicles, which formed by the
degassing of the lava as it
cooled. Courtesy of NASA
10
• Highland breccia --
collected by Apollo 16
astronauts. The breccia
contains basalt fragments
broken by a meteorite
impact and welded by the
heat and pressure of the
impact process. The rock
is 3.9 billion years old.
Courtesy of NASA.
11
Drag and Drop
12
• Highlands Anorthosite --
Roughly 50% of the outer
highlands crust consists of
the rock anorthosite. It is a
plagioclase-rich rock
containing some pyroxene,
with or without olivine. The
sample shown here was
collected by Apollo 16
astronauts and is 4.4 billion
years old.
13
Multiple Choice
Highlands anorthosite rocks are mostly composed of the mineral
quartz
plagioclase
pyroxene
olivine
14
Giant Impact Hypothesis
•Is believed that a Mars-sized object hit the earth
early in the development of our solar system
•Material ejected from the glancing blow coalesced
into the Moon
15
Impact Craters
•Ejecta is material that fell
back to the surface after
impact
•Some craters have long
trails of ejecta known as
Rays
16
•Long, deep channels that run through
the maria are known as Rilles.
Hypotheses include: lava channels,
collapsed lava tubes, but most likely
caused by thermal erosion
17
Match
Match the following
long deep channels form by expansion on the moon
long trails of material caused by big impacts
lots of these on the moon caused by impacts
what the moon is NOT made of
Most accepted theory of the formation of the moon is based on this idea
rilles
ejecta
craters
cheese
impact
rilles
ejecta
craters
cheese
impact
18
Lunar Interior
• The highlands anorthosite is
dominated by the mineral
plagioclase feldspar.
• anorthosite crystallized early
in the moon's formation from
a global magma ocean.
19
• lighter plagioclase floated
upward to form the
anorthosite crust.
• The heavier minerals
olivine and pyroxene
sank toward the bottom of
the magma ocean to form
the moon's upper mantle.
20
•The Moon has minor
quakes
•The crust is thinner
on side facing earth
•The Moon may also
have a small iron core
21
Match
Match the layer of the Moon with the correct composition
crust
mantel
core
atmosphere
plagioclase
pyroxene and olivine
iron
none
plagioclase
pyroxene and olivine
iron
none
27-2
The Moon
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