1/29
Name | Mastery | Learn | Test | Matching | Spaced | Call with Kai |
|---|
No analytics yet
Send a link to your students to track their progress
moon
a body that is smaller than a planet and orbits the planet
satellite
a object in orbit around a body with a larger mass
Sputnik I
Soviets in 1956
Explorer I
1st satellite launched by the US
6 Apollo spacecrafts
the number of Apollo spacecrafts the US sent to the moon between 1969-1972
moon’s gravity
not strong enough to hold gases so there is no atmosphere
134 °C
daytime temperature on the moon’s surface
-170 °C
nighttime temperature on the moon’s surface
27.3 days
moon’s rotational period around Earth
29.5 days
the number of Earth days 1 lunar day is on the moon
240,000 miles
distance from Earth to the moon
light areas
rough highlands composed of light colored rock (hills)
Maria
dark areas that are smooth and reflect little light (once lava)
Rilles
long, deep channels that run through the Maria (looks like dry riverbeds)
craters
bowl shaped depressions formed 4 billion years ago, from debris when solar system was formed
large craters
named for famous scholars and scientists (ex: Tycho and Copernicus), in addition to millions of smaller craters
ray
when crater forms, the displaced material settled in streaks that extend outward
seismographs
used to figure out information about the interior of the moon
60 km
depth of the crust
1000 km
thickness of the mantle
iron
makes up the core
1st stage of moon development
Mars sized body struck Earth and collision ejected a fragment into orbit, most of the material ejected was Silica-rich
2nd stage of moon development
surface of the moon covered by an ocean of hot molten rock, materials separated by density (Ti, Mg, Fe)
lunar rocks
meteorites strike the moon and crush much of the rock into dust and small fragments
Regolith
almost all of the surface is covered by this dust and rock that is 1m-6m thick
igenous rock
near the surface (O, Si)
lunar highlands
course-grained rock (Ca, Al)
basalts
found in Maria (Ti, Mg, Fe)
3rd stage of moon development
outer surface cooled and formed thick, solid crust; being struck by debris (craters); some meteorites broke through crust and molten rock and escaped, forming maria
most recent moon development stage
virtually all activity has stopped because of cooling