Studying Space
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Transcript Studying Space
Studying Space
Astronomy
study of the universe
Modern Calendar
years, months, days
Year
Time for Earth to orbit once around sun
Month
time for moon to orbit once around Earth
Day
time required for Earth to rotate once on
axis
Astronomer
Axis
scientists who study the Universe and the
Earth’s place in it
imaginary line-runs from North to South
pole
Early Astronomers
Earth Textbook
Pps 348-349
Groups of 3-4
Get a rectangular piece
of paper and create a
timeline indicating date,
astronomer/object and
significant contributions.
15 mins to complete for
a grade – NEAT and
ACCURATE
The Solar System
The Moon
¼ Earth’s diameter
less dense than Earth
no atmosphere (temp
varies greatly)
no liquid water;
evidence of small ice
patches near poles
no change in land’s
surface from
weathering/erosion
theory: planet-sized
object collided with
Earth to form moon
Motions of the Moon
Moves 2 ways:
1. rotates on its axis
2. revolves around
Earth
one day = one year
same side of moon
always faces Earth
Phases of Moon
different shapes of the
moon you see
caused by changes in
position of moon,
Earth, and sun
the phase you see
depends on how much
of the sunlit side of the
moon faces Earth
Eclipses
object in space comes
between the sun and a
third object and casts a
shadow
two types:
solar and lunar
Solar Eclipse
http://www.pbslearningmedia.org
/resource/ess05.sci.ess.eiu.totalecli
pse/total-solar-eclipse-animation/
when moon passes
directly between Earth
and sun, blocking sun
from Earth
occurs at new moon
Lunar Eclipse
Earth blocks sunlight
from reaching moon
occurs at full moon
The Sun
Sun
source of most energy
on Earth
a star; smaller and less
bright than many
others
most massive in our
solar system (99.8% of
solar system’s total
mass)
Sun
1. Core
made of 6 layers:
energy comes from nuclear
fusion (hydrogen atoms join to
form helium)
15 million degrees Celsius
2. Radiation
Zone
very tightly packed gas; very
dense
3. Convection
Zone
outermost layer of sun’s interior
hot gas rises from bottom and
cool as approach top
4. Photosphere
visible part of sun that
we can see
5. Chromosphere
thin region (only
30,000 km thick)
faint red light we only
see during eclipses
6. Corona
sun’s outer atmosphere
like a halo
thins into streams of
charged particles (solar
wind)
Sunspots
Solar Flares
areas of gas on sun’s
surface that are cooler
than gases around
them
regions of extremely
high temperature and
brightness that
develop on sun’s
surface
flares erupt and send
electrically charged
particles into solar
system
The Planets
Planets
Inner Planets
held in orbit by force of
gravity exerted by sun
two groups: inner and outer
Mercury, Venus, Earth,
Mars
small, dense, rocky surfaces
only Earth and Mars have
moons
Outer Planets
Jupiter, Saturn,
Uranus, Neptune
much larger, do not
have solid surfaces
gas giants; made of
mostly hydrogen and
helium (liquid due to
pressure)
all have many moons
Other Members of the Solar System
Satellites
objects that orbit
planets (moons)
Asteroids
fragments of rock that
orbit the sun with the
planets
travel in asteroid belt
between Mars and
Jupiter
Meteoroids
Meteor
Meteorite
chunks of rock or dust that in
space
sometimes enter Earth’s
atmosphere
when enter Earth’s
atmosphere
when it impacts surface of
Earth
Comet
loose collections of ice, dust,
and small rocky particles
travel around sun in elliptical
path
head (coma) is ice, dust
as approaches sun, heat
causes outer layers to stream
outward (tail)