Our Solar System
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Transcript Our Solar System
Our Solar System
A Journey to Our Planetary Neighbors
Ideas about the night sky have changed
over time…
Earth-centered model – early Greeks
thought planets, Sun, Moon and stars
rotated around the Earth
Modern view –
The
sun is the center of our solar system
All other objects in the solar system
revolve around the sun in elliptical orbits at
different speeds.
How did our solar system form?
A nebula of gas, ice, and dust slowly
formed in space, and rotated in space.
The cloud began to contract and the
matter was squeezed into less space.
The cloud became dense, heated up
and triggered a nuclear fusion reaction
that created the sun.
What happened next?
All leftover matter became the planets
and asteroids
The four inner planets – (Mercury, Venus,
Earth, and Mars) are small and rocky with
iron cores
The four outer planets – (Jupiter, Saturn,
Uranus, and Neptune) are large,
lightweight, and composed of gases.
Inner Planets
Mercury - closest to the Sun, smallest
planet
Many
craters and high cliffs
No true atmosphere so temperatures can
range from -292 to 806° F.
It orbits the sun once every 88 days and is
an average of 36 million miles from the
sun.
Inner Planets
Venus – second from the sun and
similar to the Earth in size and mass
Mostly
smooth volcanic plains
Extremely dense atmosphere of clouds
Carbon dioxide gas traps solar energy
resulting in temperatures between 842 to
887° F.
It is an average distance of 67 million miles
from the sun and orbits every 225 days
Inner Planets
Earth – third planet from the Sun
More than 70 percent of surface is covered
with water
Atmosphere consists of several layers, is
mostly composed of nitrogen and oxygen,
and protects the surface from meteors and
Sun’s radiation
It is an average of 93 million miles away
from the sun, and completes its orbit in
365.5 days
Inner Planets
Mars – fourth planet from the Sun
Called red planet because of iron oxide in rocks
Polar ice caps made of frozen carbon dioxide and
water
Surface contains gullies, mountains and canyons,
plains and the largest volcano in the solar system
The thin atmosphere mostly contains carbon
dioxide
It is an average of 141 million miles from the Sun,
and completes its orbit in 1.9 years
Asteroids and Other Objects in Our Solar
System
Asteroids – rocks similar to that which
formed the planets
Asteroid Belt – group of asteroids that
orbit the Sun between the planets Mars
and Jupiter
Comets
Comet - dust and rock particles
combined with frozen water, methane,
and ammonia
Halley’s
comet (occurs every 76 years),
Hale-Bopp (1995)
Look similar to a dirty snowball
The ice and dust vaporize as it
approaches the sun
This
forms a comets tail
Meteoroid, Meteor, and Meteorite
Meteoroid – small pieces of debris in
space
Meteor – small meteoroid that burns up
in Earth’s atmosphere (falling or
shooting star)
Meteorite – meteoroid that strikes Earth
Outer Planets
Jupiter – Fifth planet from the sun and
the largest in our solar system
Atmosphere
mainly consists of hydrogen
and helium
Surface is suspected to be composed of
liquid hydrogen and helium, and may have
solid core at the center
It is an average of 484 million miles from
the sun and 11.8 years to complete one
orbit
Has 16 moons
Outer Planets
Saturn – sixth planet from the Sun
Thick outer atmosphere of hydrogen,
helium, ammonia, methane, and water
vapor
Might have rocky core
Rings that circle around planet are
composed of ice and rock particles
It is an average of 887 million miles from
the Sun, and completes one orbit in 29.5
years
Outer Planets
Uranus – seventh planet from the sun
Atmosphere of hydrogen, helium, and
methane
Rotates on its side
Contains thin, dark rings
It is an average of 1.8 billion miles from
the sun, and completes one orbit in 84
years
Outer Planets
Neptune – eighth planet from the Sun
Atmosphere is similar to that of Uranus
Storms on Neptune reveal an active and
rapidly changing atmosphere
It is an average of 2.8 billion miles from the
sun, and completes its orbit every 165
years