Transcript comet

Vocabulary words

Comets - Are loose collections of ice, dust, and small rocky particles whose
orbits are usually very long, narrow ellipses.

Coma – The fuzzy outer layer of a comet.

Nucleus – The solid inner core of a comet.
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Kuiper belt – A doughnut-shaped region that stretches from around Pluto’s
orbit to about 100 times Earth’s distance from the Sun.
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Oort Cloud – A spherical region of comets that surrounds the solar system.
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Asteroid Belt - The region of the solar system between the orbits of Mars and
Jupiter, where many asteroids are found.
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Asteroids – Rocky objects revolving around the sunhat are too small and
numerous to be considered as planets.
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Meteoroid- A chunk of rock or dust in space.

Meteorites - Meteoroids that pass through the atmosphere and hit Earth’s
surface.

Meteor – A streak of light in the sky produced by the burning of a meteoroid in
Earth’s atmosphere.
COMETS
The
word "comet" comes from the Greek
word for "hair.”
Our
ancestors thought comets were stars
with what looked like flowing hair trailing
behind.
COMETS: “DIRTY SNOWBALLS”
 Comets
are loose collections of ice, dust, and
small rocky particles whose orbits are usually very
long, narrow ellipses.
STRUCTURE OF A COMET
A Comet’s Head
 Outer
layer= Coma (water vapor, CO2, and
other gases)
 Solid
inner core= Nucleus (frozen ice, gas and
dust )
COMET’S TAIL
 As
a comet approaches the sun and heats up,
some of its gas and dust stream outward, forming
a tail.
 Most
comets have 2 tails:
 gas
(ion), tail
 dust
tail
 Tails
point away from the sun because of the force
of the solar wind.
A
comet’s tail can be more than 100 million
kilometers long.
COMET’S TAIL
COMET’S ORBIT
 Comets
move in an elliptical shaped orbit.
ORIGIN OF COMETS
 Most
comets are found in 2 regions of the solar
system: Kuiper belt and Oort cloud.
 Kuiper
belt-doughnut-shaped region that extends
beyond Pluto’s orbit to about 100 times Earth’s
distance from the sun.
 Oort
cloud-spherical region of comets that
surrounds the solar system out to more than 1,000
times the distance between Pluto and the sun.
A
small and rocky space object.
 Most
 The
asteroids are found in the asteroid belt.
asteroid belt is located between the orbits of Mars
and Jupiter.
HOW MANY ASTEROIDS ARE THERE?
 There
are about 40,000 known asteroids that are over 0.5
miles (1 km) in diameter in the asteroid belt. About 3,000
asteroids have been cataloged.
 There
are many smaller asteroids (100,000).
 Asteroids
carbon.
are made of metals, silicate, iron, nickel, and
 The
first one discovered (and the biggest) is named Ceres;
it was discovered in 1801.
 Asteroids
range in size from tiny pebbles to about 578 miles
(930 kilometers) in diameter (Ceres).
ASTEROIDS BECOMING MOONS
 Asteroids
can be pulled out of their solar orbit by
the gravitational pull of a planet. They would then
orbit that planet instead of orbiting the Sun.
 Astronomers
theorize that the two moons of Mars,
Phobos and Deimos, are captured asteroids.
ASTEROID
STRIKE
 Scientists
hypothesize that one or more large
asteroids hit Earth 65 million years ago and
caused extinction of the dinosaurs.
 Scientists
also hypothesize that the largest mass
extinction, 250 million years ago, killing off 90% of
all species was also caused by a large asteroid.
Meteoroid-A
Meteoroids
chunk of rock or dust in space.
come from comets or asteroids.
 When
a meteoroid enters Earth’s atmosphere,
friction with the air creates heat and produces a
streak of light that you can see in the sky.
A
meteor is a meteoroid that enters Earth’s
atmosphere and burns up.
METEORITES
 Meteoroids
that pass through the atmosphere and
hit Earth’s surface are called meteorites.
 Classified
iron.
by composition: stony, iron ,or stony-
VIDEO CLIP ON METEOR SHOWERS

http://www.teachersdomain.org/resources/ess05/sci/ess/eiu/meteorsh
ower/index.html
http://www.youtube.com/watch?v=YHwTZs4xWFA