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Transcript
Comets and Asteroids
BY Travis Mazza
&
Mack Pekar
Comets



Comets are small, fragile,
irregularly shaped bodies
composed of a mixture of
non-volatile grains and frozen
gases.
They have highly elliptical
orbits that bring them very
close to the Sun and swing
them deeply into space, often
beyond the orbit of Pluto.
As comets approach the Sun
they develop enormous tails
of luminous material that
extend for millions of
kilometers from the head,
away from the Sun.
Cont.


develop a surrounding cloud
of diffuse material, called a
coma, that usually grows in
size and brightness as the
comet approaches the Sun.
Usually a small, bright
nucleus (less than 10 km in
diameter) is visible in the
middle of the coma. The coma
and the nucleus together
constitute the head of the
comet.
When far from the Sun, the
nucleus is very cold and its
material is frozen solid within
the nucleus. In this state
comets are sometimes
referred to as a "dirty
iceberg" or "dirty snowball"
Cont.



The evaporated molecules boil off
and carry small solid particles
with them, forming the comet's
coma of gas and dust
As the comet absorbs ultraviolet
light, chemical processes release
hydrogen, which escapes the
comet's gravity, and forms a
hydrogen envelope
The tail of the comet stays away
from the sun because of the solar
winds of the sun blowing the tail
away
Asteriods




Asteroids are rocky and
metallic objects that orbit the
Sun but are too small to be
considered planets.
They are known as minor
planets
Asteroids range in size from
Ceres, which has a diameter
of about 1000 km, down to
the size of pebbles. Sixteen
asteroids have a diameter of
240 km or greater
Most, are found in the main
belt that exists between the
orbits of Mars and Jupiter
Cont.


Asteroids are material left over from the formation of the solar system
One theory suggests that they are the remains of a planet that was
destroyed in a massive collision long ago

Asteroids that are on a collision course with Earth are called meteoroids.
Work Cited
http://encke.jpl.nasa.gov/index.html
http://www.solarviews.com/ss.html