A comet is a small icy
rocky body that orbits the Sun, some as small as 100
metres in diameter to around 6kms in diameter. Often
referred to as a "dirty snowball" comets consist of
carbon dioxide, water ice, methane and rock. In the
outer reaches of the Solar System they remain inert, it
is only when they approach the Sun that wonderful things
begin to happen. As they near the Sun the icy matter
that makes up the comet becomes energised by the heat of
the Sun. The solar winds force the energised matter in
the head of the comet backwards forming the tail, that
is the reason the tail of a comet always points away
from the Sun.
Comets are classified as either
Short period comets, or Long period comets.
Short Period Comets
The short period comets have less elliptical orbits
taking up to 200 years to complete their orbit around
the Sun. Halley's Comet, the most famous short period
comet takes 76 years to orbit the Sun. At it's furthest
from the Sun it reaches the orbit of Pluto - 35 AU from
the Sun.
Short period comets are believed to originate
in the Kuiper Belt, a belt of icy rubble, which starts
around the orbit of Neptune and extends out to 50 AU. It
is believed that Pluto, and Charon originated in the
Kuiper Belt.
Long
Period Comets
Long period comets take over
200 years to orbit the Sun, many of them having such
highly elliptical orbits that they take hundreds of
years to complete one solar revolution. One of the best
was Comet Bennett that last visited our Sun in 1970, and
is due to return in the year 3648. It’s aphelion or the
farthest point of it’s orbit is 282 AU from the Sun.
Long period comets are believed to originate in the
outer regions of the Solar System, in a region known as
the Oort cloud. It is thought that the gravity from
passing objects pulls the comets from the cloud sending
them on orbits towards the Sun.
Information
obtained from the Wikipedia web site. Wikipedia the free
encyclopedia.
The first video is not in English,
but it is very good, and shows some excellent examples
of comets.