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Comets

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Title: Comets


1
Comets
  • By Marie Allen

2
What is a Comet?
  • Comets are small, fragile, irregularly-shaped
    nuclei, sometimes surrounded by a coma and
    followed by a tail.
  • Comets tend to have highly elliptical and
    eccentric orbits that take them both very close
    to the Sun and very far away, sometimes even past
    Pluto.

3
What is a Comet?
  • Comets are composed of the original materials
    that condensed to form the Sun and planets that
    make up our solar system.
  • Many astronomers believe that collisions between
    comets and the Earth are responsible for the
    formation of our oceans.

4
A Comets Nucleus
  • The nucleus is made of ice and dust and is
    blacker than coal. Its black crust absorbs heat
    from the Sun, eventually leading to the creation
    of a coma.
  • When a comet is far from the Sun, its nucleus is
    frozen solid and can only be seen by reflected
    sunlight.

5
The Coma
  • The coma is a cloud of gases and small particles
    that have broken off of the nucleus. Its size
    and brightness increase as the comet gets closer
    to the sun.
  • The coma reflects sunlight, causing the comet to
    fluoresce and become more visible.

6
The Coma
  • As a comet approaches the Sun, the nucleus warms
    causing ices beneath the surface to turn to gases
    and expand. When this occurs, portions of the
    surface bulge and eventually burst under the
    pressure, shooting gas and small particles
    outward. This expulsion is known as a jet.

7
The Tail
  • A comets tail is a result of the Suns radiation
    and pressure and the solar wind. Gases and dust
    particles that have been expelled from the
    nucleus are accelerated at certain rates,
    depending on their size, away from the comets
    head. These differing accelerations may
    sometimes cause the appearance of multiple tails.
    Relatively massive dust tails accelerate more
    slowly, causing them to curve, while the ion
    tail, made up of gases, is accelerated more
    quickly, causing it to be straighter.

8
Halleys Comet
  • Halleys Comet has been observed since at least
    240 B.C., maybe even as early as 1059 B.C.
  • This comet appeared in the sky in 1066, the night
    before the Battle of Hastings, and is depicted on
    the Tapestrie de Bayeux.
  • Edmund Halley, in 1705, predicted its orbital
    period to be about 76 years.

9
Halleys Comet
  • Perihelion distance .587 au
  • Dimensions 16x8x8 km
  • In 1984 and 1985, 5 spacecrafts from Russia,
    Japan, and Europe were launched to observe the
    characteristics of this comet only 4 other
    comets had been studied in this way in the past.
  • These ventures told us, among other things, that
    the comets nucleus has a density of 0.1 grams
    per cubic centimeter. Therefore, the nucleus is
    obviously porous.
  • Halleys next perihelion passage is predicted to
    occur in 2061.

10
Hale-Bopp Comet
  • Discovered by two different astronomers, one
    professional (Alan Hale) in New Mexico and one
    amateur (Thomas Bopp) in Arizona, in July 1995.
  • It is a very large comet, having a diameter of
    30-40 km.

11
Hale-Bopp Comet
  • The Hale-Bopp Comet holds the record for
    remaining visible with the naked eye for the
    longest period of time 19 months.
  • It is estimated that around 81 of Americans have
    seen this comet.
  • The Hale-Bopp Comet has received much attention
    in the media, mostly due to the Heavens Gate
    cult. Thirty-seven members of this cult took
    their own lives, all at the same time, believing
    that there wasa kind of UFO behind the Hale-Bopp
    Comet that would take them to paradise.

12
Conclusion
  • Comets are beautiful to look at and have been
    perceived for centuries as everything from bad
    omens to one-way tickets to Heaven.
  • They have been observed extensively and have
    provided much information about the beginnings of
    the universe.

13
Sources
  • http//cometography.com/educate/comintro.html
  • http//csep10.phys.utk.edu/astr161/lect/comets/hal
    ley.html
  • http//www.psi.ed/hbinfo.html
  • http//seds.lpl.arizona.edu/nineplanets/nineplanet
    s/halley.html
  • http//www.sipe.com/halebopp/preface_current.htm
  • http//www.solarviews.com/eng/comet.htm
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