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COMPOSITION:
      The composition of Pluto is not completely known. Instead, scientists use the density, radius, and information about the rotation of Pluto and Charon to hypothesize the internal structure of Pluto and Charon. Scientists have made many models of the composition of Pluto. Two models are based on the fact that there is a high cosmochemical abundance of water ice and silicates on Pluto.

Model 1 (from McKinnon in 1995) This model is a low-density model of Pluto. This shows that around half of Pluto is made up of water and ice.
Model 2 (also from McKinnon in 1995) This model is the organic-rich model of Pluto. This shows that, instead of ice, Pluto is made up of organics.

      Both these models would support the idea that Charon was formed as a result of an impact on Pluto. If Charon did form as a result of an impact on Pluto, Pluto's interior would be very hot. This would lead the softening of ice and separation of rock from the core.
      Both models are not accurate; they are only guesses. Until a more definite radius can be measured, Pluto's exact composition will be hard to tell. Scientists do believe that Pluto has a higher rock-to-ice ratio that first believed. This could be the result of loss of water early in its history, perhaps when a major collision occurred and caused the formation of Charon (which would explain why Charon is more icy that rocky.)

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BRIEF HISTORY:
       An American astronomer named Percival Lowell first documented the idea of a distant ninth planet in 1905. Based on erroneous calculations (although, Lowell did not know they were incorrect at the time), Lowell predicted a planet beyond Neptune that was affecting the movements of Neptune and Uranus. He proceeded to continue his search for his mysterious planet, going so far as predicting a possible area the planet could be found. However, it wasn't until the year 1930 that the planet was finally discovered by Clyde W. Tombaugh. In honor of Lowell, who had passed away in 1916 without fulfilling his dream, Tombaugh named the planet after the Roman god of the dead. However, this planet's mass was too small to be the one causing the discrepancies. The search for Planet X continued until Voyager 2 determined a new, correct mass for Neptune. Using the new mass of Neptune, there was no longer a discrepancy in calculations. In 1978, James Christy, an astronomer at the U.S. Naval Observatory in Flagstaff, Arizona, discovered a moon for Pluto. Named Charon, the moon had a diameter of only 740 miles(1,190 kilometers).

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SOMETHING COOL:
       Pluto's orbit takes it 249 years to complete and has a 3:2 resonance with Neptune. This means its orbital period is 1.5 times longer than Neptune's is. Usually, its orbit puts it as the farthest planet from the Sun. However, for 20 years of its trip around the Sun, its orbit takes it inside Neptune's orbit. For these 20 years, Pluto is the eighth planet from the Sun. The most recent orbit crossing took place on January 21, 1979 when Pluto came inside Neptune's orbit. They switched back on February 11, 1999. This will not occur again until September 2226. Pluto and Neptune never collide as their orbits cross because as Pluto reaches perihelion, the closest it ever comes to the Sun, it is at its maximum degree of inclination. When the two planets pass by each other, Pluto is usually well below or above the plane Neptune's orbit is on. The closest the planets come together is approximately 18 A.U.

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NOTE:
      You may have noticed the shortage of images of Pluto on this page.  That is because humans have not yet reached Pluto for an up close and personal look.  The best images we have so far are from the Hubble Space Telescope and other satellites that have visited some of the other outer planets.  This will all change soon.  NASA has begun planning a mission to Pluto called the Pluto-Kuiper Express.  To learn more about this mission, click here!

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General Information
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Fact Sheet

Charon

Discovering Pluto

Clyde Tombaugh

      Pluto-Kuiper
        Express:

     Intro
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Sources for Pluto
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