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Surface, Page 2: Composition, Brief
History, Something Cool, Note
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.
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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.
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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.
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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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