The Geology of Enod

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Two famous scientists, an astronomer and a biologist, whose mission was to discover a new solar system, discovered planet Enod. Enod is part of the Nuz planetary system formed nearly 5 billion years ago. It is 400 light years from the Earth. The second mission for this exploration was to study the geology of planet Enod. The data collected by the probes and satellites provided a promising range of information about the planet's geology. |
ENOD IS BORN
The evidence collected by
Edwin and Armando leads them to conclude that Enod and
the planets of the Nuz solar system emerged from the
dusty disk around the parent star Nuz. Enod' s formation is very
similar to that of the Earth. Enod started out as little
bits of rocks and gases found rotating around the star Nuz.
These rocks and gases collided with each other within their
orbit to form small planets called "planetesimals." Enod
continued to increase its mass as the planet used its
gravitational pull to attrack more and more objects into its
center. As the the mass increased so did its gravitational
pull. This caused the atoms to be pulled very close to each
other. As a result of such forces, the center of the planet
heated up and melted all the rocks. The heavier elements
like iron and nickel continued to sink down to the center of
the planet while the lighter ones remained near the surface.
Enod was now a spinning ball of molten rock. The planet's core slowly cooled
and solidified under the great pressure acting on it.
Eventually, the surface cooled, and Enod's crust was
created. The crust, which is mostly granite and basalt,
sculptured some of Enod's unique geological features that we
see today.

The planet Enod
originated from materials that collected in a dusty disk
around the star Nuz. This protostellar disk was formed
from gas and dust in intersteller clouds. The disk grew
as material fell in from the parent cloud. Scientist
believe that a shock was created when these cloud
materials hit the protostellar disk.

Near the shock zone
newly introduced material slowed down and redistributed
itself throughout the disk. Some material made it toward
the center and became part of the developing star. Other
dust particles in these disks clumped together to form
small rocks. Eventually, these small rocks clumped
together to form numerous small solid celestial bodies or
minature planets called "planetesimals."
Enod
Cools

Enod's Tectonic
Plates
Enod's surface broke
into seven large and small moving plates or tectonic plates
during its cooling period. These massive irregular shaped
slabs of rock are composed of both continental and oceanic
lithosphere. The plates float and move across the top of
Enod's mantle. The plates, each about 50 miles thick, move
relative to one another an average of a few inches a year.
Various types of movements form the unique features found on
planet Enod. The mountain range
found near the east coast of Acirfa was formed by the
convergence of the Edwin oceanic plate and the continental
plate Acirfa. These plates moved towards each other and
collided. The oceanic plate was then forced under the
continental plate. This is called subduction. The Enodia and Barton
plates form what is called the Mid-Bartonian Ridge through
the process known as sea-floor spreading. In this process
the plates move away from each other. Molten rock rises and
adds new material to the edges of the plates.

http://pubs.usgs.gov/publications/text/Vigil.html


Enod's crust formation gave rise
to 2 large continents known as Acirfa and Enodia. Enodia is
the largest of the two. Neighboring both continents is the
large island of Linodia. Acirfa is about the same size as
South America. Enodia is about the size of Europe and Asia
combined. Both Enodia and Acirfa lie along Enod's equator.
For the most part, Enodia and Acirfa are tropical continents
gleaming with plant and animal life. Finally, each of the
continents is surrounded by two vast oceans, Barton and
Tarta.
Contour Maps of Enod

Profile of Enod's
Continents

