The Exploration of the Solar System
The European programme of outer solar system exploration in
the 22nd century was unprecedented in its aims, scale and duration. Over a period of fifty years, every known
object within 100 AU of the sun, with a diameter greater than 200 kilometres,
was visited, mapped, probed and explored by robotic swarms and astronauts, along
with many smaller objects of interest.
One of the most unexpected findings of the endeavour was the
discovery in CE 2161 of a significant cluster of unexplained physical anomalies
on just such a smaller object: Kerberos, one of the small, rocky moons
of Pluto. This first exploration
discovered unexpected results in the microgravitational, neutrino, magnetic
and other spectra. These appeared to be focused on a small, roughly spherical
volume with a diameter of approximately 10m, located some 250m below the
surface at one end of the moon. A volume which
followed Kerberos as it tumbled chaotically in its orbit around the dwarf
planet.
Exploring this further, and applying findings from the most cutting-edge
theories of physics available at the time, scientists proposed that the
Kerberos Multiple Anomalies (KMA) arose from the existence of an area of
‘softness’ between this quantum cosmos or Reesian ‘patch’ and another. According to theory, such areas could enable
the construction of wormholes, thus supporting interstellar travel at
translight speeds.
The military implications of such a finding were clear, and
a joint EuroAfrican (EA) crash programme was initiated to secure and develop
the KMA and the area of space surrounding it.
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