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04 The Planets

LoneBear's picture
Submitted by LoneBear on Thu, 03/27/2014 - 13:51

The remnants of the white dwarf companion, shattered into pieces and distributed in a narrow conic section outwards into space, will take up orbital positions around the newly formed giant star. Unlike low-speed matter which will simply be sucked into the gravitational whirlpool of the star, the white dwarf fragments will maintain broad, slightly elliptical orbits, using the new giant sun as one of the foci, and the vanished core of the supernova as the other. The orbit is maintained because the white dwarf fragment possesses ultra-high speed motion, and like a true pulsar, will generate a motion in the same direction as the progression of the natural reference system—away from all gravitational sources. So, with gravity pulling in, and ultra-high speed motion pushing away, the planets enjoy a very stable, nearly circular orbit.

After the dust of the 2nd supernova has settled, we find a red giant star, condensing and heating up, moving towards the main sequence, surrounded by a a ring of rock, and typically 8 large fragments of the former white dwarf, in the sequence 4 small fragments, asteroid ring, 4 large fragments, and finally the rock, dust, and bits and pieces that were expelled far out from the original supernova, of both A and B component matter (low and intermediate-speed range, as not all the “heavy” matter had settled into the core when the supernova explosion occurred).

The solar system will contain two general regions of planetary formation, on opposite sides of the asteroid belt. The larger fragments, having a more ultra-high speed motion (and thus a larger “outward” or anti-gravity movement), will be further out, past the asteroid belt, and will be called the “outer planets.” The smaller fragments that exist between the sun and the asteroid belt will be designated as the “inner planets.”

In the early stages of cooling, the outward motion of the white dwarf fragments will prevent any large amount of dust and debris from accreting on their surfaces. The cooling of the fragment itself, will, however, produce hydrogen and helium gases in its core which, like its stellar counterpart, will occasionally “nova,” and expel these gases and other matter onto its surface, producing a bright, combustive flare. As cooling continues, heavier elements will be produced, as more matter drops into the low speed range, and this matter will allow meteors, dust, and debris to begin to accumulate on the surface of the fragment.