The Origin of Life from Primordial Planets
  The origin of life and the origin of the universe are among the most
important problems of science and they might be inextricably linked.
Hydro-gravitational-dynamics (HGD) cosmology predicts hydrogen-helium gas
planets in clumps as the dark matter of galaxies, with millions of planets per
star. This unexpected prediction is supported by quasar microlensing of a
galaxy and a flood of new data from space telescopes. Supernovae from stellar
over-accretion of planets produce the chemicals (C, N, O, P etc.) and abundant
liquid water domains required for first life and the means for wide scattering
of life prototypes. The first life likely occurred promptly following the
plasma to gas transition 300,000 years after the big bang while the planets
were still warm, and interchanges of material between planets constituted
essentially a cosmological primordial soup. Images from optical, radio, and
infrared space telescopes suggest life on Earth was neither first nor
inevitable.
