Clumps of hydrogenous planetoids as the dark matter of galaxies

Hydrodynamic gravitational condensation theory and quasar-microlensing observations lead to the conclusion that the baryonic mass of most galaxies is dominated by dense clumps of hydrogenous planetoids. Star microlensing collaborations fail to detect planetoids as the dominant dark matter component of the inner Galaxy halo (within ≈ 30 kpc) by an unjustified uniformnumber-density assumption that underestimates the average value. At plasma neutralization and photon decoupling, existing proto-galaxies should fragment at both proto-globular-cluster (PGC) ≈ 10M⊙ and terrestrial-mass scales ≈ 10M⊙, from Gibson’s 1996 hydro-gravitational theory. Schild’s 1996 interpretation was that the mass of the lens galaxy is dominated by “rogue planets ... likely to be the missing mass”, from measured twinkling frequencies of the lensed quasar Q0957+561 A,B images and their time-delayed difference. Schild’s findings of a 1.1 year image time delay with dominant planetoid image-twinkling-period are confirmed herein by three observatories. Subject headings: cosmology: theory, observations — dark matter — Galaxy: halo — gravitational lensing — turbulence