  Hubble Space telescope (HST) images of merging galaxy system VV29 reveal the
0.3 Mpc baryonic-dark-matter (BDM) halo composed of primordial
protoglobularstarcluster (PGC) clumps of planets. Star-cluster-wakes trace the
merger by formation of stars from the planets. Aligned young globular star
clusters (YGCs), star-wakes and dust-trails show the frictional, spiral passage
of galaxy fragments VV29cdef in a long tail-like galaxy (VV29b) as the
fragments merge on the accretion disk plane of the central spiral galaxy VV29a.
The observations confirm the hydro-gravitational-dynamics (HGD) prediction of
Gibson 1996 and quasar microlensing inference of Schild 1996 that the dark
matter of galaxies is dominated by planets (PFPs) in million-solar-mass clumps.
Globular star clusters (YGCs, OGCs, PGCs) preserve the density of the plasma
epoch 30,000 years after the big bang when viscous supercluster-fragmentation
began. Tadpole images show linear galaxy clusters reflecting turbulent vortex
lines of protogalaxy fragmentation at the 0.003 Mpc Kolmogorov-Nomura scale of
the plasma before transition to gas. The halo size indicates strong diffusion
of PGC primordial-planet-clumps from a cooling protogalaxy as its planets
freeze.
