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Hubble Space telescope (HST) images of merging galaxy system VV29 reveal the0.3 Mpc baryonic-dark-matter (BDM) halo composed of primordialprotoglobularstarcluster (PGC) clumps of planets. Star-cluster-wakes trace themerger by formation of stars from the planets. Aligned young globular starclusters (YGCs), star-wakes and dust-trails show the frictional, spiral passageof galaxy fragments VV29cdef in a long tail-like galaxy (VV29b) as thefragments merge on the accretion disk plane of the central spiral galaxy VV29a.The observations confirm the hydro-gravitational-dynamics (HGD) prediction ofGibson 1996 and quasar microlensing inference of Schild 1996 that the darkmatter of galaxies is dominated by planets (PFPs) in million-solar-mass clumps.Globular star clusters (YGCs, OGCs, PGCs) preserve the density of the plasmaepoch 30,000 years after the big bang when viscous supercluster-fragmentationbegan. Tadpole images show linear galaxy clusters reflecting turbulent vortexlines of protogalaxy fragmentation at the 0.003 Mpc Kolmogorov-Nomura scale ofthe plasma before transition to gas. The halo size indicates strong diffusionof PGC primordial-planet-clumps from a cooling protogalaxy as its planetsfreeze.

Hydro-Gravitational-Dynamics Interpretation of the Tadpole VV29 Merging Galaxy System: Dark-Matter-Halo-Planet Star-Cluster Wakes