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After finding more planets than expected at the shortest period, there hasbeen an effort to explain their numbers by weak tidal friction. However, wefind that the strength of tidal dissipation that would produce the occurencedistribution found from Kepler planet candidates is different for giant versusmedium radii planets. This discrepancy can be resolved if there is a "flow" ofthe largest planets regularly arriving such that they go through a "hotJupiter" stage. We also show a correlation of higher stellar Fe/H with highereccentricity of giant planets that may be from smaller planets having been sentinto the star by the migration of the larger planet. This disruption of theorbits of medium and smaller planets could account for the lower occurrence of"hot Neptune" medium radius planets.

Flow of Planets Raises Short Period Fall Off