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We present a solution to the long outstanding meter barrier problem in planetformation theory. As solids spiral inward due to aerodynamic drag, they willenter disk regions that are characterized by high temperatures, densities, andpressures. High partial pressures of rock vapor can suppress solid evaporation,and promote collisions between partially molten solids, allowing rapid growth.This process should be ubiquitous in planet-forming disks, which may beevidenced by the abundant class of Systems with Tightly-packed Inner Planets(STIPs) discovered by the NASA Kepler mission.

Overcoming the Meter Barrier and The Formation of Systems with Tightly-packed Inner Planets (STIPs)