Evaporation of a sessile droplet is studied in a parabolic flight campaign. The setup elements are similar to some past or planned microgravity experiments in space: pure refrigerant Hydrofluoroether (HFE)-7100 for the liquid, droplet pinning at a 2 mm radius microgroove, nearly normal conditions. The droplet is injected onto a flat substrate through a small central outlet up to a volume between L and L (contact angles from to 70°) at the beginning of each ‘parabola’ (microgravity period lasting up to 20 s). Although an unfortunate ‘parasitic post-injection’ (persisting after the pump is off, a quite typical anomaly in microgravity) might have interfered with evaporation-rate measurements, such gaps are bridged using digital holographic vapor interferometry and axisymmetric simulations. Thus, we find that evaporation rates are significantly affected by residual gravity fluctuations in the plane (‘g-jitter’, g here). Quite accordingly, vapor clouds ‘dancing’ following the g-jitter are interferometrically disclosed, in good agreement with simulations. All this provides a noteworthy example of a possible difference between parabolic-flight experiments and those at other platforms (such as sounding rockets) approaching 0 g more precisely. The simulations reveal an independence with respect to high-frequency g-jitter sampling but highlight that each parabola is unique, with its own g-jitter signature. A detailed benchmark analysis is carried out motivated by the question of why the evaporation rates are appreciably higher for periods of negative (upward) g-jitter compared to positive (downward) ones. This is partly related to thermal Marangoni convection, concurrent or not to g-jitter buoyancy convection.
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