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On May 30th, 2017 at about 21h 09m 17s UTC a green bright fireball crossedthe sky of north-eastern Italy. The fireball path was observed from someall-sky cameras starting from a mean altitude of $81.1 \pm 0.2$ km (Lat.$44.369^{\circ} \pm 0.002^{\circ}$ N; Long. $11.859^{\circ} \pm 0.002^{\circ}$E) and extinct at $23.3 \pm 0.2$ km (Lat. $45.246^{\circ} \pm 0.002^{\circ}$ N;Long. $12.046^{\circ} \pm 0.002^{\circ}$ E), between the Italian cities ofVenice and Padua. In this paper, on the basis of simple physical models, wewill compute the atmospheric trajectory, analize the meteoroid atmosphericdynamics, the dark flight phase (with the strewn field) and compute the bestheliocentric orbit of the progenitor body. Search for meteorites on the groundhas not produced any results so far.

A Case Study of the May 30th, 2017 Italian Fireball