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Based on imaging and spectroscopic data, we develop a 3-D model for theHuygens Region of the Orion Nebula. Theta1OriC , the hottest star in theTrapezium, is surrounded by a wind-blown Central Bubble that opens SW into theExtended Orion Nebula. Outside of this feature lies a layer of ionized gas atabout 0.4 pc from Theta1OriC. Both of these features are moving rapidly awayfrom Theta1OriC with an expansion age for the Central Bubble of only 15,000yrs.

Deciphering the 3-D Orion Nebula-I: Expanding Shells in the Huygens Region