Ori I-2, a cometary globule to the north of IC 434. Hα emission (top left) traces out a ~4 pc long tail, which also exhibits lower line ratios in [S II]/Hα (bottom left) and [N II]/Hα (bottom right). Tentative kinematic differences are also seen in Hα emission tracing the tail (top right). An overdensity of B stars (cyan) is also associated with the cometary tail. Note that the vertical stripe in the [N II]/Hα at the center of the tail is a data artifact.