The dark nebula that forms the Fish’s Mouth extends across the full span of M42, segregating a small branch to the north that Charles Messier cataloged separately as M43. In reality, both are one and the same physical cloud. Through most binoculars, M43 is a roundish cloud surrounding the 8th-magnitude star SAO 132328. It turns asymmetrical through giant binoculars, looking like a comma that hooks toward the north, pointing the way to our final targets this month.
The northern end of the sword, marked by the wide stellar pair 42 and 45 Orionis, is also engulfed in interstellar dust clouds visible only by reflected starlight. Although the nebula carries three separate entries in the New General Catalogue — NGC 1973, NGC 1975, and NGC 1977 — it’s actually the same complex. Of these, only NGC 1977, the portion just south of 42 and 45 Orionis, is visible through binoculars, and then only with difficulty.
While many people marvel at M42 and M43 and then move on, there is a sparsely populated open cluster to their north that few seem to know even exists. NGC 1981 lies just north of the sword, and it is readily visible through 7x binoculars. You will likely count eight or nine stars within its boundaries, with the three brightest set in a gentle north-south arc.