The Pacman’s Dark Ghosts

Sun Oct 11 2026

NGC 281, also catalogued as IC 11 and Sh2-184, is the Pacman Nebula, an emission nebula and star-forming region in Cassiopeia that sits in the Perseus Arm of the Milky Way. Distance estimates range from roughly 9,200 to 10,000 light-years, depending on the method. The young open cluster IC 1590 lights it up, and its brightest member, HD 5005, is a multiple star whose primary is a hot, luminous O-type star. The dark knots near the center are Bok globules, dense clumps of gas and dust named after astronomer Bart Bok, who proposed them in the 1940s. Some of them may eventually collapse into new stars; others may simply evaporate. The locator and close-ups below show the globules, the bright rims along the nebula’s edge, and the dust lane that forms the Pacman’s mouth. 📷 NGC281_locator.png 📷 NGC281_closeup_1.png 📷 NGC281_closeup_2.png 📷 NGC281_closeup_3.png 📷 NGC281_closeup_4.png

About this object

Type
Star Cluster with Nebulosity
Constellation
Cassiopeia (the Queen)
Apparent size
6.3′
Catalogue designations
IC 1590

IC 1590 is a star cluster with nebulosity in the constellation Cassiopeia (the Queen). It spans roughly 6.3′ on the sky.

Acquisition

Equipment

Astrophotography by David Joyce, AstroDavido.