DWB 111, Simeis 57, Propeller Nebula
Cygnus (RA 20h 16.0m / Dec +43° 40′)
~15′ × 15′ (The main propeller structure)
Extremely faint (Requires long narrow-band exposure)
1950s (Simeis survey) / 1969 (DWB Catalog)
Emission Nebula / H II Region
~3,000 Light Years
~13 Light Years across
Unknown OB stars within the Cygnus X complex
Visual Appearance & Pareidolia: True to its colloquial name, DWB 111 displays a striking resemblance to a two-bladed propeller in motion. This structure is defined by two sweeping, intersecting arms of glowing Hydrogen-alpha gas that arc through the surrounding dark dust. The S-shaped symmetry makes it a highly recognizable, yet deeply mysterious, target among the many tangled filaments of Cygnus.
The Cygnus X Complex: The Propeller Nebula is just a small fragment of a much grander stage known as Cygnus X. This massive, sprawling region of the Milky Way is one of the most active star-forming areas in our local galactic neighborhood, containing dozens of distinct nebulae, powerful OB associations, and tens of thousands of solar masses of cold molecular gas. DWB 111 sits within this crowded, energetic environment, constantly bombarded by stellar winds.
A Mystery of Ionization: Unlike famous nebulae such as the Orion Nebula or the Rosette Nebula, the exact stars responsible for lighting up the Propeller Nebula remain somewhat ambiguous. Because it lies within the incredibly dense and opaque regions of Cygnus X, the hot, massive stars powering it are likely obscured by thick layers of foreground dust, requiring radio and infrared observations to trace the true power sources hidden behind the veil.
History of Discovery: The nebula was largely missed by early visual astronomers due to its low surface brightness. It was first cataloged during the Simeis Observatory survey in the 1950s as Simeis 57. However, its most common scientific designation, DWB 111, comes from a comprehensive 1969 radio and optical survey of the Cygnus X region conducted by astronomers H.R. Dickel, H. Wendker, and J.H. Bieritz (hence "DWB").
Astrophotography Guide: For amateur astrophotographers, DWB 111 is an excellent summer and autumn target. While it glows brightly in Hydrogen-alpha (making up the red "blades" of the propeller), capturing the surrounding Oxygen-III and Sulfur-II signals requires significant integration time from dark locations. Processed in the Hubble Palette (SHO), the propeller bursts with fiery tones against a beautifully complex, mottled background of deep blues and golds, showcasing the chaotic nature of the Cygnus X region.
Interactive Scaling Explanation: This panel acts as a dynamic comparator of angular sizes in the night sky. All selected objects are rendered exactly over each other from a common center, allowing an immediate, direct comparison. The Full Moon (diameter 31') serves as a permanent baseline reference.
The Photon Arrives: Right now, the light captured in this photograph is ending its roughly 3,000-year journey through deep space, hitting your camera's digital sensor. Move the slider back in time to see what humanity was doing while these precise photons were rushing through the void.
Dynamic Linear Scaling & Manipulation: This view builds an interactive, deep-space linear cosmic coordinate system. When swapping objects, the line auto-calculates its limit. Leave only near targets (Pleiades, Orion) checked to reveal detailed stellar gaps inside our galactic neighborhood. Turn on remote galaxies (Andromeda, Whirlpool) to watch the Milky Way bundle together on the left margin. Use your mouse wheel to zoom in/out and drag to pan across space to explore cluttered zones!