The Propeller Nebula DWB 111
Telescope SVbony SV550 122/854mm, SW 150PDS 150/810mm. TS 102/571mm SD-APO
Camera ZWO ASI2600MC DUO, Touptek 2600C
Filters Scorpio 3nm Dualband Ha+O3, Askar D2, Antlia RGB Triband
Mount Sky-Watcher EQ6-R Pro, Juwei-17
Exposure 20+20+15 Hours
Date Jun, Jul, Aug 2025
Acquisition Details

The Propeller Nebula is relatively faint compared to its famous Cygnus neighbors, requiring deep integration. The central part of the DWB111 nebula—the propeller itself—is a relatively brighter object composed mainly of red Hα emission, while its immediate surroundings consist primarily of S₂ and O₃ emissions, which glow in shades of blue and blue-green. The rest of the nebula’s surroundings are a mixture of both. This makes the DWB111 nebula an interesting but challenging subject for both the photography itself and the subsequent post-processing. To highlight and blend the individual parts, I again used a combination of three telescopes and filters.

DWB 111

The Propeller Nebula (DWB 111) is a fascinating, relatively faint emission nebula located in the heart of the incredibly rich Cygnus X star-forming complex. Resembling the spinning blades of an airplane or boat propeller, this glowing cloud of ionized gas sits approximately 3,000 light-years away, woven deeply into the dense molecular clouds of our Milky Way's Orion Spur.

Key Astrophysical Data

Catalog Designations

DWB 111, Simeis 57, Propeller Nebula

Position in the Sky

Cygnus (RA 20h 16.0m / Dec +43° 40′)

Apparent Size

~15′ × 15′ (The main propeller structure)

Apparent Magnitude

Extremely faint (Requires long narrow-band exposure)

Discovery Date

1950s (Simeis survey) / 1969 (DWB Catalog)

Object Type

Emission Nebula / H II Region

Distance from Earth

~3,000 Light Years

Physical Size

~13 Light Years across

Power Source

Unknown OB stars within the Cygnus X complex

Object Overview & Facts

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.

Deep Sky Objects Size Comparison Laboratory

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.

Cosmic Time Machine: DWB 111 vs. Earth's History

Present Day Photon Departs (3,000 ly)
Year 2026 AD

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.

Cosmic Scale: Distance Map Laboratory

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!