Ou4 and Sh2-129 The Giant Squid and Flying Bat
Telescope SVbony SV550 122/854mm, SW 150PDS 150/810mm
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 18+18+15 Hours
Date Sep, Oct 2025
Acquisition Details

The Giant Squid is notoriously one of the faintest objects ever attempted by amateur astrophotographers. Photographing this interesting yet extremely challenging subject—especially in areas with light pollution—requires a great deal of effort, long exposure times, and a solid mastery of technique. The post-processing and image processing involved are also among the most demanding I have encountered to date. The photograph is composed of a mosaic of two fields, and even so, I was only able to fit the entire Ou4 Nebula—The Giant Squid Nebula—into the final image, which was, however, my primary goal.

Ou4 & Sh2-129

The Giant Squid Nebula (Ou4) and the Flying Bat Nebula (Sh2-129) form one of the most striking, yet difficult-to-capture pairings in the entire night sky. Located in the constellation Cepheus, the vast, glowing red emission of the Bat surrounds an incredibly faint, ethereal blue-green bipolar outflow known as the Squid. Together, they create a colossal cosmic tapestry spanning an area equivalent to five full moons.

Key Astrophysical Data

Catalog Designations

Ou4 (Giant Squid), Sh2-129 (Flying Bat)

Position in the Sky

Cepheus (RA 21h 11.8m / Dec +59° 59′)

Apparent Size

150′ × 150′ (Absolutely massive widefield area)

Apparent Magnitude

Extremely faint (Ou4 requires extreme exposure)

Discovery Date

1950s (Sh2-129) / 2011 (Ou4 by N. Outters)

Object Type

H II Emission Region & Bipolar Outflow

Distance from Earth

~2,300 Light Years

Physical Size

Ou4 spans ~50 Light Years across

Power Source

HR 8119 (Triple star system)

Object Overview & Facts

A Recent, Incredible Discovery: While the red emission nebula Sh2-129 (The Flying Bat) has been cataloged since the 1950s by Stewart Sharpless, its hidden companion remained completely invisible to science for decades. It wasn't until June 2011 that French amateur astrophotographer Nicolas Outters, while shooting an extremely deep exposure of the region through a narrow Oxygen-III filter, noticed a faint, bizarre shape. This led to the discovery of Ou4, now famously known as the Giant Squid Nebula.

The Bipolar Outflow (Ou4): The Giant Squid is not a standard emission nebula. It is a massive bipolar outflow—a colossal pair of jets composed primarily of doubly ionized oxygen (OIII). The jets are being blasted outward in opposite directions at immense speeds. The true nature of Ou4 was initially debated; some thought it might be a planetary nebula (the death throes of a sun-like star), but modern consensus suggests it is an outflow driven by the massive, young stars at its heart.

The Engine (HR 8119): At the very center of the Squid's body lies the triple star system HR 8119. This system contains massive, hot, young stars whose fierce stellar winds and ultraviolet radiation are responsible for both ionizing the vast red hydrogen gas of the Flying Bat and propelling the blue-green jets of the Squid. The outflow from this system has carved the spectacular, elongated shape of Ou4 over hundreds of thousands of years.

Immense Scale: The physical size of this complex is staggering. Because it sits roughly 2,300 light-years from Earth, its apparent size of 2.5 degrees on the sky means the entire Flying Bat complex is over 100 light-years across. The Giant Squid alone stretches approximately 50 light-years from tip to tip, making it one of the largest bipolar outflows ever discovered in our galaxy.

Astrophotography Guide: Ou4 is widely considered an "endgame" target for deep sky astrophotographers. The Hydrogen-alpha signal of the Flying Bat is relatively straightforward to capture, but the OIII signal of the Squid is punishingly faint. Imagers must use narrow bandpasses (usually 3nm) and routinely collect 30, 40, or even 60+ hours of exposure time to properly reveal the body and tentacles of the Squid against the background space.

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: Squid & Bat vs. Earth's History

Present Day Photon Departs (2,300 ly)
Year 2026 AD

The Photon Arrives: Right now, the light captured in this photograph is ending its roughly 2,300-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!