PELICAN
NEBULA
A luminous wall of hydrogen, oxygen, and dark dust shaped by newborn stars nearly 2,000 light-years away in the rich Milky Way fields of Cygnus.
The Pelican Nebula, cataloged as IC 5070, is a broad H II region in Cygnus and part of the same enormous star-forming complex as the neighboring North America Nebula, NGC 7000. The two familiar shapes are not separate clouds in space: dark foreground dust divides one luminous region into the outlines we recognize from Earth.
Ultraviolet radiation from young, massive stars strips electrons from the surrounding hydrogen. When the electrons recombine with the atoms, the cloud glows. Stellar radiation and winds simultaneously erode the denser material, cutting bright ionization fronts, long ridges, and black pillars through the nebula.
The bright ridge forming the Pelican’s “neck” is often identified with IC 5067. It contains dense knots, embedded young stars, and Herbig–Haro objects—jets launched by stars that are still forming. One of the best known, HH 555, emerges from the tip of a dusty pillar and is visibly bent by the energetic flow around it.
This photograph is a narrowband map rather than a natural-color view. Hydrogen-alpha emission carries much of the warm red and gold structure, while doubly ionized oxygen is translated into cool cyan and blue. Separating those wavelengths reveals the collision between luminous gas and the dark molecular clouds where the next generation of stars is taking shape.
The Pelican Nebula does not have an ancient story of its own. It is far too faint for the unaided eye, and its birdlike profile only became apparent through long-exposure photography. The name is a modern act of celestial pattern-making: a dark beak, bright neck, and folded body traced across a glowing cloud.
Its surrounding constellation, Cygnus, carries much older stories. Greek traditions imagined a swan flying along the Milky Way, although different writers connected that swan with different myths. The same stars also form the Northern Cross, with brilliant Deneb marking one end of the figure.
That bright region of sky also matters in Polynesian wayfinding. Hōkūleʻa star-line materials identify Deneb as Piraʻetea / Hawaiki, while noting that Piraʻetea is a Society Islands name and that no older Hawaiian name is recorded. With Keoe (Vega) and Humu (Altair), it forms a bright navigator’s triangle used to hold direction across the night.
The Pelican therefore sits inside several overlapping ways of reading the heavens: a modern photographic silhouette, the swan and cross of Western sky lore, and a field of bright stars used to navigate the Pacific.
Press Play to follow Deneb to Pelican Nebula. The guide identifies the constellation, traces the landmarks, then finishes with a precise bullseye.
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Chart notes & credits
This is a landmark chart, with north up and east left at its centre, rather than a live view for a particular date or horizon. Dashed lines connect catalogue landmarks; they are directions to sweep, not exact extensions of stellar pointer lines. Distances and directions are calculated from catalogue coordinates. Bullseyes mark reference positions, not objects’ size or visible brightness. The sky’s orientation changes as it moves. Star symbols are enlarged for clarity. Stars: ESA Hipparcos catalogue. Constellation lines: Stellarium Modern skyculture, adapted under CC BY-SA 4.0. Deep-sky reference positions: OpenNGC; individual source links below where applicable. Reference 1.
Select Play to begin. Tap the sky to pause or resume. Four step buttons revisit each landmark. The guide finishes with a stationary bullseye. Replay starts again. Reduced-motion preferences keep the waiting globe still.