The North America Nebula NGC 7000
Telescope SVbony SV550 122/854mm, SW 150PDS 150/810mm, TS 102/571mm
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 May, Jun, Jul, Aug 2026
Acquisition Details - Wide View

I photographed this enormous emission complex using my three telescopes, each of which was equipped with a different type of filter—the refractors were fitted with dual-band Ha+O3 and S2+O3 filters, while the 150PDS Newtonian telescope was fitted with an Antlia RGB Triband filter. I then used the stars from that telescope in the final photograph. The North America Nebula is very extensive, and to capture it in its entirety, I had to divide the entire composition into 4 images using these telescopes and then stitch them together in post-processing. However, using this method, I managed to photograph not only the most famous part, the so-called Cygnus Wall, but also the remaining parts of this interesting nebula.

NGC 7000

The North America Nebula (NGC 7000) is a sprawling, iconic emission nebula located in the constellation Cygnus. Thanks to a remarkable cosmic coincidence, the glowing ionized gas is divided by a thick, dark lane of interstellar dust, creating a shape that beautifully mimics the continent of North America, complete with a prominent and unmistakable "Gulf of Mexico."

Key Astrophysical Data

Catalog Designations

NGC 7000, Caldwell 20, Sharpless 117 (Sh2-117)

Position in the Sky

Cygnus (RA 20h 59m 17s / Dec +44° 31′ 44″)

Apparent Size

120′ × 100′ (Roughly 4 times the Full Moon)

Apparent Magnitude

+4.0 mag (Visible to naked eye in dark skies)

Discovery Date

October 24, 1786 (by William Herschel)

Object Type

Emission Nebula / H II Region

Distance from Earth

~2,590 Light Years

Physical Size

~100 Light Years across

Power Source

J205551.3+435225 (Massive obscured O-type star)

Object Overview & Facts

The Continental Shape: The striking resemblance to North America is entirely an optical illusion created by the interplay of light and dark. The "continent" is a vast cloud of ionized hydrogen gas emitting a bright red glow. The "Gulf of Mexico," "Florida," and the "Atlantic Ocean" are not empty space; they are formed by a dense, opaque cloud of cold interstellar dust (cataloged as LDN 935) sitting right in front of the glowing gas, physically blocking the light from reaching Earth.

The Hidden Engine: For decades, the energy source illuminating this massive 100-light-year-wide cloud was a mystery. Astronomers initially suspected Deneb, the brightest star in Cygnus, but Deneb is an A-type supergiant and not hot enough to ionize so much hydrogen. In 2005, infrared telescopes finally pierced the dark dust of the "Gulf of Mexico" and found the true culprit: a massive, blistering hot O-type star (J205551.3+435225, sometimes referred to as the Bajamar star). This star is completely invisible to optical telescopes due to the thick soot blocking it.

The Pelican Connection: NGC 7000 is not an isolated object. It is physically part of the exact same massive H II region as its famous neighbor, the Pelican Nebula (IC 5070). The only thing separating the "Pelican" from "North America" from our perspective on Earth is the dark molecular dust lane of LDN 935 slicing right between them.

The Cygnus Wall: The most active and detailed region of the nebula is the "Mexico and Central America" portion, famously known as the Cygnus Wall. This is a violent star-forming shock front where ultraviolet radiation is aggressively eating into the cold dust. Here, astronomers have cataloged numerous young stellar objects (YSOs) and Herbig-Haro objects—jets of gas being blasted out by newly born, embryonic stars still wrapped in their dusty cocoons.

History of Discovery: The brilliant astronomer William Herschel originally discovered the nebula in 1786. However, because of its enormous size, its surface brightness is highly spread out, making the full continental shape very difficult to see through early telescopes. The iconic shape and its famous moniker were only widely recognized after the pioneer of astrophotography, Max Wolf, captured it on photographic plates in 1890.

Astrophotography Guide: NGC 7000 is arguably one of the most famous and rewarding targets for astrophotographers. Due to its massive size (spanning over 2 degrees of the sky), capturing the entire continent requires a wide-field instrument (around 200mm to 400mm focal length on an APS-C sensor). It responds incredibly well to both HOO and Hubble Palette (SHO) imaging. Imagers using longer focal lengths (700mm+) frequently target just the "Cygnus Wall" segment to resolve the incredibly intricate, towering pillars of dust and gas located there.

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: NGC 7000 vs. Earth's History

Present Day Photon Departs (2,590 ly)
Year 2026 AD

The Photon Arrives: Right now, the light captured in this photograph is ending its roughly 2,590-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!