Which size is right for your space?
- Living room (above sofa): 48x32
- Bedroom (above headboard): 36x24 or 48x32
- Dining room: 36x24 or 48x32, depending on wall size
- Home office or den: 30x20 or 36x24
- Large foyer or entryway: 48x32
- Hallway, bathroom, or gallery wall: 18x12 or 24x16
When in doubt, go bigger than you think. The art, including any frame, should fill about ⅔ the width of the furniture beneath it. Sizes listed are the photograph itself; framed paper prints, with a 2" mat and frame, are about 3–5" larger in each direction.
See it on your wall before you order
Use the buttons below the image:
- Wall Preview: upload a photo of your room and see this print on your wall in your chosen size and frame.
- Live Preview AR: on your phone or tablet, point your camera at your wall and see the print there in real time.
Framed prints arrive ready to hang
Framed paper prints are matted with a 2" white mat and protected by non-glare acrylic, so the image stays clear without reflections from windows or lights. Acrylic is lighter and safer to ship than glass, and every framed print arrives with hanging hardware already attached.
MetalPrints with a float mount or frame also arrive ready to hang.
Questions about size, material, or framing? See the FAQ or email me a photo of your wall, and I'll suggest a size and finish.
About this photograph
Here, familiar shapes lie in unfamiliar locations. On the left is an emission nebula cataloged as NGC 7000, the North America Nebula, famous partly because it resembles the continent of North America. The emission region to the right of the North America Nebula is IC 5070, also known for its suggestive outlines as the Pelican Nebula. Separated by a dark cloud of obscuring dust, the two bright nebulae are about 1,500 light-years away. This spectacular cosmic portrait combines narrow-band images of the region in a false-color palette to highlight bright ionization fronts with fine details of dark, dusty forms in silhouette. Emission from atomic hydrogen, sulfur, and oxygen is captured in the narrow-band data.
The "IC 5070 Pelican Nebula" photograph reveals a stunning star-forming region, approximately 30 light-years wide. Captured from my Bortle 8 backyard in Phoenix, this image showcases the dynamic interplay of hydrogen gas emitting light, a hallmark of emission nebulae. Over five nights, I meticulously gathered 175 subframes in Hydrogen-alpha, Oxygen III, and Sulfur II, allowing the vibrant colors and intricate details to emerge.
This nebula, often likened to a pelican due to its shape, is a testament to the ever-evolving nature of the cosmos. The ionization front, driven by the light from young, energetic stars, is gradually transforming the gas clouds, ensuring that this celestial formation will look different in millions of years. The thin dark dust cloud known as L935 separates it from the nearby North America Nebula, adding depth to the scene.
NOTE:
The majority of photographs of nebulae are in a false color palette. False-color photographs of nebulae are essentially color (RGB) photographs whose color channels have been mapped to specific emission lines. In these images, each color can represent a specific element. In other words, a false-color image of a nebula tells us exactly what it’s made of. There are many emission lines, but the three most photographed by astronomers are hydrogen-alpha, oxygen-III, and sulfur-II. These emission lines are captured by using narrowband filters which only let through the light at very specific wavelengths, typically most of my photographs are taken with filters allowing a bandwidth of 3µm.
|
Element
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Emission line
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Wavelength
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Color
|
|
Hydrogen
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Hα
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656.3 nm
|
Red
|
|
Oxygen
|
O-III
|
500.7 nm
|
Blue/Green
|
|
Sulfur
|
S-II
|
672.4 nm
|
Red
|

Mapping Hα, O-III and S-II to red, green and blue is problematic when two of them are red, one is blue/green, and none is pure blue. Astronomers deal with this by using false color — one or more of these elements is going to have to take a hit for the team and take on an unnatural hue. The Hubble palette assigns red to S-II, green to Hα, and blue to O-III: red is accurate, green and blue are false. This photograph uses the Hubble color palette, hence the golds and blues you find in the photograph.