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
IC 410 (also known as the Tadpole Nebula or Sh 2-365) is an emission nebula in the constellation of Auriga, and the nearby IC 405 (Flaming Star Nebula) and the open clusters M36 and M38. This nebulae complex is approximately 12,000 light-years from Earth. It is part of a larger star-forming complex.
I shot this region of Auriga over three nights, collecting over 30.9 hours of data, including about 10.3 hours each of Ha, OIII, and SII. All taken in my backyard here in Bortle 8 urban Phoenix. In the field of view you see the Flaming Star Nebula in the lower left hand corner, while the upper right area of the photograph is the Tadpole Nebula. The Tadpole Nebula derives it's name from two prominent dense structures of gas and dust (each approximately 10 light-years long) that resemble tadpoles with long tails you can see near the bottom right of the interior of the Nebula (the blue region).
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
|
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Hydrogen
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Hα
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656.3 nm
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Red
|
|
Oxygen
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O-III
|
500.7 nm
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Blue/Green
|
|
Sulfur
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S-II
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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.