Unveiling The Veiled Volume
Veil nebula supernova remnant as an animated GIF

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My animated photo of a supernova remnant shows that it’s actually a three-dimensional volume floating in three-dimensional space. This artwork is not just guesswork, it’s based on scientific data about the structure of emission nebulae and real distance information

Veil Nebula by JiiPee Metsavainio

My original photo of Veil nebula SNR



We all are children of supernovae sinceall of the heavier elements are born in exploding stars. Veil Nebula is locatedin the constellation Cygnus at a distance of about 1500 light-years. It spans aboutthree degrees of sky, (Moon has an angular diameter of 0,5 degrees at the sky) realdiameter is around 70 light-years. I collect data for the photo between 2012-202 and I made this 3D model in 2021,exposure time is 45 hours.

How the 3D model is made

My Moleskine notebook pages fom 2008 shows plans how to turn nebulae to 3d model.

For as long as I have captured images of celestial objects, I have always seen them three-dimensionally in my head. The scientific information makes my inner visions much more accurate, and the 3-D technique I have developed enables me to share those beautiful visions with others.

How accurate my 3-D-visions are depending on how much information I have and how well I implement it.

The final 3-D-image is always an appraised simulation of reality based on known scientific facts, deduction, and some artistic creativity.

After I have collected all the necessary scientific information about my target, I start my 3-D conversion from stars. Usually, there is a recognizable star cluster that is responsible for ionizing the nebula. We don’t need to know its absolute location since we know its relative location. Stars ionizing the nebula have to be very close to the nebula structure itself. I usually divide up the rest of the stars by their apparent brightness, which can then be used as an indicator of their distances, brighter being closer. If true star distances are available, I use them, but most of the time my rule of thumb is sufficient. By using a scientific estimate of the distance of the Milky Way object, I can locate the correct number of stars in front of it and behind it.

Emission nebulae are not lit up directly by starlight; they are usually way too large for that. Rather, stellar radiation ionizes elements within the gas cloud and the nebula itself is glowing light, the principle is very much the same as in fluorescent tubes. The thickness of the nebula can be estimated from its brightness since the whole volume of gas is glowing, brighter means thicker.

By this means, forms of the nebula can be turned into a real 3-D shape. Nebulae are also more or less transparent, so we can see both sides of it at the same time, and this makes model-making a little easier since not much is hidden.

The local stellar wind, from the star cluster inside the nebula, shapes the nebula by blowing away the gas around the star cluster. The stellar wind usually forms a kind of cavity in the nebulosity. The same stellar wind also initiates the further collapse of the gas cloud and the birth of the second generation of stars in the nebula. The collapsing gas can resist the stellar wind and produces pillar-like formations that must point to a cluster.

Ionized oxygen (O-III) glows with a bluish light, and since oxygen needs a lot of energy to ionize it, this can only be achieved relatively close to the star cluster in the nebula. I use this information to position the O-III area (the bluish glow) at the correct distance relative to the heart of the nebula.

Many other small indicators can be found by carefully studying the image itself. For example, if there is a dark nebula in the image, it must be located in front of the emission one, otherwise, we couldn’t see it at all.

Using the known data in this way I build a kind of skeleton model of the nebula. Then the artistic part is mixed with the scientific and logical elements, and after that, the rest is very much like creating a sculpture on a cosmic scale.

The 3D model without textures