The Flaming Skull Nebula.

By Phil Plait



Photo by T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOAO/AURA/NSF)
Planetary nebulae are among my favorite objects in the sky. When a star a bit more massive than the Sun starts to die, it blows off a super solar wind of gas. As it ages more, this wind it blows speeds up, slamming into the stuff previously ejected, carving it into weird and amazing shapes. Eventually, the entire outer layers of the star blow off, exposing the star’s hot, dense core. This floods the surrounding gas with ultraviolet light, causing it to glow.

Once it starts to emit light, the gas cloud becomes visible to us on Earth, and we can see the weird forms it can take. This structure can be quite fantastic, depending on how exactly the star was spinning as it blew off those winds, what angle we see this at, and the chemical composition of the gas.

In the case of the planetary nebula Sh2-68, though, we have an added factor: motion. The star at the heart of this nebula is moving rapidly through space, and it happens to be in a location in our galaxy where there is more gas and dust between stars than usual. So as it moves, the gas it blows off is itself blown back, like a dog’s hair is blown back when it sticks its head out of a car window.

The image above, taken by my friend Travis Rector using the KPNO 4-meter telescope, shows this in detail. The blue gas is oxygen (which is slightly false-color here; this flavor of oxygen is actually more greenish), and the red is hydrogen. The star itself is the blue one right in the center of the blue gas.

I could go into great detail about the overall shape of the gas, the cavities in it, the actually quite interesting physics of how the gas interacts with the interstellar gas … but c’mon. Seriously.

The nebula looks like a giant screaming head with its hair aflame streaking across the galaxy!

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http://www.slate.com/blogs/bad_astronomy/2013/06/28/planetary_nebula_sh2_68_the_flaming_skull_nebula.html