Celestial hemisphere:  Northern  ·  Constellation: Cassiopeia (Cas)  ·  Contains:  Bubble nebula  ·  NGC 7635  ·  Sh2-162
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NGC 7635 Bubble Nebula #5 - HOO, Molly Wakeling
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NGC 7635 Bubble Nebula #5 - HOO

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Description

This image was taken in three different wavelengths that are emitted by three different energy transitions of elements in space: hydrogen alpha (Ha, or HII), oxygen-III (OIII), and sulfur-II (SII).

This image is a popular combination known as HOO. It's a natural-ish color combination, where Ha is red and OIII is both green and blue. It's natural-ish because Ha light is really in the deep red, and OIII is a blue-green color. SII is very close in wavelength to Ha, so you don't really miss it in this kind of color combo (especially for an object like this one that doesn't have a whole lot of SII to begin with).

The Bubble Nebula is a beautiful and fascinating object. It lies within a region of hydrogen gas up in the constellation Cassiopeia. The bubble itself is shaped by the stellar wind (ejected charged particles) from a hot, young, massive star in the center, which is thought to be 44 times more massive than our own Sun. The bubble is 10 lightyears across, which is relatively small as far as nebulae go, and lies about 11,000 lightyears away from us.
The rings around the bright star to the lower right of the bubble are an optical effect of the imaging system because of the star's brightness. They were a lot more prominent in the SII and OIII channels, but largely I think because the nebula signal at those wavelengths was much weaker.

Data from Brian Sheets.

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NGC 7635 Bubble Nebula #5 - HOO, Molly Wakeling