The Blue Planetary Nebula, a planetary nebula in Centaurus

 
The Blue Planetary Nebula, a planetary nebula in Centaurus

Image Credit: ESA/Hubble and NASA

The Blue Planetary Nebula (NGC 3918) is a bright planetary nebula of some 0.3 light-year across that lies about 4,900 light-years from Earth in the constellation of Centaurus. It is approaching us at roughly 17 kilometers per second, while the nebulosity is expanding at around 24 kilometers per second.

Despite their name, planetary nebulae have nothing to do with planets. The name of planetary nebulae arose because of the visual similarity between some round planetary nebulae and the planets Uranus and Neptune when viewed through early telescopes.

When a star with a mass up to eight times that of the Sun runs out of fuel at the end of its life, it blows off its outer shells and begins to lose mass. This allows the hot, inner core of the star (collapsing from a red giant to a white dwarf) to radiate strongly, causing this outward-moving cocoon of gas to glow brightly.

Over the next several thousand years, the Blue Planetary Nebula will gradually disperse into space. In the meantime the red giant has become a white dwarf which will cool and fade away for billions of years. Our own Sun is expected to undergo a similar fate, but fortunately this will not occur until some 5 billion years from now.

In the center of the Blue Planetary Nebula, and completely dwarfed by it, lies a white dwarf star called HD 102854, the dying remnants of a red giant. The intense ultraviolet radiation from this tiny remnant star causes the surrounding gas to glow.

The distinctive eye-like shape of this cloud of colorful gas, with a bright inner shell of gas and a more diffuse outer shell that extends far from the nebula looks as if it could be the result of two separate ejections of gas. But this is in fact not the case: studies of the object suggest that they were formed at the same time, but are being blown from the central star at different speeds. The powerful jets of gas emerging from the ends of the large structure are estimated to be shooting away from the star at speeds of up to 350,000 kilometers per hour.

This nebula is easily visible through small telescopes, but the central star remains invisible to optical observers.

The image is a composite of visible and near-infrared photos taken with the Wide Field Planetary Camera 2 onboard the Hubble Space Telescope using four different color filters.

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