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Nicmos Peers Into Heart of Dying Star
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Nicmos Peers Into Heart of Dying Star

February 8, 2005
The Egg Nebula, also known as CRL 2688, is shown on the left as it appears in visible light with the Hubble Space Telescope's Wide Field and Planetary Camera 2 (WFPC2) and on the right as it appears in infrared light with Hubble's Near Infrared Camera and Multi-Object Spectrometer (NICMOS). Since infrared light is invisible to humans, the NICMOS image has been assigned colors to distinguish different wavelengths: blue corresponds to starlight reflected by dust particles, and red corresponds to heat radiation emitted by hot molecular hydrogen.

Objects like the Egg Nebula are helping astronomers understand how stars like our Sun expel carbon and nitrogen — elements crucial for life — into space. Studies on the Egg Nebula show that these dying stars eject matter at high speeds along a preferred axis and may even have multiple jet-like outflows. The signature of the collision between this fast-moving material and the slower outflowing shells is the glow of hydrogen molecules captured in the NICMOS image.

The distance between the tip of each jet is approximately 200 times the diameter of our solar system (out to Pluto's orbit).


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