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Resembling a nightmarish beast rearing
its head from a crimson sea, this monstrous object is actually an innocuous
pillar of gas and dust. Called the Cone Nebula (NGC 2264) so
named because, in ground-based images, it has a conical shape
this giant pillar resides in a turbulent star-forming region.
This picture shows the upper 2.5 light-years
of the nebula, a height that equals 23 million roundtrips to the Moon.
The entire nebula is 7 light-years long. The Cone Nebula resides 2,500
light-years away in the constellation Monoceros.
Radiation from hot, young stars [located
beyond the top of the image] has slowly eroded the nebula over millions
of years. Ultraviolet light heats the edges of the dark cloud, releasing
gas into the relatively empty region of surrounding space. There, additional
ultraviolet radiation causes the hydrogen gas to glow, which produces
the red halo of light seen around the pillar. A similar process occurs
on a much smaller scale to gas surrounding a single star, forming the
bow-shaped arc seen near the upper left side of the Cone. This arc,
seen previously with the Hubble telescope, is 65 times larger than the
diameter of our solar system. The blue-white light from surrounding
stars is reflected by dust. Background stars can be seen peeking through
the evaporating tendrils of gas, while the turbulent base is pockmarked
with stars reddened by dust.
Over time, only the densest regions
of the Cone will be left. Inside these regions, stars and planets may
form.