At the bottom left of this vertical image are the thickest regions of brown and rusty red gas and dust,
known as pillars. There are many layers of semi-transparent gas and dust overlaying one another. A peak
rises about a third of the way from the bottom in the left corner, and becomes far darker brown with
two bright red areas toward the tip where stars are forming. The light brown dust becomes more
diaphanous about half way up the screen, ending in a softer, medium brown peak toward the left
center. There’s a slight gap in the dust, which allows the blue background to come into view clearly.
About 60% of the background in this image is set in shades of blue and littered with tiny stars that are
primarily yellow, but many are also blue. The brown pillars continue, taking the shape of a shoulder at
the base, with three prominent columns rising from it toward the upper right. The top left pillar is the
largest and widest. The second one to its right is slightly smaller, and the third significantly smaller. The
peaks of the second and third pillars are set off in darker shades of brown, but also appear to have red
outlines. The second pillar has a lava-like red area at its top left, and a dark arch that looks like an
upside-down L halfway down. The third pillar is largely set off in dark brown shades, but also very bright
red all along its edges. The largest bright blue stars in the background, toward the top center, have eight
bright, long diffraction spikes. At the bottom left, in front of layers of brown dust, is another large star
with eight diffraction spikes, but it is set off in orange shades.
Créditos:
SCIENCE: NASA, ESA, CSA, STScI
IMAGE PROCESSING: Joseph DePasquale (STScI), Anton M. Koekemoer (STScI), Alyssa Pagan (STScI)
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