The Rho Ophiuchi cloud (pronounced 'oh-fee-yoo-ki' and named after a bright star in the region) is found rising above the plane of the Milky Way in the night sky, bordering the constellations Ophiuchus and Scorpius.
It's one of the nearest star-forming regions to Earth, allowing us to resolve much more detail than in more distant similar regions, like the Orion nebula.
The amazing variety of colours seen in this image represents different wavelengths of infrared light. The bright white nebula in the centre of the image is glowing due to heating from nearby stars, resulting in what is called an emission nebula.
The same is true for most of the multi-hued gas prevalent throughout the entire image, including the bluish, bow-shaped feature near the bottom right.
The bright red area in the bottom right is light from the star in the centre - Sigma Scorpii - that is reflected off of the dust surrounding it, creating what is called a reflection nebula. And the much darker areas scattered throughout the image are pockets of cool, dense gas that block out the background light, resulting in absorption (or 'dark') nebulae.
WISE's longer wavelength detectors can typically see through dark nebulae, but these are exceptionally opaque.
The bright pink objects just left of centre are young stellar objects (YSOs). These baby stars are just now forming; many of them are still enveloped in their own tiny compact nebulae.
In visible light, these YSOs are completely hidden in the dark nebula that surrounds them, which is sometimes referred to as their baby blanket. We can also see some of the oldest stars in our Milky Way galaxy in this image, found in two separate (and much more distant) globular clusters.
The first cluster, M80, is on the far right edge of the image towards the top. The second, NGC 6144, is found close to the bottom edge near the centre. They both appear as small densely compacted groups of blue stars.
Globular clusters such as these typically harbour some of the oldest stars known, some as old as 13 billion years, born soon after the universe formed.
There are two other items of interest in this image as well. At the 3 o'clock position, relative to the bright central region, and about two-thirds of the way from the centre to the edge, there is a small faint red dot (more visible in the larger downloadable image files).
That dot is an entire galaxy far far away known as PGC 090239 and, at the bottom left of the image, there are two lines emerging from the edge. These were not created by foreground satellites; they are diffraction spikes (optical artifacts from the space telescope) from the bright star Antares that is just out of the field of view.
The colours used in this image represent specific wavelengths of infrared light. Blue and cyan (blue-green) represent light emitted at wavelengths of 3.4 and 4.6 microns, which is predominantly from stars. Green and red represent light from 12 and 22 microns, respectively, which is mostly emitted by dust.
Image credit: NASA/JPL-Caltech/UCLA
Posts
No comments:
Post a Comment