Universe Observed From A Pale Blue Dot

Though didn’t seem very sharp, this picture has amazing stories to reveal. The picture shows a baby star, 1,149 light-years away from our Earth, blowing two massive “bubbles”. But instead of bubble gum, this youngster, called HH 46/47, is using powerful jets of gas to make bubbles in outer space.
The infant star can be seen as a white spot toward the center of the image. The two bubbles are shown as hollow elliptical shells of bluish-green material extending from the star. Wisps of green in the image reveal warm molecular hydrogen gas, while the bluish tints are from starlight scattered by surrounding dust.
These bubbles formed when powerful jets of gas, traveling at 200 to 300 kilometers per second, (about 120 to 190 miles per second), smashed into the cosmic cloud of gas and dust that surrounds HH 46/47. Red specks at the end of each bubble show the presence of hot sulfur and iron gas where the star’s narrow jets are currently crashing head-on into the cosmic cloud’s gas and dust material.
Taken by Spitzer Space Telescope, this infrared image is a three-color composite, with data at 3.6 microns represented in blue, 4.5 and 5.8 microns shown in green, and 24 microns represented as red.
For astronomers who know what to look for, Spitzer’s supersensitive infrared instruments are excellent tools for studying young stars embedded within thick clouds of cosmic dust and gas, revealing information about their growth. However, it is often difficult for most people to get a clear, detailed picture of infant stars and their “growing pains”.
When we see a star through a telescope, its image is blurred in a known way, and the smaller the telescope the larger is the blurring. To clear up these blurring, astronomers at NASA’s Jet Propulsion Laboratory (JPL) developed an advanced image-processing technique for Spitzer data called Hi-Res deconvolution. This process reduces blurring and makes the image sharper and cleaner, enabling astronomers to see the emissions around forming stars in greater detail. When this technique applied to the Spitzer image of HH 46/47, they were able to see winds from the star and jets of gas that are carving the celestial bubbles.
According to Dr. William Langer from JPL, this image will help scientists determine which of many different mechanisms are responsible for producing the winds and jets of baby stars.
Image credits: NASA/JPL-Caltech/T. Velusamy (Jet Propulsion Laboratory)
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This entry was posted by dhani on Thursday, November 15th, 2007 at 3:00 am and is filed under Discoveries, Pictures. You can follow any responses to this entry through the RSS 2.0 feed.
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