Majestic Gas Shell
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Majestic Gas Shell

June 30, 2010
Majestic Gas Shell A majestic gas shell revealed by the Very Large Array (VLA), a collection of 27 radio antennas located at the National Radio Astronomy Observatories (NRAO) site in Socorro, N.M. What appears to be the hole of an elongated smoke ring in this image, is really an enormous, nearly empty, bubble blown into the dusty, gas disk of our Milky Way Galaxy. Important: This image is approved for personal use only, by the National Radio Astronomy Observatory. If you wish to use this image for any other purpose, please read the NRAO Image Use Policy. More about this Image Interstellar bubbles like the one in this image are sculpted by the force of the wind and radiation from typically a few dozen hot, massive stars along with the explosive impact of dying stars, called supernovae. The force sweeps up the disk's gas that is in its path, creating a gas shell surrounding a bubble. The neighborhood of our own solar system resides in such a cavity. However the shell in this image, catalogued using its coordinates as galactic shell GS 62.1+0.2-18, is located at a distance of 30,000 light years from Earth, and measures 1,100 by 520 light years. Despite its distance, this "smoke ring" appears so large on the sky that the apparent width of the full moon would fit eight times inside it. The bright yellowish-orange dots scattered across this image are clusters of young, massive stars surrounded by hot gas, called nebulae. Astronomers from the International/VLA Galactic Plane Survey have determined that none of these clusters harbor the stars that blew the giant shell since none of the clusters are at the same distance as the shell. Indeed, they all are located closer to the Earth than the shell is. Probably, the stars that blew GS 62.1+0.2-18's hole perished as supernova explosions. This image shows only a small part of a survey which uses both VLA and the Green Bank telescopes to trace, in detail, the cool gas in our galaxy. This gas has been colored purple, blue and green in this image. In order to show the locations of star clusters, the image of gas was overlaid with 2 additional images. The one of radio emission associated with regions of hot gas was colored orange, while heated dust, imaged in infrared by the Midcourse Space Experiment satellite, was colored red. The principal investigator for the survey is A. R. Taylor. This study is published by VGPS investigators J. M. Stil, A. R. Taylor, J. M. Dickey, D. W. Kavars, P. G. Martin, T. A. Rothwell, A. I. Boothroyd, Felix J. Lockman, and N. M. McClure-Griffiths in the Astronomical Journal, Volume 132, number 3, page 1158. (Date of Image: unknown)

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