eso0926 — Photo Release
An Eagle of Cosmic Proportions
16 July 2009
Today ESO has released a new and stunning image of the sky around the Eagle Nebula, a stellar nursery where infant star clusters carve out monster columns of dust and gas.
Located 7000 light-years away, towards the constellation of Serpens (the Snake), the Eagle Nebula is a dazzling stellar nursery, a region of gas and dust where young stars are currently being formed and where a cluster of massive, hot stars, NGC 6611, has just been born. The powerful light and strong winds from these massive new arrivals are shaping light-year long pillars, seen in the image partly silhouetted against the bright background of the nebula. The nebula itself has a shape vaguely reminiscent of an eagle, with the central pillars being the òÀÜtalonsòÀÝ.
The star cluster was discovered by the Swiss astronomer, Jean Philippe Loys de Ch†éseaux, in 1745òÀÓ46. It was independently rediscovered about twenty years later by the French comet hunter, Charles Messier, who included it as number 16 in his famous catalogue, and remarked that the stars were surrounded by a faint glow. The Eagle Nebula achieved iconic status in 1995, when its central pillars were depicted in a famous image obtained with the NASA/ESA Hubble Space Telescope. In 2001, ESOòÀÙs Very Large Telescope (VLT) captured another breathtaking image of the nebula in the near-infrared, giving astronomers a penetrating view through the obscuring dust, and clearly showing stars being formed in the pillars.
The newly released image, obtained with the Wide-Field Imager camera attached to the MPG/ESO 2.2-metre telescope at La Silla, Chile, covers an area on the sky as large as the full Moon, and is about 15 times more extensive than the previous VLT image, and more than 200 times more extensive than the iconic Hubble visible-light image. The whole region around the pillars can now be seen in exquisite detail.
The òÀÜPillars of CreationòÀÝ are in the middle of the image, with the cluster of young stars, NGC 6611, lying above and to the right. The òÀÜSpireòÀÝ òÀÔ another pillar captured by Hubble òÀÔ is at the centre left of the image.
Finger-like features protrude from the vast cloud wall of cold gas and dust, not unlike stalagmites rising from the floor of a cave. Inside the pillars, the gas is dense enough to collapse under its own weight, forming young stars. These light-year long columns of gas and dust are being simultaneously sculpted, illuminated and destroyed by the intense ultraviolet light from massive stars in NGC 6611, the adjacent young stellar cluster. Within a few million years òÀÔ a mere blink of the universal eye òÀÔ they will be gone forever.
More information
ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the worldòÀÙs most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the worldòÀÙs most advanced visible-light astronomical observatory. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become òÀÜthe worldòÀÙs biggest eye on the skyòÀÝ.
Contacts
Henri Boffin
ESO
Garching, Germany
Tel: +49 89 3200 6222
Email: hboffin@eso.org
About the Release
Release No.: | eso0926 |
Legacy ID: | PR 26/09 |
Name: | Eagle Nebula |
Facility: | MPG/ESO 2.2-metre telescope,Very Large Telescope |