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Spectacular new image of the Sculptor Galaxy

By observing in infrared light, VISTA's view is less affected by dust and reveals myriad cooler stars as well as a prominent bar of stars across the central region.
Provided by ESO, Garching, Germany
Sculptor Galaxy (NGC 253)
Infrared/visible light comparison of views of the Sculptor Galaxy (NGC 253).
ESO
June 17, 2010
The European Southern Observatory's (ESO) Visible and Infrared Survey Telescope for Astronomy (VISTA) at the Paranal Observatory in Chile has taken a spectacular new image of the Sculptor Galaxy (NGC 253) as part of one of its first major observational campaigns. By observing in infrared light, VISTA's view is less affected by dust and reveals myriad cooler stars as well as a prominent bar of stars across the central region. The VISTA image provides new information on the history and development of the galaxy.

The Sculptor Galaxy lies in the constellation of the same name, and it is one of the brightest galaxies in the sky. It is prominent enough to view with good binoculars, and Caroline Herschel from England discovered the galaxy in 1783. NGC 253 is a spiral galaxy that lies about 13 million light-years away. It is the brightest member of a small collection of galaxies called the Sculptor Group, one of the closest such groupings to our own Local Group of galaxies. Part of its visual prominence comes from its status as a starburst galaxy, one in the throes of rapid star formation. NGC 253 is also very dusty, which obscures the view of many parts of the galaxy. Seen from Earth, the galaxy is almost edge on, with the spiral arms clearly visible in the outer parts, along with a bright core at its center.

VISTA, the latest addition to ESO's Paranal Observatory in the Chilean Atacama Desert, is the world's largest survey telescope. After being handed over to ESO at the end of 2009, the telescope was used for two detailed studies of small sections of the sky before it embarked on the larger surveys that are now in progress. One of these "mini surveys" was a detailed study of NGC 253 and its environment.

As VISTA works at infrared wavelengths, it can see right through most of the dust that is such a prominent feature of the Sculptor Galaxy when viewed in visible light. Huge numbers of cooler stars that are barely detectable with visible-light telescopes are also seen. The VISTA view reveals most of what was hidden by the thick dust clouds in the central part of the disk and allows a clear view of a prominent bar of stars across the nuclear region, a feature that is not seen in visible-light pictures. The majestic spiral arms now spread over the whole disk of the galaxy.

The spectacular viewing conditions VISTA shares with ESO's Very Large Telescope (VLT), located on the next mountain peak, also allow VISTA images to be exceptionally sharp for a ground-based telescope.

With this powerful instrument at their command, astronomers wanted to peel away some of the mysteries of the Sculptor Galaxy. They are studying myriad cool red giant stars in the halo that surrounds the galaxy, measuring the composition of some of NGC 253's small dwarf satellite galaxies, and searching for undiscovered new objects such as globular clusters and ultra-compact dwarf galaxies. Using the unique VISTA data, they plan to map how the galaxy formed and evolved.
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