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Image Gallery > Astronomical Images > Galaxies and the Universe > sig05-013

image
NASA/JPL-Caltech/R. Kennicutt (University of Arizona) and the SINGS Team

NGC 1566

This beautiful spiral galaxy NGC 1566, located approximately 60 million light-years away in the constellation Dorado was captured by the Spitzer Infrared Nearby Galaxies Survey (SINGS) Legacy Project using the telescope's Infrared Array Camera (IRAC).

The faint blue light is coming from mature stars, while the "glowing" red spiral arms indicate active star formation and dust emission. Much of the active star formation is seen in the two symmetric arms that are reminiscent of other grand design spirals such as the Whirlpool galaxy. The small and very luminous blue nucleus suggests that this is a Seyfert galaxy (a galaxy that is actively emitting radiation from a very small region in its core).

The SINGS image is a four-channel false-color composite, where blue indicates emission at 3.6 microns, green corresponds to 4.5 microns, and red to 5.8 and 8.0 microns. The contribution from starlight (measured at 3.6 microns) in this picture has been subtracted from the 5.8 and 8 micron images to enhance the visibility of the dust features.

To download, choose your preferred resolution and file format below. "High-Resolution" files will always be the highest resolution and widest crop available, intended for print. Other resolutions are provided for convenient on-screen viewing.

Screen-Resolution (450x450) : JPEG (56 KB)
Medium-Resolution (900x900) : JPEG (164 KB)
High-Resolution (974x974) : JPEG (1 MB) | Mac TIFF (1.7 MB) | PC TIFF (1.7 MB)

About the Object (1)
Object name:NGC 1566
Object type:Spiral galaxy
Position (J2000):RA: 04h 20m 0.40s  Dec: -54° 56' 16.00"
Distance:60 million light-years
Constellation:Dorado
About the Data
Spitzer Data
Image Credit:NASA/JPL-Caltech/R. Kennicutt (University of Arizona) and the SINGS Team
Instrument:IRAC
Wavelength:3.6 (blue), 4.5 (green), 5.8-8.0 (red) microns
Image scale:12.2x12.2 arcmin
Orientation:North is 123 deg CW from up
Release Date:2005/09/15
Observers
Robert Kennicutt, Principal Investigator (Steward Observatory, University of Arizona)
Lee Armus (Spitzer Science Center, Caltech)
Brent Buckalew (Caltech)
George Bendo (Steward Observatory, University of Arizona)
Daniela Calzetti (Space Telescope Science Institute)
Daniel Dale (University of Wyoming)
Bruce Draine (Princeton University)
Charles Engelbracht (Steward Observatory, University of Arizona)
Karl Gordon (Steward Observatory, University of Arizona)
George Helou (Caltech)
David Hollenbach (NASA Ames Research Center)
Thomas Jarrett (Caltech)
Lisa Kewley (University of Hawaii)
Claus Leitherer (Space Telescope Science Institute)
Aigen Li (University of Missouri-Columbia)
Sangeeta Malhotra (Space Telescope Science Institute)
Helene McLaughlin (Space Telescope Science Institute)
Martin Meyer (Space Telescope Science Institute)
Eric Murphy (Yale University)
Michael Regan (Space Telescope Science Institute)
George Rieke (Steward Observatory, University of Arizona)
Marcia Rieke (Steward Observatory, University of Arizona)
Helene Roussel (Spitzer Science Center, Caltech)
Kartik Sheth (Caltech)
John-David Smith (Steward Observatory, University of Arizona)
Michele D. Thornley (Bucknell University, Space Telescope Science Institute)
Fabian Walter (MPIA Heidelberg)


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