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ssc2004-09a
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| NASA/JPL-Caltech/J. Keene (SSC/Caltech) |
A Parallelogram-Shaped Meal
This image taken by NASA's Spitzer Space Telescope shows in unprecedented detail the galaxy Centaurus A's last big meal: a spiral galaxy seemingly twisted into a parallelogram-shaped structure of dust. Spitzer's ability to see dust and also see through it allowed the telescope to peer into the center of Centaurus A and capture this galactic remnant as never before.
An elliptical galaxy located 10 million light-years from Earth, Centaurus A is one of the brightest sources of radio waves in the sky. These radio waves indicate the presence of a supermassive black hole, which may be "feeding" off the leftover galactic meal.
A high-speed jet of gas can be seen shooting above the plane of the galaxy (the faint, fuzzy feature pointing from the center toward the upper left). Jets are a common feature of galaxies, and this one is probably receiving an extra boost from the galactic remnant.
Scientists have created a model that explains how such a strangely geometric structure could arise. In this model, a spiral galaxy falls into an elliptical galaxy, becoming warped and twisted in the process. The folds in the warped disc create the parallelogram-shaped illusion.
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| About the Object | | Object name: | Centaurus A, NGC 5128 | | Object type: | Elliptical galaxy | | Position (J2000): | RA: 13h 25m 42.09s Dec: -42° 53' 59.50" | | Distance: | 3.4 Mpc or 11,000,000 light-years | | Constellation: | Centaurus | | Magnitude: | 7.0 |
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About the Data
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Spitzer Data
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| Image Credit: | NASA/JPL-Caltech/J. Keene (SSC/Caltech) | | Instrument: | IRAC | | Wavelength: | 3.6 to 8 microns | | Exposure Date: | 10 Feb 2004 | | Exposure Time: | about 60 seconds | | Image scale: | 27.1 x 17.7 arcmin | | Orientation: | North is Up | | Release Date: | 2004/06/01 |
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Observers
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Jocelyn Keene, Principal Investigator (JPL & SSC)
Peter Eisenhardt (JPL)
Varoujan Gorjian (JPL)
Charles Lawrence (JPL)
Alice Quillen (University of Rochester)
Karl Stapelfeldt (JPL)
Daniel Stern (JPL)
Michael Werner (JPL) |
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