Archivo de imágenes de Hubble

Galaxia activa Centauro A

Resembling looming rain clouds on a stormy day, dark lanes of dust crisscross the giant elliptical galaxy Centaurus A. Hubble's panchromatic vision, stretching from ultraviolet through near-infrared wavelengths, reveals the vibrant glow of young, blue star clusters and a glimpse...

Fecha
Jan 1, 2011
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2011-18-2858-image
Por

Resembling looming rain clouds on a stormy day, dark lanes of dust crisscross the giant elliptical galaxy Centaurus A.

Hubble's panchromatic vision, stretching from ultraviolet through near-infrared wavelengths, reveals the vibrant glow of young, blue star clusters and a glimpse into regions normally obscured by the dust.

The warped shape of Centaurus A's disk of gas and dust is evidence for a past collision and merger with another galaxy. The resulting shockwaves cause hydrogen gas clouds to compress, triggering a firestorm of new star formation. These are visible in the red patches in this Hubble close-up.

At a distance of just over 11 million light-years, Centaurus A contains the closest active galactic nucleus to Earth. The center is home for a supermassive black hole that ejects jets of high-speed gas into space, but neither the supermassive black hole or the jets are visible in this image.

This image was taken in July 2010 with Hubble's Wide Field Camera 3.

Credits

NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration;
Acknowledgment: R. O'Connell (University of Virginia) and the WFC3 Scientific Oversight Committee

Detalles de la imagen

About The Object
Object NameCentaurus A, Cen A, NGC 5128
Object DescriptionElliptical/Active Galaxy
R.A. Position13h 25m 27.61s
Dec. Position-43° 1' 8.79"
ConstellationCentaurus
Distance1 million light-years (3.4 parsecs)
DimensionsThis image is 2.7 arcminutes (8,500 light-years or 2,600 parsecs) wide.
About The Data
Data DescriptionThe image was created from Hubble data from proposal : R. O'Connell (University of Virginia), B. Balick (University of Washington), H. Bond (STScI), D. Calzetti (University of Massachusetts), M. Carollo (Swiss Federal Institute of Technology, Zurich), M. Disney (University of Wales, College of Cardiff), M. Dopita (Australian National University), J. Frogel (Ohio State University Research Foundation), D. Hall (University of Hawaii), J. Holtzman (New Mexico State University), P. McCarthy (Carnegie Institution of Washington), F. Paresce (European Southern Observatory, Germany), A. Saha (NOAO/AURA), J. Silk (University of Oxford), A. Walker (NOAO/CTIO), B. Whitmore (STScI), R. Windhorst (Arizona State University), and E. Young (University of Arizona). Science team: S. Kaviraj (Imperial College London and the University of Oxford), R. Crockett (University of Oxford), and J. Silk (University of Oxford).
InstrumentHST>WFC3/UVIS
Exposure DatesJuly 6-17, 2010, Exposure Time: 4.8 hours
FiltersF225W (U), F336W (U), F438W (B), F487N (H-beta), F502N ([O III]), F547M (y), F657N (H-alpha + [N II]), F673N ([S II]), and F814W (I)
About The Image
Color InfoThis image is a composite of separate exposures acquired by the WFC3 instrument on HST. Several filters were used to sample broad and narrow wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: White: F225W (U) + F336W (U) + F438W (B) Blue: F487N (H-beta) Cyan: F502N ([O III]) Aqua: F547M (y) Red/orange: F657N (H-alpha + [N II]) Yellow/green: F673N ([S II]) Red: F814W (I)

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