A Multi-Wavelength View of Radio Galaxy Hercules A

Stsci_2012-47a_1024

stsci_2012-47a November 29th, 2012

Credit: NASA, ESA, S. Baum and C. O'Dea (RIT), R. Perley and W. Cotton (NRAO/AUI/NSF), and the Hubble Heritage Team (STScI/AURA)

Spectacular jets powered by the gravitational energy of a supermassive black hole in the core of the elliptical galaxy Hercules A illustrate the combined imaging power of two of astronomy's cutting-edge tools, the Hubble Space Telescope's Wide Field Camera 3, and the recently upgraded Karl G. Jansky Very Large Array (VLA) radio telescope in New Mexico. Some two billion light-years away, the yellowish elliptical galaxy in the center of the image appears quite ordinary as seen by Hubble in visible wavelengths of light. The elliptical galaxy is roughly 1,000 times more massive than the bulge of our Milky Way and harbors a 2.5-billion-solar-mass central black hole that is 1,000 times more massive than the black hole in the Milky Way. But the innocuous-looking galaxy, also known as 3C 348, has long been known as the brightest radio-emitting object in the constellation Hercules. Emitting nearly a billion times more power in radio wavelengths than our Sun, the galaxy is one of the brightest extragalactic radio sources in the entire sky. The VLA radio data reveal enormous, optically invisible jets that, at one-and-a-half million light-years wide, dwarf the visible galaxy from which they emerge. The jets are very-high-energy plasma beams, subatomic particles and magnetic fields shot at nearly the speed of light from the vicinity of the black hole. The outer portions of both jets show unusual ring-like structures suggesting a history of multiple outbursts from the supermassive black hole at the center of the galaxy. The innermost parts of the jets are not visible because of the extreme velocity of the material; relativistic effects confine all of the light to a narrow cone aligned with the jets, and so that light is not seen by us. Far from the galaxy, the jets become unstable and break up into the rings and wisps. The entire radio source is surrounded by a very hot, X-ray-emitting cloud of gas, not seen in this optical-radio composite. Hubble's view of the field also shows a companion elliptical galaxy very close to the center of the optical-radio source, which may be merging with the central galaxy. Several other elliptical and spiral galaxies that are visible in the Hubble data may be members of a cluster of galaxies. Hercules A is by far the brightest and most massive galaxy in the cluster.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2012/news-2012-47

Curator: STScI, Baltimore, MD, USA

Image Use Policy: http://hubblesite.org/copyright/

Image Details Image Details

Image Type
Observation
Object Name
Hercules A Herc A 3C 348
Subject - Distant Universe
Galaxy > Activity > AGN
Galaxy > Type > Elliptical

Distance Details Distance

Universescale3
637,000,000 light years
Stsci_2012-47a_128
 

Position Details Position Details

Position (ICRS)
RA = 16h 51m 8.2s
DEC = 4° 59’ 34.5”
Orientation
North is 36.0° CW
Field of View
3.3 x 2.4 arcminutes
Constellation
Hercules

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (WFC3) Optical (V) 606.0 nm
Orange Hubble (WFC3) Optical (I) 814.0 nm
Red VLA Radio (C) -
Green VLA Radio (C) -
Blue VLA Radio (X) -
8-Oct-12
Spectrum_xray1w
Blue
Orange
Stsci_2012-47a_1280
×
ID
2012-47a
Subject Category
D.5.3.2   D.5.1.4  
Subject Name
Hercules A, Herc A, 3C 348
Credits
NASA, ESA, S. Baum and C. O'Dea (RIT), R. Perley and W. Cotton (NRAO/AUI/NSF), and the Hubble Heritage Team (STScI/AURA)
Release Date
2012-11-29T00:00:00
Lightyears
637,000,000
Redshift
0.156
Reference Url
https://hubblesite.org/contents/news-releases/2012/news-2012-47
Type
Observation
Image Quality
Good
Distance Notes
2.1 billion light-years (637 million parsecs or redshift z = 0.156)
Facility
Hubble, Hubble, VLA, VLA, VLA
Instrument
WFC3, WFC3, -, -, -
Color Assignment
Blue, Orange, Red, Green, Blue
Band
Optical, Optical, Radio, Radio, Radio
Bandpass
V, I, C, C, X
Central Wavelength
606, 814, -, -, -
Start Time
2012-10-08, 2012-10-08, -, -, -
Integration Time
Dataset ID
Notes
8
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
252.78403830924, 4.99292628183
Reference Dimension
5000.00, 3552.00
Reference Pixel
2535.73867592424, 1847.41734505712
Scale
-0.00001113711, 0.00001113711
Rotation
-35.98762088520
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
World Coordinate System resolved using PinpointWCS 0.9.2 revision 218+ by the Chandra X-ray Center FITS X FITS Y EPO X EPO Y 1475.12 365.43 4463.96 2628.77 1699.62 1850.15 1516.17 2985.29 767.03 2413.44 457.79 1109.64 220.45 1668.95 1961.54 73.82 769.31 1074.95 3103.04 1193.70 741.56 186.05 4861.37 1190.86 1349.21 1291.29 2641.05 2326.37 Center Pixel Coordinates: 2500.00 252.78389884049 1776.00 4.99205794535
Creator (Curator)
STScI
URL
http://hubblesite.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
Address
3700 San Martin Drive
City
Baltimore
State/Province
MD
Postal Code
21218
Country
USA
Rights
http://hubblesite.org/copyright/
Publisher
STScI
Publisher ID
stsci
Resource ID
STSCI-H-p1247a-f-5000x3552.tif
Resource URL
https://mast.stsci.edu/api/latest/Download/file?uri=mast:OPO/product/STSCI-H-p1247a-f-5000x3552.tif
Related Resources
http://hubblesite.org/newscenter/archive/releases/2012/47
Metadata Date
2022-07-06T00:00:00
Metadata Version
1.2
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Detailed color mapping information coming soon...

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Universescalefull
637,000,000 light years

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