Pandora's Cluster -- Abell 2744

Stsci_2011-17a_1024

stsci_2011-17a June 22nd, 2011

Credit: NASA, ESA, J. Merten (Institute for Theoretical Astrophysics, Heidelberg/Astronomical Observatory of Bologna), and D. Coe (STScI)

A team of scientists studying the galaxy cluster Abell 2744, nicknamed Pandora's Cluster, have pieced together the cluster's complex and violent history using telescopes in space and on the ground, including the Hubble Space Telescope, the European Southern Observatory's Very Large Telescope, the Japanese Subaru telescope, and NASA's Chandra X-ray Observatory. The giant galaxy cluster appears to be the result of a simultaneous pile-up of at least four separate, smaller galaxy clusters. The crash took place over a span of 350 million years. The galaxies in the cluster make up less than five percent of its mass. The gas (around 20 percent) is so hot that it shines only in X-rays (colored red in this image). The distribution of invisible dark matter (making up around 75 percent of the cluster's mass) is colored here in blue. Dark matter does not emit, absorb, or reflect light, but it makes itself apparent through its gravitational attraction. To pinpoint the location of this elusive substance the team exploited a phenomenon known as gravitational lensing. This is the bending of light rays from distant galaxies as they pass through the gravitational field created by the cluster. The result is a series of telltale distortions in the images of galaxies in the background of the Hubble and VLT observations. By carefully analyzing the way that these images are distorted, it is possible to accurately map where the dark matter lies. Chandra mapped the distribution of hot gas in the cluster. The data suggest that the complex collision has separated out some of the hot gas (which interacts upon collision) and the dark matter (which does not) so that they now lie apart from each other, and from the visible galaxies. Near the core of the cluster there is a "bullet" shape where the gas of one cluster collided with that of another to create a shock wave. The dark matter passed through the collision unaffected. In another part of the cluster, galaxies and dark matter can be found, but no hot gas. The gas may have been stripped away during the collision, leaving behind no more than a faint trail.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2011/news-2011-17

Curator: STScI, Baltimore, MD, USA

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

Image Details Image Details

Image Type
Observation
Object Name
Pandora's Cluster Abell 2744
Subject - Distant Universe
Cosmology > Phenomenon > Dark Matter
Galaxy > Grouping > Cluster

Distance Details Distance

Stsci_2011-17a_128
 

Position Details Position Details

Position (FK5)
RA = 0h 14m 28.0s
DEC = -30° 22’ 1.3”
Orientation
North is 0.1° CCW
Field of View
6.7 x 6.7 arcminutes
Constellation
Sculptor

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (ACS) Optical (B) 435.0 nm
Green Hubble (ACS) Optical (V) 606.0 nm
Red Hubble (ACS) Optical (I) 814.0 nm
Blue VLT Optical (B) -
Green VLT Optical (R) -
Red VLT Optical (I) -
Red Chandra X-ray (.5-7keV) -
Dark matter map is displayed as blue.
Spectrum_base
Blue
Green
Red
Stsci_2011-17a_1280
×
ID
2011-17a
Subject Category
D.6.2.3   D.5.5.3  
Subject Name
Pandora's Cluster, Abell 2744
Credits
NASA, ESA, J. Merten (Institute for Theoretical Astrophysics, Heidelberg/Astronomical Observatory of Bologna), and D. Coe (STScI)
Release Date
2011-06-22T00:00:00
Lightyears
Redshift
.308
Reference Url
https://hubblesite.org/contents/news-releases/2011/news-2011-17
Type
Observation
Image Quality
Good
Distance Notes
Facility
Hubble, Hubble, Hubble, VLT, VLT, VLT, Chandra
Instrument
ACS, ACS, ACS
Color Assignment
Blue, Green, Red, Blue, Green, Red, Red
Band
Optical, Optical, Optical, Optical, Optical, Optical, X-ray
Bandpass
B, V, I, B, R, I, .5-7keV
Central Wavelength
435, 606, 814
Start Time
2009-10-29T00:00:00, 2009-10-27T00:00:00, 2009-10-27T00:00:00
Integration Time
Dataset ID
Notes
D
Coordinate Frame
FK5
Equinox
2000.0
Reference Value
3.6164592766900001, -30.3670358884999985
Reference Dimension
8068.0000000000000000, 8067.0000000000000000
Reference Pixel
2120.7284851099998377, 6402.4384765599997991
Scale
-0.0000138727584916, 0.0000138727584916
Rotation
0.0715176833992943
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
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-p1117a-f-8068x8067.tif
Resource URL
https://mast.stsci.edu/api/latest/Download/file?uri=mast:OPO/product/STSCI-H-p1117a-f-8068x8067.tif
Related Resources
http://hubblesite.org/newscenter/archive/releases/2011/17
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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There is no distance meta data in this image.

 

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