Credit & Copyright: NASA,  
ESA,  
E. Jullo  
(JPL), P. Natarajan  
(Yale), & J.-P. Kneib  
(LAM,  
CNRS) 
Acknowledgment: H. Ford and N. Benetiz (JHU), & T. Broadhurst (Tel Aviv)
Explanation:
What's the matter with this cluster of galaxies?  
  
To find out what forms matter takes in the  
Abell 1689 cluster requires not only deep images from  
telescopes like the  
Hubble Space Telescope, but detailed   
computer modeling  
as well.  
  
To start, almost every fuzzy yellow patch in the  
above image is an entire galaxy.  
  
A close inspection, however, shows that many background galaxies are strangely magnified  
and distorted into  
long curving arcs by the  
gravitational lens deflections of the cluster.    
  
Computer analyses of the  
placement and smoothness  
of these arcs indicate that in addition to the matter in the galaxies you can see,  
the cluster must also contain a significant amount of  
dark matter such as the model digitally superposed in   
purple.    
  
Now Abell 1689 remains enigmatic  
because the arcs are so numerous and diverse that no single   
dark matter model has emerged that can   
explain them all and still remain consistent with dark matter models needed  
to constrain their motion.    
  
Still, the detailed information available from   
clusters of galaxies like Abell 1689 gives  
hope that one day full solutions will be found that will not only fully reveal the   
dark matter in clusters,   
but also reveal the amounts of   
dark energy   
in the   
universe   
needed to lie along the line of sight to the   
distant arcs.  
  
Acknowledgment: H. Ford and N. Benetiz (JHU), & T. Broadhurst (Tel Aviv)
 Authors & editors: 
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official:  Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
  