Elliptical Galaxy Centaurus A from CFHT
			
		
		
			Credit & 
Copyright:  
Jean-Charles
Cuillandre
(CFHT) &
Giovanni Anselmi
(Coelum Astronomia),
Hawaiian Starlight
		
		
			Why is peculiar galaxy Centaurus A so dusty?  
Dramatic dust lanes that run 
across the galaxy's center mark 
Cen A.  
These dust lanes are so thick they almost completely obscure the 
galaxy's center in 
visible light.  
This is particularly unusual as 
Cen A's 
red stars and round shape are characteristic of a giant 
elliptical galaxy, 
a galaxy type usually low in dark dust.  
Cen A, 
also known as NGC 5128, is also unusual compared to an average 
elliptical galaxy because it contains a 
higher proportion of young blue stars and is a 
very strong source of 
radio emission.  
Evidence indicates that 
Cen A is likely the result of the 
collision of two 
normal galaxies.  
During the collision, many 
young stars were formed, but
details of the creation of 
Cen A's unusual dust belts are still being researched.  
Cen A lies only 13 million 
light years away, making it the closest 
active galaxy.  
Cen A, 
pictured above,  spans 60,000 light years and can be 
seen with binoculars toward the constellation of 
Centaurus.