B A R R E D   S P I R A L S



NGC 4314

NGC 4123

NGC 5850

NGC 3953

NGC 5905

NGC 3992


All images courtesy David W. Hogg, Michael R. Blanton, and the Sloan Digital Sky Survey Collaboration.
Copyright 2006 Michael R. Blanton & David W. Hogg. See the Sloan Digital Sky Survey Home Page.


The Milky Way is a barred spiral galaxy like the six objects pictured on this page (see Spiral Structure of the Milky Way). Like many nearby galaxies, ours may have a somewhat irregular, disrupted appearance, given its long history of violent interactions with smaller nearby galaxies such as the Large and Small Magellanic Clouds.

Large surveys of spiral galaxies similar in age to the Milky Way have shown that more than half (65%) contain central bars. A study by Kartik Sheth and colleagues recently demonstrated that bars are an indication of advanced evolution. They require billions of years to grow out of more compact galactic cores. When the universe was half its present age, less than half of all spiral galaxies were barred.


See also Rings and The Galactic Rim.







All text is copyright Raymond Harris 2006-2008. Image credits appear in the accompanying caption.