Our home galaxy. The Milky Way is a spiral galaxy with four major arms containing young bright stars, gas, and dust. The mass of the Milky Way is estimated to be between 400 billion and one trillion times the mass of the Sun. The Milky Way's diameter is about 100,000 light-years, with the Sun orbiting about 27,000 light-years from the galactic center. However, most of the galaxy's mass consists of "dark matter" which encircles the Milky Way's disk in a vast halo. Dark matter may account for 90 percent of the Milky Way's mass.
Resources
Radio Programs
The Antennae
Seeing the future of the Milky Way
Tuesday, April 16, 2013
M2
A distant home for old stars
Sunday, January 6, 2013
Star Populations
Segregating the stars of the Milky Way
Monday, December 3, 2012
Arcturus
Tracing a star’s origins
Tuesday, August 28, 2012
Pipe Nebula
Lighting up a dark nebula
Sunday, June 17, 2012
‘Milky’ Way
The “milky” band of the Milky Way
Sunday, June 10, 2012
Hercules Cloud
Piling up stars in the outer galaxy
Thursday, May 24, 2012
Cosmic Clocks
The ticking of cosmic clocks
Thursday, April 12, 2012
Snack Time
Snack time for a giant black hole
Thursday, March 29, 2012
Alien Clusters
Alien visitors from other galaxies
Friday, March 23, 2012
Featured Images