A look at the night sky at any time of year will reveal a faint band of light stretching across the sky, either through the middle or near the horizon. The ancient Greeks saw this band of light and called it "galaxies kuklos," for "milk circle." The Romans called it the "Milky Way." In 1610, Galileo used the first telescopes and determined that the light of the Milky Way comes from billions of dim stars that surround us.

For centuries, astronomers asked many basic questions about the Milky Way. What is it? What is it made of? What is it shaped like? These questions were difficult to answer for several reasons.
The 20th century brought great advancements in telescope technology. Large optical, radio, infrared, and X-ray telescopes (both ground-based and orbiting space telescopes) allowed astronomers to peer through the vast quantities of dust and far into space. With these tools, they could piece together what the Milky Way actually looks like.
What they discovered was amazing:
Come follow us on a journey of discovery as we explore the Milky Way. We'll examine how astronomers figured out its shape, size and structure. We'll look at how the stars within it move and how the Milky Way compares to other galaxies.
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