However, the most compelling evidence for the existence of dark matter came more than 40 years later, when astronomers started measuring the speeds at which stars orbit the center of the galaxy they are in. If you look at the photo of a spiral galaxy above, you will see that it is much brighter at its center than it is at its edges. Based on such observations, it was assumed that most of a galaxy’s mass is located at its center. If that assumption were correct, it would mean that the stars near the center of the galaxy would orbit the center faster than the stars at the edge of the galaxy, just as the planets near the sun orbit much faster than the planets far from the sun.
In 1975, Dr. Vera Rubin and Dr. Kent Ford announced at a meeting of the American Astronomical Society that their studies indicated the stars in a galaxy orbit the center at roughly the same speed, regardless of where they are in the galaxy. This was a shock, and about the only thing that could explain it was the assumption that there was a lot of mass spread throughout the galaxy that could not be detected. Dark matter, which up until that time was mostly a curiosity, soon became a staple of modern astronomy. Today, astrophysicists estimate that 83% of the matter in the universe is dark matter – stuff that we cannot (as yet) detect directly.1