The invisible matter might be a better name for it. It cannot be seen or detected by any instrument. We only know it’s there because of its gravitational effects on regular matter and light.
In 1933 Swiss astronomer Fritz Zwicky, working at Caltech, was studying the Coma Cluster of galaxies. The Coma Cluster, about 320 million light-years away from us contains over 1,000 galaxies. It is the nearest cluster to our home cluster, the Virgo Cluster, which contains our home galaxy, the Milky Way.
Galaxies in a cluster are held together by gravity and rotate around the center of the cluster. They don’t all rotate in the same direction but rather all rotate in different directions. Zwicky noticed something strange about their rotational speed. They were all rotating way too fast. That is the amount of visible matter in the cluster was not nearly enough to hold the galaxies inside the cluster, they should have long ago escaped the cluster. Zwicky calculated that the cluster needed 400 times as much matter as was apparent from observation to hold the cluster together. (Since Zwicky’s time that number has been reduced but the cluster still rotates far too fast for the assumed matter present.) Zwicky assumed that there had to be far more matter in the cluster than could be observed. He called this matter “dark matter”.