Velocity Map of Andromeda Stars (IMAGE) University of California - Santa Cruz Caption Dots show locations of stars in the spectroscopic survey superimposed on an image of the Andromeda galaxy (M31). Dots are color coded according to their velocity relative to the Milky Way, as measured using the DEIMOS spectrograph on the Keck II telescope. The center of M31 is moving towards us at 300 km/s, whereas stars to the northeast of the center have more positive velocities, indicating that they are moving away from us relative to M31's center. Credit Claire Dormanm European Space Agency Usage Restrictions For use only with news coverage of this research. License Licensed content Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.