Binary stars evolving (IMAGE) University of Toronto Caption This artist's impression shows how hot, brilliant and high-mass stars evolve. The more massive brighter star expands first, until the outer layers start to strongly feel the gravitational pull of the companion. The companion then starts to suck material from the primary star. When the primary has been stripped from its entire hydrogen-rich envelope it shrinks. Credit Navid Marvi, courtesy of the Carnegie Institution for Science Usage Restrictions N/A License Original 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.