Why stars that survive close black hole encounters produce dimmer flares
Astronomers have discovered that stars surviving partial tidal disruption events near supermassive black holes produce progressively dimmer flares because of their initial rotation speed. Rapidly spinning stars lose material in a way that causes subsequent flares to fade more quickly.
Why it matters
This finding helps astrophysicists better understand the complex gravitational interactions between stars and black holes, solving a long-standing puzzle in stellar observation.
Some stars can make repeated close passes around supermassive black holes, losing part of their material each time while surviving to return again. These encounters produce bursts of light, or flares, that can recur months or even years apart. But astronomers have been puzzled by a pattern seen in some of these systems: each successive flare becomes dimmer. According to a study published in The Astrophysical Journal, researchers now think the answer may lie in how fast the star was spinning before its first encounter with the black hole. The research suggests that an unusually rapid initial spin can reproduce the progressively fading flares seen in some systems.A star that survivesWhen a star ventures too close to a supermassive black hole, the difference in the black hole's gravitational pull across the star can become so extreme that it is torn apart.
Get smarter about the news
Sign up free for a feed built around what you actually care about, Dive Deeper research on any story, and the full text of every article.
Create free accountAlready have an account? Sign in