Star Flare: Black Hole Shreds Distant Star
- Here's a breakdown of the key details from the provided text, focusing on what happened to the star and why:
- * The Star's Demise: A massive star was torn apart by a supermassive black hole.
- In essence, the star's fate was a result of a disruptive collision, a close encounter with a supermassive black hole, and the resulting gravitational forces that tore it...
Here’s a breakdown of the key details from the provided text, focusing on what happened to the star and why:
* The Star’s Demise: A massive star was torn apart by a supermassive black hole. This process is called “spaghettification” – the star was stretched into a long, thin shape due to the intense gravity.
* Cause of the Star’s Trajectory: Astronomers believe the star was originally in orbit around the black hole but was knocked off course by a collision with another, more massive object. This collision put it on a highly elliptical orbit.
* The Elliptical Orbit‘s Role: The new orbit brought the star to close to the black hole during its closest approach.
* The Flare: The bright flare observed was caused by the gas from the shredded star heating up as it spiraled into the black hole.
* Star’s Mass: the star was unusually massive, making it a rare find.
In essence, the star’s fate was a result of a disruptive collision, a close encounter with a supermassive black hole, and the resulting gravitational forces that tore it apart.
