If the remaining core is dense enough, it collapses into a point of infinite density known as a singularity . Here, the laws of conventional physics break down, and space-time becomes infinitely curved.
In the 18th century, thinkers like John Michell imagined "dark stars" with gravity so strong light couldn't escape, but it wasn't until Albert Einstein’s General Relativity in 1915 that a mathematical framework existed to describe them. Download File 452.Agujero negro. La evol. de un...
Title: From Starlight to Darkness: The Evolution of the Black Hole If the remaining core is dense enough, it
The concept evolved into a visible reality in 2019 when the Event Horizon Telescope captured the first-ever image of a black hole’s shadow in the galaxy M87. Title: From Starlight to Darkness: The Evolution of
A black hole is defined by its horizon de sucesos (event horizon)—the "point of no return".
Once nuclear fusion stops, gravity takes over. The star’s core collapses in seconds, often triggering a supernova explosion that scatters heavy elements like oxygen and silicon into space.