GW231123 : Recently, an international team of astrophysicists announced the discovery of an exceptionally rare black hole merger, identified as GW231123.
o As they orbit, they emit gravitational waves, ripples in spacetime predicted by Einstein’s theory of general relativity, causing them to lose energy and gradually move closer.
o Eventually, their orbits decay, leading to a final collision where they merge into a single, more massive black hole.
o This powerful event releases a burst of gravitational waves, detectable by observatories like LIGO (USA), Virgo (Italy), and KAGRA (Japan).
o The combined mass falls in the "mass gap" (100–150 solar masses), where existing models predict very few black holes should exist.
o Both black holes were observed to be spinning at extremely high speeds, challenging current theories of black hole formation and angular momentum.
o Black holes grow by accreting nearby matter, pulling in stars, gas, and dust through their intense gravitational field.
o The central point of infinite density where the black hole’s entire mass is concentrated.
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