For the first time the scientists of Laser Interferometer Gravitational Wave Laboratory (LIGO) have recently recorded the first merger of black holes that were of unequal mass black holes.
The event has been named as GW190412.
This observation once again confirms Einstein’s theory of general relativity.
That theory predicts the existence of higher harmonics, i.e. gravitational waves at two or three times the fundamental frequency.
One was some 30 times the mass of the Sun and the other had a mass nearly 8 times the solar mass.
Solar Mass is the standard of mass in astronomy that is used to indicate masses of other masses.
One solar mass is equal to 2×1030 Kg.
This is almost five years after the first ever detection of gravitational wave signals by these powerful detectors.
The actual merger took place at a distance of 2.5 billion light years away.
About LIGO
The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory.
It works to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool.
Two large observatories were built in the United States with the aim of detecting gravitational waves by laser interferometry.
A black hole is an object in space that is so dense and has such strong gravity that no matter or light can escape its pull.
Because no light can escape, it is black and invisible.