Chandrashekar limit explained in hindi

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All things die, even stars. When stars run out of hydrogen — the fuel that sustains the nuclear fusion reactors at their cores — they become unstable and collapse in on themselves. But not all stars collapse in the same way. Some of the most massive ones explode into a supernova and then collapse down into neutron stars, or black holes. This knowledge is given to us by an Indian astrophysicist Subrahmanyan Chandrasekhar. He had given us the value which is known as the Chandrashekhar limit which is the maximum mass at which a star near the end of its life cycle can become a white dwarf and above which the star will collapse to form a neutron star or black hole : a stellar mass equal to about 1.4 solar masses • To know more abou Chandrashekar limit watch this entire video till the end. • Also do not forget to like share and subscribe our channel for more videos. • Thanks for watching. • Music credit- Whitesand musics • / @whitesandcomposer • Video credit- Pixabay, Hubble, Nasa • FAIR-USE COPYRIGHT DISCLAIMER This video is meant for Educational/Inspirational purpose only. We do not own any copyrights, all the rights go to their respective owners. The sole purpose of this video is to inspire, empower and educate the viewers. • #ChandrashekarLimit

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