What are the contributions of Chandrasekhar?

His mathematical treatment of stellar evolution yielded many of the current theoretical models of the later evolutionary stages of massive stars and black holes. The Chandrasekhar limit is named after him.

What did Chandrasekhar do as a student at Cambridge?

In his first year at Cambridge, as a research student of Fowler, Chandrasekhar spent his time calculating mean opacities and applying his results to the construction of an improved model for the limiting mass of the degenerate star. At the meetings of the Royal Astronomical Society, he met E. A. Milne.

Why did Chandrasekhar win the Nobel Prize in Physics?

Chandrasekhar was awarded the Nobel Prize in Physics in 1983 for his studies on the physical processes important to the structure and evolution of stars. Chandrasekhar accepted this honor, but was upset the citation mentioned only his earliest work, seeing it as a denigration of a lifetime’s achievement. He shared it with William A. Fowler .

Why did Chandrasekhar move from Chicago to Princeton?

In 1946, when Princeton University offered Chandrasekhar a position vacated by Henry Norris Russell with a salary double that of Chicago’s, Hutchins incremented his salary matching with that of Princeton’s and persuaded Chandrasekhar to stay in Chicago.

How good was Dhyan Chandra?

For a nation starved of wins abroad, Chandra was a rare jewel: he was for long India’s biggest match-winner overseas, with 42 wickets in five Tests. Batsmen didn’t know quite what to expect from him and sometimes neither did Chandra himself, as he once admitted.

Was Chandrasekhar the biggest spinner of the cricket ball?

Chandrasekhar was not the biggest spinner of the cricket ball. His strength lay in his unnerving accuracy delivered from a long run up. The batsmen were left confounded by a spate of sharp googlies, spitting leg-breaks and top-spinners at a pace of a medium quickie.

How has Chandrasekhar revised the model of stellar dynamics?

Chandrasekhar revised the models of stellar dynamics first outlined by Jan Oort and others by considering the effects of fluctuating gravitational fields within the Milky Way on stars rotating about the galactic centre.