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Meghnad Saha: Reading the Temperature of Stars

Every time an astronomer reads a star’s temperature from its spectrum, they’re using an equation a Bengali physicist worked out in 1920. Meghnad Saha never won a Nobel Prize. His equation still underpins how modern astrophysics understands stars.

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Must Know

  • Meghnad Saha was born on 6 October 1893, in Dhaka district, Bengal. He came from a poor family, the fifth of eight children of a village shopkeeper.
  • In 1920, Saha developed the Saha ionization equation. It relates a gas’s ionization state to its temperature and pressure, using quantum and statistical mechanics together.
  • This equation let astronomers read a star’s actual temperature from its light spectrum. It became foundational to modern stellar astrophysics and spectral classification.
  • Saha held professorships at the University of Allahabad and the University of Calcutta. The Royal Society elected him a Fellow in 1927.
  • In 1950, Saha founded the Institute of Nuclear Physics in Kolkata. After his death, it was renamed the Saha Institute of Nuclear Physics in his honour.
  • Saha died on 16 February 1956, in New Delhi.

Good to Know

  • Saha founded the journal Science and Culture in 1935. He used it to push for a stronger relationship between science and Indian public life and policy.
  • In 1952, the Council of Scientific and Industrial Research appointed a Calendar Reform Committee, chaired by Saha. After three years of study, it proposed a unified Indian National Calendar based on the Saka Era.
  • The Government of India adopted the committee’s Saka-Era-based calendar on 22 March 1957. It’s still used alongside the Gregorian calendar for official purposes today.
  • In 1951, Saha was elected to India’s Parliament as an independent candidate, extending his public role beyond pure science.

Test Yourself

1. Meghnad Saha’s 1920 ionization equation relates a gas’s ionization state to its temperature and which other physical quantity?

 

Great to Know

  • Saha’s ionization equation is often cited as Nobel-calibre work that never received the prize. Several historians of science consider this one of the more notable omissions in the Nobel Committee’s history.
  • Saha’s later career shows a pattern seen in several major Indian scientists of his generation. Pure research eventually gave way to institution-building and public policy work, reflecting a period when India’s scientific infrastructure itself still needed to be built from scratch.
  • The Saha equation’s core insight, connecting an abstract physical quantity (temperature) to something directly observable (a spectral line pattern), is a recurring theme in astrophysics: most of what we know about distant stars comes from indirect inference like this, not direct measurement.

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