Log in
EN हिंदी
Meghnad Saha
← All heroes
Science & innovation · West Bengal

Reading the temperature of the stars

Why do some lines in a star's light appear and others vanish? Meghnad Saha, who came from a poor family in Bengal, answered with a single equation, and changed how astronomers read the sky.

Meghnad Sahaमेघनाद साहा
WhatsApp X Facebook

Meghnad Saha. Photo: archival image; credit being confirmed

Listen to this story0:00 / 1:41
Narrated with an AI voice
Born
6 October 1893, Dhaka district (now Bangladesh)
Died
1956
Field
Astrophysics, thermal ionisation
Institutions
University of Allahabad; University of Calcutta; Institute of Nuclear Physics
Honours
Fellow of the Royal Society 1927
c. 1920Saha ionisation equation
1927Fellow of the Royal Society

Against the odds

Meghnad Saha was born on 6 October 1893 into a family of modest means in Dhaka district. Despite money troubles he kept studying, and at Presidency College he was among brilliant contemporaries including Satyendra Nath Bose.

Scholarships and academic excellence carried him past poverty and the limits of the colonial education system, and short research stays abroad linked his ideas to the international scientific network.

One equation for the stars

Around 1920 he developed the theory of thermal ionisation, now called the Saha ionisation equation. It gave a quantitative link between temperature, pressure and the ionisation states of atoms.

It explained, through thermodynamics and atomic physics, why the spectral lines of different elements appear or disappear in stellar atmospheres. It is counted among the foundational equations of modern astrophysics.

A scientist in public life

Saha taught and researched at the universities of Allahabad and Calcutta, built scientific institutions and journals, took an interest in river planning and national science policy, and later became a Member of Parliament. The Saha Institute of Nuclear Physics carries his name.

He is one of the earliest examples of a scientist with a public-policy role: scientific knowledge, his life suggests, is not separate from public policy.

Sources