How stars work, and how they die.
11 topics · 10 curated works
Assumes you know the vocabulary.
Periods of 25 Variable Stars in the Small Magellanic Cloud
Henrietta Swan Leavitt · 1912
Shows that brighter Cepheid variable stars have longer pulsation periods in a tight relation, giving astronomy its first reliable way to measure…
+1 more at this level
Primary sources and full treatments.
The Internal Constitution of the Stars
Arthur Stanley Eddington · 1926
Works out how pressure, temperature and radiation balance inside a star, establishing the mass-luminosity relation and treating stars as gas spheres…
+7 more at this level
10 works
Henrietta Swan Leavitt
Shows that brighter Cepheid variable stars have longer pulsation periods in a tight relation, giving astronomy its first reliable way to measure distances beyond the solar neighbourhood.
link checked 17 Sept 2026Prsa et al.
Builds the first large, uniformly processed catalogue of eclipsing binary light curves from Kepler, turning binary star census-taking into a data-mining problem.
link checked 17 Sept 2026Arthur Stanley Eddington
Works out how pressure, temperature and radiation balance inside a star, establishing the mass-luminosity relation and treating stars as gas spheres governed by physics rather than mystery.
link checked 17 Sept 2026S. Chandrasekhar
Derives a firm upper mass limit above which a white dwarf cannot support itself against gravity, the boundary that decides whether a dying star becomes a white dwarf or something more violent.
link checked 17 Sept 2026Baade & Zwicky
Coins the term supernova to separate it from the ordinary nova, and proposes that such an explosion could leave behind a star made almost entirely of neutrons.
link checked 17 Sept 2026Oppenheimer & Snyder
Works through the collapse of an idealised massive star under general relativity and shows it does not stop at any finite radius, the first calculation of what would later be called a black hole.
link checked 17 Sept 2026Edwin E. Salpeter
Derives the distribution of stellar masses at birth from observed luminosities, giving stellar evolution theory the initial mass function it still uses today.
link checked 17 Sept 2026Burbidge, Burbidge, Fowler & Hoyle
Argues that nearly every element heavier than helium was forged inside stars by a specific sequence of nuclear processes, not created all at once at the beginning of the universe.
link checked 17 Sept 2026Hewish et al.
Reports a radio signal pulsing with millisecond precision, the discovery that revealed pulsars and, with them, the first direct evidence for neutron stars.
McKee & Ostriker
Reviews how molecular clouds collapse into stars and argues that turbulence and feedback, not simple gravitational collapse, set the pace and efficiency of star formation.
link checked 17 Sept 2026