100 Billion SunsThe Birth, Life, and Death of the Stars
Kippenhahn — a German astrophysicist who spent a working life on stellar models at Max Planck — writes the book he wished he could have given his younger self. The shape is biographical: a star is born from a collapsing cloud, lights its fusion fire, lives by a careful balance between gravity pulling inward and radiation pushing outward, exhausts its fuel in a sequence the chemistry of nuclei makes precise, and ends — depending only on its mass — as a quiet white dwarf, a violent supernova, a neutron star, or a black hole. The exposition is patient, the analogies are German-precise, and the chapters on the late stages of massive stars are still, decades later, one of the best non-technical accounts available. The Chinese translation has kept its dignity.
If you read only one book on stars, this is still it. The physics has not aged because the physics it describes is the slow physics — nuclear binding energies, hydrostatic equilibrium, electron degeneracy — that does not move.
A star's mass at birth writes its obituary in advance.