Research news on Stellar evolution

Stellar evolution as a research area investigates the physical processes governing the formation, structural changes, and end states of stars across cosmic time, using stellar structure theory, nuclear astrophysics, hydrodynamics, and radiative transfer. It encompasses modeling of protostellar collapse, main-sequence hydrogen burning, post–main-sequence shell burning, and advanced nucleosynthesis up to core collapse or thermonuclear disruption, as well as mass loss, rotation, magnetic fields, and binary interactions. The field integrates observations (e.g., HR diagrams, asteroseismology, stellar populations) with numerical simulations to constrain stellar lifetimes, remnant formation (white dwarfs, neutron stars, black holes), and the chemical and energetic feedback of stars into galaxies.

The universe's most powerful telescope

SN 2025mkn is a Type II supernova and it wasn't supposed to be visible at all. The violent death of a massive star that had exhausted its nuclear fuel and collapsed under its own gravity sits at a redshift of 1.371. That ...

Two's company: Scientists identify new class of star remnants

In about 5 to 8 billion years, our sun is expected to evolve into a white dwarf—an extremely dense, Earth-sized stellar remnant that has exhausted its fuel and shed its outer layer. But while our sun is a solitary star, research ...

The most pristine star yet found in the known universe

An unusual team of astronomers used Sloan Digital Sky Survey-V (SDSS-V) data and observations on the Magellan telescopes at Carnegie Science's Las Campanas Observatory in Chile to discover the most pristine star in the known ...

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