Gregory Thomas
Gregory
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A white dwarf is a dense and faint stellar remnant that results from the evolution of low-mass stars. Learn about the history, properties, and types of white dwarfs, and see some of the nearest and brightest ones in the sky.
Jul 26, 2024 · Learn about white dwarf stars, the dense and compact remnants of intermediate- and low-mass stars that have exhausted their nuclear fuel. Find out how they are supported by degeneracy pressure, what their mass-radius relationship is, and what their evolution and fate are.
- The Editors of Encyclopaedia Britannica
Apr 25, 2023 · White dwarfs are the hot, dense cores of dead stars that mark the final stage of evolution for most stars, including our sun. Learn how they are born, what they are made of, and how they can explode or fade away in this astronomy essentials article.
Mar 4, 2022 · Learn how white dwarfs are formed, what makes them so dense and what will happen to them in the future. Find out how some white dwarfs have rocky material falling into them and how they may explode as supernovas.
Learn about the dense and ancient stars that result from the end of hydrogen fusion in smaller stars. Discover how white dwarfs evolve, cool, and sometimes explode in supernovas.
Jun 12, 2020 · A white dwarf star is a dense and compact stellar remnant that emits thermal energy from its core. Learn about its formation, characteristics, examples, and how it differs from other types of stars.
Learn how white dwarfs and neutron stars are formed from the death of stars, and how they affect the universe with their gravity, radiation, and chemistry. Explore the research topics and projects of Center for Astrophysics scientists on these compact objects.
