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https://quizlet.com/4936454/astronomy-exam-ii-flash-cards/
phase of a high-mass star: iron cannot provide fusion energy, so it accumulates in the core until the degeneracy pressure can no longer support it and the core collapses neutron star, black hole phase of a high-mass star: the core's collapse forms a ball of neutrons, which may remain as a ___ or collapse further to make a ___
https://quizlet.com/17364613/astronomy-13-flash-cards/
There is a mass limit for a star in the white-dwarf phase, the Chandrasakhar limit, beyond which the electron degeneracy pressure can no longer support the star against its own gravity.
https://afrinewz.com/how-do-stars-explode/
Jan 06, 2020 · Supernovas can occur in one of two ways: through a process of runaway nuclear fusion or through a rapid collapse of the star’s core. The first process occurs in binary star systems where at least one star is a white dwarf, a dense, aging star that can no longer support nuclear fusion.The second star can be another white dwarf, a red giant, or a main sequence star such as our own Sun, that ...
https://www.reddit.com/r/EverythingScience/comments/ekune0/stars_explode_in_one_of_two_ways_through_a/
Stars explode in one of two ways: through a process of runaway nuclear fusion or through a rapid collapse of the star’s core. The first process occurs in binary star systems where at least one star is a white dwarf, a dense, aging star that can no longer support nuclear fusion.
https://quizlet.com/12337430/stars-flash-cards/
Some massive star supernovae can make black hole if enough mass falls onto core, Neutron degeneracy pressure can no longer support a neutron star against gravity if its mass exceeds about 3Msun Some massive star supernovae can make black hole if enough mass falls onto core Beyond the limit no known force can resist the crush of gravity
https://en.wikipedia.org/wiki/Compact_star
Formation. The usual endpoint of stellar evolution is the formation of a compact star.. Most stars will eventually come to a point in their evolution when the outward radiation pressure from the nuclear fusions in its interior can no longer resist the ever-present gravitational forces.
https://quizlet.com/58951467/vocab-13-flash-cards/
This is the glowing core that forms when a star can no longer support itself by fusion reactions in its center. It is the final episode in the existence of a star. solar eclipse. This occurs when the Moon passes between the Sun and the Earth so that the Sun is completely or partially obscured.
https://quizlet.com/81170264/the-death-of-stars-flash-cards/
There is a mass limit for a star in the white-dwarf phase, the Chandrasakhar limit, beyond which the electron-degeneracy pressure can no longer support the star against its own gravity. This mass limit is
https://science.nasa.gov/astrophysics/focus-areas/how-do-stars-form-and-evolve
Having achieved iron, the star has wrung all the energy it can out of nuclear fusion - fusion reactions that form elements heavier than iron actually consume energy rather than produce it. The star no longer has any way to support its own mass, and the iron core collapses.
https://www.coursehero.com/file/p6tdin2/Main-sequence-stars-that-can-no-longer-support-nuclear-fusion-of-hydrogen-in/
Main sequence stars that can no longer support nuclear fusion of hydrogen in their cores will become red giant stars STAR CLUSTERS -all formed at the same time -all the same age in cluster -all the same composition in cluster -all the same distance from us The only difference between stars in …
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