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Published byEarl Bailey Modified over 6 years ago
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HOW DO STARS DIE ? MAYUMI BARCENA AND JASMIN DE LEON
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STARS massive SUN
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end of productive phase Chandrasekhar Limit
WHITE DWARF
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CHANDRASEKAHAR LIMIT stable white dwarf 1.4 Subrahmanyan Chandrasekhar
Wilhelm Anderson and E.C. Stoner the limit,ignored logically require black hole
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NEUTRON STAR created,4-8 solar masses undergo supernova explosion remaining protons and electrons
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SUPERNOVA stellar explosion radiating energy Sun expected to emit before fading hydrogen fusing
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SUPERNOVA
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BLACK HOLE condense to black hole region of spacetime
prevents anything stellar masses continue to grow supermassive black holes
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BLACK HOLE
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REFERENCES en.wikipedia.org/wiki/Chandrasekhar_limit
en.wikipedia.org/wiki/Black_hole en.wikipedia.org/wiki/Subrahmanyan_Chandrasekhar imagine.gsfc.nasa.gov/docs/ask_atro/answers/010607a.html chandra.harvard.edu/resources/illustrations/stellar_evolution._html sky_is_full_of_shinning_stars_the_moon_walking_soft_and_gentle_light_wish_one_good_sleep_hd_natural_scenery_walpaper/ en.wikipedia.org/wiki/star en.wikipedia.org/wiki/Sun en.wikipedia.org/wiki/Neutron_star venturegalleries.com/blog/finding_my_writing_place_in_the_universe/
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