[amp_mcq option1=”Raman Effect” option2=”Chandrasekhar limit” option3=”Aurora Borealis” option4=”Quasan Zone” correct=”option2″]<\/p>\n
The correct answer is: B. Chandrasekhar limit<\/strong><\/p>\n The Chandrasekhar limit is the maximum mass of a stable white dwarf star. Beyond this limit, electron degeneracy pressure cannot support the star against gravitational collapse.<\/p>\n The Raman effect is the inelastic scattering of light by a substance, resulting in a change in frequency of the light.<\/p>\n The Aurora Borealis, also known as the Northern Lights, is a natural light display in the sky, predominantly seen in the high-latitude regions (around the Arctic and Antarctic).<\/p>\n The Quasan Zone is a region of space that is thought to be the source of quasars. Quasars are extremely bright objects that are powered by supermassive black holes.<\/p>\n The Chandrasekhar limit is named after Indian astrophysicist Subrahmanyan Chandrasekhar, who first calculated it in 1931. The limit is approximately 1.4 solar masses, which is the mass of the Sun.<\/p>\n If a white dwarf star has a mass greater than the Chandrasekhar limit, it will collapse under its own gravity. This collapse can lead to a supernova explosion, or the formation of a neutron star or black hole.<\/p>\n","protected":false},"excerpt":{"rendered":" [amp_mcq option1=”Raman Effect” option2=”Chandrasekhar limit” option3=”Aurora Borealis” option4=”Quasan Zone” correct=”option2″]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[958],"tags":[],"class_list":["post-58344","post","type-post","status-publish","format-standard","hentry","category-world-geography","no-featured-image-padding"],"yoast_head":"\n