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The Action of the dying Sun
Why does the sun expand out as far as Jupiter before it contracts all
the way back to becoming a White Dwarf? Our sun would end up as a neutron star if it had 50% more mass. A star with to much mass is not beneficial for life. I don't think rock planets could form if their sun only lasted for 100 million years. Lets go with that supermassive star Eta Carinae it had a giant outburst,and released as much energy as a supernova. This star is still around. Hmmmm How did it survive that explosion? Astronomers estimate its mass to be 100 times that of the sun. With that mass it should end up as a blackhole. It could be the seed for another mini-bang that will reach a critical mass,and the moment it stops spinning its horizon will collape into the core,and release its singularity. to create a mirror image of the universe it was recycled from.(I love that idea) Bert |
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"G=EMC^2 Glazier" ha scritto nel messaggio
... Why does the sun expand out as far as Jupiter before it contracts all the way back to becoming a White Dwarf? Our sun would end up as a neutron star if it had 50% more mass. A star with to much mass is not beneficial for life. I don't think rock planets could form if their sun only lasted for 100 million years. Lets go with that supermassive star Eta Carinae it had a giant outburst,and released as much energy as a supernova. This star is still around. Hmmmm How did it survive that explosion? Astronomers estimate its mass to be 100 times that of the sun. With that mass it should end up as a blackhole. It could be the seed for another mini-bang that will reach a critical mass,and the moment it stops spinning its horizon will collape into the core,and release its singularity. to create a mirror image of the universe it was recycled from.(I love that idea) Bert What about if Eta Carinae will become a gravastar? Or this theory is completely wrong? Luigi Caselli |
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Hi Casselli I never heard of a "gravastar" Sounds interesting please
explain. Bert |
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"G=EMC^2 Glazier" ha scritto nel messaggio ... Hi Casselli I never heard of a "gravastar" Sounds interesting please explain. Bert It's an interesting new theory a bit difficult to believe (not more than black holes...) You can see a rapid overview at http://www.space.com/scienceastronom...rs_020423.html "Emil Mottola of the Los Alamos National Laboratory and Pawel Mazur of the University of South Carolina suggest that instead of a star collapsing into a pinpoint of space with virtually infinite gravity, its matter is transformed into a spherical void surrounded by an extremely durable form of matter never before experienced on Earth." "The matter inside a gravastar would be akin to the Bose-Einstein condensate. It would exist in a vacuum, surrounded by an ultra-thin, ultra-cold, ultra-dark bubble, hence the name gra (vitational) va (cuum) star, or gravastar." I like this theory because I've always hated singularities, they bring too much entropy in our universe... .. Luigi Caselli |
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nightbat wrote
Luigi Caselli wrote: "G=EMC^2 Glazier" ha scritto nel messaggio ... Hi Casselli I never heard of a "gravastar" Sounds interesting please explain. Bert It's an interesting new theory a bit difficult to believe (not more than black holes...) You can see a rapid overview at http://www.space.com/scienceastronom...rs_020423.html "Emil Mottola of the Los Alamos National Laboratory and Pawel Mazur of the University of South Carolina suggest that instead of a star collapsing into a pinpoint of space with virtually infinite gravity, its matter is transformed into a spherical void surrounded by an extremely durable form of matter never before experienced on Earth." "The matter inside a gravastar would be akin to the Bose-Einstein condensate. It would exist in a vacuum, surrounded by an ultra-thin, ultra-cold, ultra-dark bubble, hence the name gra (vitational) va (cuum) star, or gravastar." I like this theory because I've always hated singularities, they bring too much entropy in our universe... . Luigi Caselli nightbat Yes, Luigi, slowly many are coming around to nightbat's " Black Comet " profound resolution for black hole paradox. Many scientists have been getting clues from us net Mavericks for quite some time now. Glad you like the fact simile gravastar to original nightbat no hole in space idea over a more credible extremely dense neutron star class one going over Chandra limit and metamorphosing into super plasma state. Funny, ha, ha, as soon as they get a clue and immediately try to name and claim it as theirs, they get caught and dated and try to do a patch up job of playing catch up. Unless you have the right working model you're out in left field. Too much entropy, ha, ha, it was always there just imbedded in the quantum space fabric (VED). Bert speculates in his " what if " posts that the Earth was hit by a comet. I have tried to explain to him that the Earth was a " Black Comet ". The large Oort cloud and high momentum broken off smaller ice comets are some of the remains of the blown away outer core shell of the Black Comet as it came into its galactic dispersed normal gravity restabilization position. Ever wonder how white comets have so much power, ha, ha, it's all in the remaining super condensed plasma gas. the nightbat |
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"G=EMC^2 Glazier" wrote in message
... Why does the sun expand out as far as Jupiter before it contracts all the way back to becoming a White Dwarf? Our sun would end up as a neutron star if it had 50% more mass. "The stars that eventually become neutron stars are thought to start out with about 15 to 30 times the mass of our sun." http://www.astro.umd.edu/~miller/nstar.html#formation A star with to much mass is not beneficial for life. I don't think rock planets could form if their sun only lasted for 100 million years. Lets go with that supermassive star Eta Carinae it had a giant outburst,and released as much energy as a supernova. This star is still around. Hmmmm How did it survive that explosion? Astronomers estimate its mass to be 100 times that of the sun. With that mass it should end up as a blackhole. It could be the seed for another mini-bang that will reach a critical mass,and the moment it stops spinning its horizon will collape into the core,and release its singularity. to create a mirror image of the universe it was recycled from.(I love that idea) Bert |
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JohnZ Read that book again. In my book (just studied it),and it tells
me a star with 1.4 mass greater than the sun would end up as a neurton star. However JohnZ we should stop throwing books at each other,and discuss things. You started it so you have to end it.. My books are heavier than yours,and I can add more pages to it for sure. Bert |
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"G=EMC^2 Glazier" wrote in message
... JohnZ Read that book again. In my book (just studied it),and it tells me a star with 1.4 mass greater than the sun would end up as a neurton star. However JohnZ we should stop throwing books at each other,and discuss things. You started it so you have to end it.. My books are heavier than yours,and I can add more pages to it for sure. Bert Nonsense. Your "Heavy Books" probably say something like "a Neutron Star is about 1.4 solar masses". A Neutron Star does not contain the entire mass of its progenitor. I suggest you take a closer look at your "Heavy Books". |
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"G=EMC^2 Glazier" wrote in message
... JohnZ Read that book again. In my book (just studied it),and it tells me a star with 1.4 mass greater than the sun would end up as a neurton star. "It is believed that the remnant of a core collapse SN is a neutron star if the mass of the progenitor is less than ~ 20-25M(Sun) [80, 78]. If the progenitor's mass is in the range 20-25 ~ M ~ 40-50M(Sun), not the entire star is ejected in the SN explosion. More than 2M(Sun) will fall back onto the nascent neutron star and lead to black hole formation. If the progenitor's mass exceeds roughly 40-50M(Sun), then no explosion will occur and the star will collapse directly to a black hole. These objects are known as collapsars. However, it is unclear if high metallicity stars with M ~ 40-50M(Sun) actually end their lives in collapse or are prevented from doing so by stellar wind driven mass loss [78]. Note that the limits on the progenitor masses quoted in this paragraph (especially the 40-45M(Sun), lower limit for direct black hole formation) are uncertain because the progenitor mass dependence of the neutrino explosion mechanism (see below) is unknown [88, 150]." http://www.emis.de/journals/LRG/Arti...new/node9.html However JohnZ we should stop throwing books at each other,and discuss things. You started it so you have to end it.. My books are heavier than yours,and I can add more pages to it for sure. Bert |
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JohnZ Using far less words than you because the books I read come
right to the point. The Chandrasekhar mass is roughly 1.4 suns,and just above this limit gravity squeezes the electrons and protons together. We call this density a neutron star. Yes I do have the book and page number. Well I do know a neutron star has 3 times less mass than a blackhole. So that might help your saying 40 times a sun mass.(hopefully) JohnZ why do you have to always be negative? Bert |
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