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#21
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Two white dwarf stars orbiting each other every five minutes,confirmed
Brad Guth wrote:
Plus attracted to one another by their magnetic forces (especially if poles flip) which can be rather considerable. Magnetic attraction is balanced out by magnetic repulsion. The only thing magnetism will serve to do is tidally lock them into position quicker. Gravity is the only force at work here. Yousuf Khan |
#22
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Two white dwarf stars orbiting each other every five minutes,confirmed
On Mar 14, 6:32*am, Yousuf Khan wrote:
Brad Guth wrote: Plus attracted to one another by their magnetic forces (especially if poles flip) which can be rather considerable. Magnetic attraction is balanced out by magnetic repulsion. The only thing magnetism will serve to do is tidally lock them into position quicker. Gravity is the only force at work here. * * * * Yousuf Khan Gravity is an extremely weak force. Those white dwarfs have a lot going for them, except having too few of those repulsive elections to keep themselves apart. One pole flip and it's magnetic attraction of that pair of perhaps 1e6 gauss stars merging very quickly. ~ BG |
#23
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Two white dwarf stars orbiting each other every five minutes,confirmed
Brad Guth wrote:
Gravity is an extremely weak force. Those white dwarfs have a lot going for them, except having too few of those repulsive elections to keep themselves apart. One pole flip and it's magnetic attraction of that pair of perhaps 1e6 gauss stars merging very quickly. Let's not forget how magnetic attraction and repulsion actually work: the poles actually have to point towards each other. The poles in stars are usually aligned parallel to each other. There is no net attraction or repulsion there. It wouldn't matter if one star's pole is north and the other star's pole is south, when they are parallel. There are localized attractions and repulsions which would serve to sync up the two stars' rotations with each other, but once synchronized, nothing further happens. Yousuf Khan |
#24
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Two white dwarf stars orbiting each other every five minutes,confirmed
On Mar 15, 3:32*pm, Yousuf Khan wrote:
Brad Guth wrote: Gravity is an extremely weak force. Those white dwarfs have a lot going for them, except having too few of those repulsive elections to keep themselves apart. One pole flip and it's magnetic attraction of that pair of perhaps 1e6 gauss stars merging very quickly. Let's not forget how magnetic attraction and repulsion actually work: the poles actually have to point towards each other. The poles in stars are usually aligned parallel to each other. There is no net attraction or repulsion there. It wouldn't matter if one star's pole is north and the other star's pole is south, when they are parallel. There are localized attractions and repulsions which would serve to sync up the two stars' rotations with each other, but once synchronized, nothing further happens. * * * * Yousuf Khan You need to play with magnets before you assume anything, especially about white dwarf stars that could represent 1e6 gauss each. Try to orbit powerful magnets in open space as a simulation, such as within the zero delta V of our moon-Earth L1(Selene L1). Whatever you do, don't place yourself in the center. The natural order of magnetic items is to join up or merge together and stay that way. ~ BG |
#25
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Two white dwarf stars orbiting each other every five minutes,confirmed
On Mar 9, 3:32*pm, Yousuf Khan wrote:
These two white dwarfs are so close together, that they might fall into each other some day. This would be an ideal test to see if two white dwarfs falling into each other produce a Type Ia supernova, leaving nothing behind. Or if they simply turn into a neutron star. * * * * Yousuf Khan *** SPACE.com -- Fastest Orbiting Stars Circle Each Other in Mere Minutes "After a decade of mystery, astronomers have now shown that a pair of white dwarf stars spin around each other in just 5.4 minutes, making them the fastest-orbiting and tightest binary star system ever found, the researchers claim. The record-setting stellar duo, known as HM Cancri or RX J0806.3+1527, offer challenges in explaining how such a system might form. The super-quick stars may also present a great future test-bed for detecting gravitational waves, which are elusive ripples in space-time."http://www.space.com/scienceastronomy/fastest-orbiting-stars-100309.html Apparently if these two eventually merge, their combined mass isn't going to trigger a supernova, instead just a normal stellar explosion of 0.01 c or less. Any ideas as to their individual gauss? ~ BG ~ BG |
#26
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Two white dwarf stars orbiting each other every five minutes,confirmed
On Mar 9, 3:32*pm, Yousuf Khan wrote:
These two white dwarfs are so close together, that they might fall into each other some day. This would be an ideal test to see if two white dwarfs falling into each other produce a Type Ia supernova, leaving nothing behind. Or if they simply turn into a neutron star. * * * * Yousuf Khan *** SPACE.com -- Fastest Orbiting Stars Circle Each Other in Mere Minutes "After a decade of mystery, astronomers have now shown that a pair of white dwarf stars spin around each other in just 5.4 minutes, making them the fastest-orbiting and tightest binary star system ever found, the researchers claim. The record-setting stellar duo, known as HM Cancri or RX J0806.3+1527, offer challenges in explaining how such a system might form. The super-quick stars may also present a great future test-bed for detecting gravitational waves, which are elusive ripples in space-time."http://www.space.com/scienceastronomy/fastest-orbiting-stars-100309.html Apparently white dwarfs can go with 2+ solar masses, so perhaps most everything we know about white dwarfs is at risk. These two little dwarfs magnetically combining would hardly make a bang, much less a supernova. ~ BG |
#27
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Two white dwarf stars orbiting each other every five minutes,confirmed
Brad Guth wrote:
Apparently white dwarfs can go with 2+ solar masses, so perhaps most everything we know about white dwarfs is at risk. These two little dwarfs magnetically combining would hardly make a bang, much less a supernova. They're talking about the combined mass of the two white dwarfs together as about 2+ Msun, not either WD individually. Of course the maximum any single WD can go upto is just slightly less than 1.4 Msun (i.e. Chandrasekhar Limit). Yousuf Khan |
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