Pair-instability supernova calculation

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Pair-instability supernovae are significantly brighter than typical supernovae, with calculations indicating they can be 600 billion times brighter than their ancestor stars. The apparent magnitude of such a supernova, calculated as -29.5 when the ancestor star's magnitude is 0, is correct but requires consideration of distance. The apparent magnitude is inversely proportional to the square of the distance from the observer, necessitating a comparison between the distances of the ancestor star and the supernova. This results in an unusually high apparent magnitude, even exceeding that of the Sun. The discussion highlights the potential for such distant stars to influence conditions on Earth, despite their minuscule apparent size.
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Usual supernova 6 billion times brighter then ancestor star. Pair-instability supernova 100 times brighter then supernova 600 billion times brighter then ancestor star. If ancestor star apparent magnitude is 0 then apparent magnitude of pair-instability supernova from that star is = - 2.5* lg(6*10^11) = -29.5 Is my calculation correct?
 
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Yes, it is correct. I assure you, but the concept is not
the apparent magnitude depends upon the distance also. You also need to compare the distance of the ancestor star from you with the distance of supernova from you. Something like this...
Let the distance from you to ancestor star be d, and distance from you to supernova be x.
Then the apparent magnitude will be -2.5*log((6*10^11)*d^2/x^2), since it is inversely proportional to the square of distance.
That is why you are getting such an unusually high magnitude. In fact, higher than the Sun. It is -26.7.
 
It's hard to imagine that star located several thousand light Earth from solar system with so small apparent diameter just 0.00001'' can potentially create on Earth Mercury weather
 
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