Added: 2 years ago
From: yoonoose
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  • Recent work seems to refute this. A "killer SN" needs to be within a few tens of light years. Search for "supernova danger Brian fields" (He has worked on this subject.)

  • PTF11kly Super Nova IA in m101

  • @thiagokeizo exactly! :)

  • IK Pegasi is only 150 LY from us and this will most likely happen when the primary star goes red giant.  We need to be 3000 ly or farther to be safe

  • @JeremysRants Yes! seems like a supernova radiation threat in near future (I mean millions of years :)) better to start to build a magnetic shield for the planet against the burst of high-energetic radiation.

  • What happened to the other star? Could it survive?

  • @rottencranberry google for "SN 1572" you'll find much information taken from a real sample :)

  • @rottencranberry and find the page "APOD: 2011 April 30 - Tycho's Supernova Remnant" and look for the link on text "What exploding white dwarf star" there is the page of Chandra's good explanation about that sample supernova too

  • @yoonoose Thank you, i't makes much more sense now. There is a whole universe out there you know...

    Best regards.

  • @rottencranberry :) my pleasure.

    best wishes

  • @rottencranberry yes the other star survive only lost the serupefial area

  • Which caused which?

  • @vap0rxt this is an example to the evolution of binary stars

  • @yoonoose I was wondering, as the white dwarf is exploding, it brightens, dims and THEN explodes. Why is there that dip in brightness?

  • @05swanbe good question. that first flash must represent a different burning or fusion process of elements from the collapsed gas and then when this runs off, it contracts and the core gets hotter for the actual fusion process for the explosion. First trigger for carbon element and then gets hotter for burning (fusing) the oxygen and goes on for heavier elements. These are what told in the "Type Ia supernova" entry in wikipedia, and I guess this seconds in the animation represent that steps.

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