Minimum safe distance from a supernova?

You are standing in a spacesuit on a 100 km diameter rock orbiting a star of 10 solar masses. The rock is tidally locked to the star. The star has no companion. The star explodes in a supernova. There is no gamma ray burst. How far away from the star for you to survive does the rock have to be if you are on the near side of the rock? How about the far side?

30 light years isn’t enough.

That’s a whole different kettle of fish, one which is not relevant to my OP.

A supernova is about 10 billion times brighter than a star. The sun is comfortable at Earth’s distance, but if it were 10 times brighter it would be lethal in a normal spacesuit–you’d quickly overheat. So you need to be at least sqrt(1000000000) = 32,000 AU away, or about half a light year. I think I might want the full light year for a bit more comfort.

In related news, you’ll get a lethal dose of neutrino radiation poisoning at 2.3 AU.

This guy, Michael Richmond, crunched a lot of the numbers for you. Original page doesn’t work anymore, hence the archive.org link.

Highlights:

If you’re close enough to be tidally locked, you’re probably in the supernova.

Guys, for this thread I’m not interested in the effect of life on Earth; I am interested on the astronaut in the spacesuit on the rock.

But isn’t a supernova a near-flash or wave which quickly passes you? A camera flash is from hundreds of thousands to millions of lumens.

How about being on the far side of the rock?

Rocks don’t protect against neutrinos, so adding a fudge factor for safety we’re looking at a distance of Jupiter for neutrinos.

I’m sorry; I should have read further:

That’s insane. But then we’re dealing with insane energies.

The “supernova at 1AU vs H-bomb against the eye comparison” is one of my all time favorites.

Especially the illustration and its popup text, which says “Can you hurry up and set it off? This is heavy.” After reading that, I suddenly noticed the “motion lines” around the bomb, which are clearly intended to convey the impression that the poor stick figure is trembling while struggling to hold that thing up against his eye.

(Warning: both links below are directly to PDF files)

That may be a little close, since the “What If?” article uses results from Andrew Karam’s calculations, and in the referenced paper, Karam says:

And, you know, if you’re just talking about distance-of-Jupiter instead of parsecs, something completely insignificant could become significant…

(The paper by Collar can be found here. I couldn’t find a copy of the Cossairt and Marshall comment on his paper, nor his reply to them, that wasn’t behind a paywall.)

I think it’s safe to say that any rock orbiting the star before it goes supernova would be toast … standing on the far side is of little protection if your rock is suddenly vaporized … even the furthest reaches of the planetary system would be bombarded with solar innards … an iron atom traveling at the speed of light packs a punch … and we’ll have a gaggle of heavy atoms hitting us …

We’d be better off orbiting the next star over …

“Quickly”, in this context, means a few months.

And even that might be too close.