arjan de lumens said:Hmmm, better not confuse "astrologists" with "astronomers" - I suspect both groups would be rather offended by being associated with the other one.
No it doesn't!ANova said:It literally destroys whole galaxies;
No we don't!astronomers call these Death Stars.
That "simulation" is regarded with a great deal of scepticism by anyone with a serious scientific background (it's little more than a bunch of assumptions coddled together with numbers plucked from the air). The media love it of course, because it's gigadeath!A simulation has been created of what would happen to Earth if the closest star to this galaxy went hypernova, and although it wouldn't destory the planet, rest assured nothing would survive.
arjan de lumens said:While GRBs can release large amounts of energy, the vast majority of the energy is apparently beamed out from its poles, and if you are not within that beam, the GRB looks rather unremarkable. This means that early estimates of the actual power in a GRB are now considered vast overestimates.
Incidentally, if you're afraid of GRBs, check out a star named "Eta Carinae". It is a notoriously volatile blue giant star ~7000 light years away from us. This star is the heaviest star known to man at ~150 solar masses and is expected to go hypernova/GRB on us very soon now (well, "very soon" on an astronomical timescale, which could still mean thousands of years).
AFAIK, current estimates of GRB power indicate that if Eta Carinae goes GRB straight on Earth, it is still too far away to do serious damage to our atmosphere (if it was closer, like, say 1000 light years, then it would be quite deadly, but 7000 light years is believed to be rather safe), so to us people on the ground it will probably just be a spectacular light show.K.I.L.E.R said:Arjan, wouldn't the resulting GRB destory our atmosphere?
That I actually don't know. Looking directly into an ongoing GRB might pose dangers similar to looking directly into a solar eclipse (usually small permanent blind spots rather than general blindness), but the actual GRB itself only lasts for a few seconds, after which it should be fairly safe to look at it.K.I.L.E.R said:Wouldn't the people looking at the light show go blind or would our atmosphere protect us from it?
nutball said:No it doesn't!
No we don't!
That "simulation" is regarded with a great deal of scepticism by anyone with a serious scientific background (it's little more than a bunch of assumptions coddled together with numbers plucked from the air). The media love it of course, because it's gigadeath!
ANova said:Ninety somewhat percent of our understanding of the universe and our existence comes from assumptions. Some believe it, even though you may not. True, none of it may be correct, but we won't know until it happens, assuming it ever does.
Hmm, I only get an apparent magnitude of -7.7; my workings could be totally wrong of course but I first calculated 990123's absolute magnitude by using M = m-5(log10D-1) where m is the apparent magnitude, D is the distance in parsecs and M is the absolute magnitude. So if 990123 had an apparent mag of +9 at a distance of 7Gpc, then M = 9-5((log10 x 7 x 10^6)-1) = -20.2 I know that one has to use luminosity distance for objects further away than, say, 10~50kpc but I'm assuming that nutball's figure for 990123 is the lum dist! Anyway, if -20.2 is right and eta carinae is the same, then one can find the apparent magnitude in reverse; m = M+5(log10D-1) = -20.2+5((log10 x 3.2 x 10^3))-1) = -7.7arjan de lumens said:OK, then we can do some (rather speculative) math. If we assume that Eta Carinae will reach the same strength as 990123, then: 990123 is placed about 10^6 times times farther away than Eta Carinae, so the light intensity of an Eta Carinae GRB will be about 10^12 times stronger (light intensity falls off by about square of distance). 1 "magnitude" in astronomy corresponds to a factor of 2.512, so Eta Carinae would be ~30 magnitudes stronger than 990123, as seen from Earth, placing its apparent magnitude around -21 - not quite as strong as the mid-day Sun (-26), but much stronger than the full Moon (-12). Given that Eta Carinae due to distance would take up a much smaller section of the sky than the Sun, I suspect that if you are unlucky enough to look directly at it at the peak of such a burst, you would get a small permanent burn scar on your retina.
Coming first with a bunch of doomsaying, then hiding behind the "we cannot know" shield, strikes me as useless fearmongering.ANova said:Ninety somewhat percent of our understanding of the universe and our existence comes from assumptions. Some believe it, even though you may not. True, none of it may be correct, but we won't know until it happens, assuming it ever does.
Ligt intensity falls off as 1/distance^2, not 1/distance.Neeyik said:Hmm, I only get an apparent magnitude of -7.7; my workings could be totally wrong of course but I first calculated 990123's absolute magnitude by using M = m-5(log10D-1) where m is the apparent magnitude, D is the distance in parsecs and M is the absolute magnitude. So if 990123 had an apparent mag of +9 at a distance of 7Gpc, then M = 9-5((log10 x 7 x 10^6)-1) = -20.2 I know that one has to use luminosity distance for objects further away than, say, 10~50kpc but I'm assuming that nutball's figure for 990123 is the lum dist! Anyway, if -20.2 is right and eta carinae is the same, then one can find the apparent magnitude in reverse; m = M+5(log10D-1) = -20.2+5((log10 x 3.2 x 10^3))-1) = -7.7
I know but I don't think your calcs are right with the figures though - distance to 990123 is 7 x 10^6 pc whereas EC is about 3.2 x 10^3 pc. So with I being proportional to 1/d^2 then that puts the ratio of intensities of Iec/I99 = (1/Dec^2)/(1/D99^2) = D99^2/Dec^2 = (7x10^6)^2/(3x10^3)^2 = 4.8x10^6 which seems quite different to 10^12. I don't think that I've made a mistake here but my astrophysics, even basic stuff, is pretty rusty!arjan de lumens said:Ligt intensity falls off as 1/distance^2, not 1/distance.
Umm, no. The numbers that nutball stated and I have been able to find on the distance to GRB 990123 are on the order of 10^9 parsecs, not 10^6.Neeyik said:I know but I don't think your calcs are right with the figures though - distance to 990123 is 7 x 10^6 pc whereas EC is about 3.2 x 10^3 pc. So with I being proportional to 1/d^2 then that puts the ratio of intensities of Iec/I99 = (1/Dec^2)/(1/D99^2) = D99^2/Dec^2 = (7x10^6)^2/(3x10^3)^2 = 4.8x10^6 which seems quite different to 10^12. I don't think that I've made a mistake here but my astrophysics, even basic stuff, is pretty rusty!
I merely asserted one possibility which I think has some relevency, however I can't pretend to know as fact and neither can you or nutball.arjan de lumens said:Coming first with a bunch of doomsaying, then hiding behind the "we cannot know" shield, strikes me as useless fearmongering.
Doh! I'd even read the darn distance right as being 7Gpc but in my head, used it as 7Mpc - lo and behold, you get -22.7 for m when use it right!arjan de lumens said:Umm, no. The numbers that nutball stated and I have been able to find on the distance to GRB 990123 are on the order of 10^9 parsecs, not 10^6.