Astronomers Awaiting 1a Supernova 204
Aryabhata writes to tell us BBC News is reporting that astronomers have sighted a star on the brink of a "1a" supernova. This opportunity presents the first chance astronomers have ever had to view a supernova of this magnitude up close. From the article: "They are so rare that the last one known in our galaxy was seen in 1572 by the great Danish astronomer Tycho Brahe, who first coined the term nova, for "new star", not realizing he was in fact witnessing the violent end of an unknown star. It has long been believed that type 1a supernovae are the death throes of a white dwarf star. But all modern ones have been so distant that it has not been possible to see what had been there beforehand."
How long?!? (Score:3, Interesting)
Wait for it... (Score:5, Funny)
Re:Wait for it... (Score:2)
This is old news (Score:2)
That's nice (Score:5, Funny)
From TFA:
But soon, RS Oph could pass the tipping point - the nuclear flame will detonate from deep inside the star and blow it apart. How soon is not clear.
"It could be tomorrow, but most likely it'll be 1,000, 10,000, 100,000 years from now," says Jeno Sokoloski.
Wow that's some long life astronomers. I wonder if they will be around to see DNF getting release.
Stupid headline.
Meh, I mean come on (Score:5, Funny)
Re:Meh, I mean come on (Score:2)
Re:Meh, I mean come on (Score:2)
After all it could be released tomorrow, or in a 1000 years, or 10000 or a 100000...
Re:Meh, I mean come on (Score:2)
Rho Casspiopiae (Score:5, Informative)
Coincidentally, two other supernovas have ocurred in that area, one of which was the one Tycho Brahe saw. Keep an eye on the hypergiants (see: Wikipedia's explanation of how stars are classified [wikipedia.org])
Re:Rho Casspiopiae (Score:5, Informative)
Because type 1a SN are believed to occur under nearly identical circumstances, they are considered especially important in astronomy. Astronomers believe that they can be used as what they call "standard candles." A "standard candle" is a light source of known brightness. Standard candles are important, because astronomers can directly determine the distance of these sources. Certain stars already act as standard candles, but stars can only be resolved at a certain distance. A type 1a SN can be seen at such a large distance that astronomers believe they can more accurately determine cosmoloigical properties if they can determine exactly how bright one is, and how it may fluctuate under different circumstances.
Other SN are interesting, but a Type 1a SN in our galaxy might tell us a lot about the entire universe indirectly.
Re:Rho Casspiopiae (Score:2)
Further explanation? (Score:2)
Re:Further explanation? (Score:5, Informative)
The utility of type 1a supernovae is that they are all produced by white dwarf stars exploding. White dwarfs are roughly earth-sized stellar cores that have no thermonuclear reactions going on inisde - they are the remnants of stars between about 1 and 5 solar masses after the outer layers have been blown off.
The imporant point is that the gravity of the stellar core's mass is not counteracted up by the pressure of the thermonuclear reactions inside. Rather, something called degenerate electron pressure holds the white dwarf up and prevents it from collapsing. Degenerate electron pressure can only counteract gravity for masses up to 1.4 solar masses, meaning that any white dwarf that somehow grows to a mass greater than 1.4 solar masses (usually by grabbing mass from a companion star), it will collapse. The collapse catastrophically increases the pressure inside the white dwarf, re-igniting nuclear fusion, and produces a sudden violent explosion.
Because white dwarfs are all of the same mass when they explode - 1.4 solar masses (the Chandrasekhar (sp?) limit - they are all of roughly the same brightness (>10^9 times as bright as the Sun). Because of this, one only has to see a type 1a supernova to deduce from the apparent brightness the distance from earth to the explosion. If a type 1a supernova occurs inside a cluster of stars, it conveniently tells us the distance from here to that cluster of stars. Because the distances over which supernova can be observed is orders of magnitude greater than most other stellar phenomena, the are essential in determining distances to faraway objects (from 1 to 1000 megaparsecs away (1 parsec = ~3.2 light years)). Distances to other galaxies are determined this way.
They type of supernova being observed can be determined by the specatra of light coming from it. I can't recall the distinguishing characterisitics of type 1a supernova, but suffice it to say they can be distinguished from other types of supernova.
Re:Further explanation? (Score:2)
1Mpc is about 3 million light years. So if we see light that is 3 million years old, the object that emi
Re:Rho Casspiopiae (Score:3, Informative)
Something to add here, in regards to cosmic cartography:
Parallax can only be used to measure distances within a radius of a couple of dozen light years beyond Earth. This technique gave us the Herzprung-Russell diagram, which is basically a profile of all known type of stars in the main sequence, various combinations of age, size, color and temperature.
Cepheid variables allow us to measure distances outwards to a
Re:Rho Casspiopiae (Score:2)
100,000 years? Saw it coming. (Score:3, Insightful)
She read the
From the article: "How soon is not clear [but]
My girlfriend's lack of cynicism aside, this is one of my major problems with the science community. So much is driven by a desperate need to secure funding, that science "news", most of the time, is either hypothetical, theoretical, or so far in the future that it makes no difference to the present. In these cases, when a person finds out that no actual advance has been made, he feels both disappointed and betrayed.
I am fed up with reading...
"Newsflash: No physical reason humans cant live to be 300, once the technology arrives!" *
or
"Newsflash: the universe *might* be made up of string!" *
or
"Newsflash: in 100 billion years, this star will explode!" *
etc, when the invisible postscript to every story is:
* Now that I have your attention, please give me some more funding!
Tycho Brahe (Score:2, Funny)
*yeah, I know
"Soon" ... (Score:5, Insightful)
"Space is big. Really big. You just won't believe how vastly hugely mind-bogglingly big it is. I mean, you may think it's a long way down the road to the chemist, but that's just peanuts to space." -- the Hitchhiker's Guide to the Galaxy.
Not only are the distances vast, the times are vast too. Stars live for billions of years. One year in the lifespan of a human is roughly comparable to perhaps 70 million years in the lifespan of a star.
So when someone says "soon" in reference to a prediction of when some stellar event is going to occur, it's likely you'll have to scale up the term by roughly the same amount. "Soon" to a human generally means within/around a day or so, so scaled up to stellar times, that would be within/around 200,000 years.
I expect that by the time this supernova happens, humans will either be unbelievably technologically advanced, or they'll be extinct.
Re:"Soon" ... (Score:2)
So if something/someone doesn't kill us all in the meantime, will we be advanced enough to use this as a power source?
Re:"Soon" ... (Score:3, Insightful)
Based on the current trends it will provide just enough power for one person to travel to the corner store.
Re:"Soon" ... (Score:2, Informative)
That depends on the star though. Giant stars for example are quite short-lived (millions of years instead of billions), and the last step in the fusing process where the whole core of a star gets conver
Re:"Soon" ... (Score:2)
Re:"Soon" ... (Score:2)
Re:"Soon" ... (Score:2)
There is actually another star about to go nova that is only half the distance of RS Ophiuchi. Nobody talks about it, though, because no astronomer wants to waste time on a half-vast star.
This supernova should be interesting (Score:5, Funny)
Re:This supernova should be interesting (Score:2)
The star is 1,950 light years away? (Score:5, Interesting)
Shit.
Re:The star is 1,950 light years away? (Score:3, Interesting)
If you look at the next paragraph, things don't look so bleak.
Re:The star is 1,950 light years away? (Score:2)
Re:The star is 1,950 light years away? (Score:4, Interesting)
Re:The star is 1,950 light years away? (Score:3, Funny)
On the plus side, when it goes boom, since its type 1a we wil know _exactly_ how far away it is, and whether we're or not we're screwed.
Re:The star is 1,950 light years away? (Score:2)
Re:The star is 1,950 light years away? (Score:2)
So what?
we have seen a number of large gamma ray bursts over the decades and they deliver 1000x what a large solar flare produces. Your point was?
Re:The star is 1,950 light years away? (Score:2)
Aim matters (Score:2, Interesting)
1572 is a long time ago? (Score:2, Interesting)
Gamma Ray burst = earth fried (Score:2, Funny)
Have a nice Sunday!
Re:Gamma Ray burst = earth fried (Score:4, Interesting)
IANAExpertOnThisCrap, but... if the burst lasts less than 12 hours, at least a north-south slice of the planet would be spared. If it's just a few minutes, only half the planet would be "fried", and if the Pacific Ocean happens to be facing it, then it's only bad for the relatively small island population, but if Eurasia is facing it, that's gonna be really really bad.
Of course, that's based on the event being near the plane of the ecliptic. If the event was near a pole, then one of either the North or South hemispheres is fried, the other is spared.
I'm also assuming that the gamma rays aren't powerful enough to turn surface matter into radioactive isotopes that pollute the atmosphere and ocean, or to do that to the atmosphere itself. In that case, it's more proper to say that the Earth is poisoned, not fried.
Re:Gamma Ray burst = earth fried (Score:4, Interesting)
I think your confusing types of radiation here. Gamma rays are electromagnetic radiation and will not create radioactive isotopes no matter how intense they are. Generally, what they are going to do is ionize atoms and heat things up. Damage to biologicals from Gamma rays is via ionization and heat effects.
If there were a very intense neutron burst, that could potentially "activate" some materials, i.e. transmute them into a radioacive isotopes. However, neutron burst are not going to be something we have to worry about at this distance from the event.
Re:Gamma Ray burst = earth fried (Score:2)
Granted spallation does occur, but cross-section for knocking nucleons out of a nucleus with gamma rays is vanishingly small. And secondary isotope creation from freed nucleons has to be an even smaller possibility.
Much more likely as a possibility for nucleosynthesis from Gamma rays would be beta plus decay, where a proton becomes a neutron and ejects a positron (and neutrino). But I don't think that would happen significantly either. Almost all the gamma rays are going to be absorbed via photoelectri
Re:Gamma Ray burst = earth fried (Score:2)
http://en.wikipedia.org/wiki/Gamma_ray_burst#Mass
Re:Gamma Ray burst = earth fried (Score:3, Funny)
Pain at the Pump (Re:Gamma Ray burst=earth fried) (Score:3, Funny)
It won't make gasoline more expensive, will it?
Although I'm sure technology will have advanced by then to let me use gamma rays to run my Hummer.
Re:Gamma Ray burst = earth fried (Score:2)
If we are all going to die then why did we invest in swift
http://www.nasa.gov/mission_pages/swift/main/inde
Re:Gamma Ray burst = KFG (Kentucky Fried Gaia) (Score:2)
Which begs the all-important question: Has the correlation between Type 1a Supernova and Gamma Ray Bursts been confirmed beyond a shadow of a doubt?
The way I understand the theory, which is not yet engraved in stone, if either of this star's magnetic poles are pointing towards Earth, we're gonna get zapped. However, if we're facing the star's equator, or anywhere but the poles for that matter, we're home free.
Re:Gamma Ray burst = earth fried (Score:2)
Only if you moon it. [rimshot]
First thing I thought of... (Score:2)
"May the best sentience win."
(Psst: obscure nerdy reference.)
What lag time. (Score:2)
I'll never complain about lag on IRC again!
tycho (Score:3, Funny)
from what i heard, Gabe was pretty pissed about not being invited to it. Apparently he also looked at his neighbor with a telescope ans stole a haribrush she thre out as well.
Range of lethality (Score:4, Interesting)
As far as the size of the galaxy is concerned, 1,950 light-years is essentially in our back-yard. Keeping with scale, are we talking about a firecracker or a stick of dynamite?
Re:Range of lethality (Score:5, Informative)
While this doesn't directly answer your question, you might find the following interesting. Steven Dutch, a professor at the University of Wisconsin at Green Bay has estimated what would happen if the sun were to go supernova [nagt.org]. Some highlights: the radiation flux on the daylight side of the earth would be the same as if our entire nuclear arsenal were to go off once per second at a distance of one kilometer. The reflected light from the full moon would be 10,000 times brighter than the sun; Venus would shine six times as intensely as the normal sun. The earth vaporize in a matter of days.
By the way, the sun will never become a supernova. The calculations are illustrative only.
Re:Range of lethality (Score:4, Informative)
One more thing... (Score:2)
It would be nice if we got one.... (Score:3, Interesting)
Re: (Score:3, Interesting)
Re:It would be nice if we got one.... (Score:5, Funny)
Isn't that typical. Before the telescope, there was a frickin' smorgasboard of supernovae at close range, then no sooner does man invent the telescope and the party's over, which draws me to the conclusion: I blame this supernovae drought on Galileo.
The joy of modern science (Score:2)
Wow. What incredible science. Did NewScientist buy the BBC over the weekend?
Break out the marshmallows (Score:2)
Not too close, I hope.
Actually (Score:4, Interesting)
Re:Actually (Score:4, Insightful)
What do they teach in relativity class these days?
Re:Actually (Score:4, Informative)
Suppose we send a signal towards the supernova as soon as we see it explode. Suppose that there is an observer, a really though one, staying close to the supernova as it goes off, who measures the time difference between the supernova explosion and our signal. Suppose that, as soon as he receives our signal, he sends another signal, with this data encoded, towards us. Suppose also, for simplicity, that all observers are at rest relative to each other and the supernova (they aren't really - stars move relative to each other - but that movement is too slow to cause much problems for our experiment).
Now, since light travels at a constant speed, the observer got our signal halfway between us sending it and us receiving the reply. Since both we and him are at rest relative to each other and supernova, we don't get any time dilation, and can use simple math to calculate when the nova exploded. Simply substract the time difference told to us by the other observer from the midpoint between us sending him the signal and receiving a reply. We'll arrive at a point in time somewhere before we observed the nova; whether that point is in the "distant" past or "near" past is a value judgement.
Another way of looking at this is simply understanding that light moves at a finite speed; so, if we observe the light from a distant event, that light was emitted at the moment of the event and took a nonzero time to reach us, and so the event must have happened at a nonzero time in the past.
Haven't you ever heard: the further you look in space, the further back you look in time ?
Or just read the page you linked to. It talks about causal past and future. It doesn't claim that events that we cannot yet observe due to the limited speed of light haven't yet happened, only that we can't be affected by them yet - which is pretty self-obvious, if you think about it a bit.
The Sun could have blown up 4 minutes ago, but we wouldn't know for another 4. It still blew up 4 minutes ago, it simply takes another 4 until this can be observed by us. Of course it's unlikely that the Sun would blow up suddenly, but - hey, what's that ligNO CARRIER.
Not enough, apparently. Which is a great pity, since relativity deals with the basic structure of time and space and the very nature of reality itself. It's utterly fascinating stuff, completely different from endlessly memorizing formulas and using them to calculate how much tension some wire has - that's fine for engineers, but relativity is the "actually, you can build a time machine [wikipedia.org] and warp drive [wikipedia.org]" theory and quantum mechanics are the dreams stuff is made of [physics.ubc.ca]; that is where physics education should start, to give the student the motivation to go through the grind, knowing where the basics will lead.
Re:Actually (Score:2)
Re:WRONG. (Score:2)
Re:Actually (Score:2)
Exactly.
The "time" is essentially a numerical label you can apply to events. Typically the label is chosen in such a way that an event at a higher time can't affect an event at a lower time. But when events are outside each other's light cones there are different ways to label spacetime so that in some labelings, one comes at an earlier "time" than the other, and in othe
Re:Actually (Score:5, Informative)
Welcome! (Score:3, Funny)
Re:Actually (Score:5, Informative)
Re:Actually (Score:3, Informative)
Re:Actually (Score:2, Interesting)
Re:Actually (Score:5, Informative)
http://en.wikipedia.org/wiki/Supernova#Impact_of_
So, who knows? Hollywood disaster movies might have t right after all!
Re:Actually (Score:2)
So... it's roughly 83 trips in the Millineum Falcon.
Re:Actually (Score:3, Informative)
As for effect of the light, 2000 LY is 126,000,000 AU, so if a supernova is 5 B times as bright as the sun, then it will appear to be 5e9 / 1.26e8 ^ 2 = 3e-7 as bright as the sun from Earth.
Re:Actually (Score:3, Interesting)
There is nothing between us and the star.
If you were lifted out from the gravity well of our solar system, I bet you can hit the star with a rock.
Or one rock out of billions thrown. Kinda hard to hit precisely at that distance.
Re:Actually (Score:2)
Maybe. Depends on the relative velocity with respect to our solar system, which is typically on the order of 10 kilometers per second or so. If that velocity is away from us, you're going to need a heck of an arm :^)
Re:Actually (Score:5, Informative)
Re:Actually (Score:2)
Re:Actually (Score:2)
Re:Actually (Score:2)
Re:Actually (Score:2, Informative)
Re:Actually (Score:2)
Re:Actually (Score:2)
Do an article need to *tell* you that?
All supernovas actually happened some time ago unless it's our Sun that's blowing up.
Re:Actually (Score:2)
Re:Actually (Score:3, Insightful)
Which was my point.
The problem at hand is perspective. Does "it happens at time X" refer to the supernova event taking place at the star, or does it refer to our observation of the event, which would have to take place 1,950 after the event took place at the star?
To put it more genera
Re:Warp Drive (Score:2)
People with clues (Score:2)
"Past light cone" means a lot more than just saying that the light hasn't reached us yet. The need to talk about there being no preferred reference frame is evidenced by all the self-deluded knuckle-draggers here who are saying, "yeah, well, it happened 1950 years ago the light just hasn't reached us yet."
That's not what special relativity says - past and future are not meaningful concep
Re:Don't hold your breath. (Score:2)
"The exact time period of this explosion is not known, but will likely occur within the next 100,000 years."
So you'd have some pretty long-living great-grandkids.
Re:Don't hold your breath. (Score:5, Insightful)
The radius of observation of these kinds of things is substantially smaller than infinite. Especially when you consider that earlier periods had a lower capability of observation.
So, really, we're talking about a fairly finite range of space and time in which supernovas would have to occur for them to be human-observable.
Re:Don't hold your breath. (Score:2)
Re:Don't hold your breath. (Score:2, Informative)
>quote:
>In a quasi infinate universe these things would happen constantly,
>not only once in a 225year span. (3*75, which is the human life
>expectency in Western Europe and the biggest part in the US)
>
>If the universe is 13.7 billion years old and there is only one
>supernova in the universe each 226years, that would make only
>60 619 469 supernovas since the origin of the universe.
first, most people have children sometime considerably sooner than their death. A
Re:Don't hold your breath. (Score:2, Offtopic)
Will that star go nova first, or will DNF and Vista be released first?
Heck: will our Sun go red giant before DNF ships?
(yeah I know, ZOMG DNF is late!!111!!! is getting old)
Re:Don't hold your breath. (Score:2)
(Don't forget about the 5 light year spread!)
Re:CNN Story is different... (Score:5, Informative)
Re:CNN Story is different... (Score:5, Funny)
So that would be like eating a vindaloo and lighting farts.
Re:CNN Story is different... (Score:2)
Re:CNN Story is different... (Score:5, Informative)
That's a nova. You've got a white dwarf, with a red giant companion star. Gas flows from the red giant to the white dwarf, accumulating there. Eventually enough builds up for fusion to begin in that accreted matter, and that causes a great increase in luminosity which we call a nova.
But that accreted mass doesn't disappear. Sure, some of it gets blown out into space, but the 'ash' of the fusion 'burn' accumulates with each cycle. Eventually, enough mass accumulates that the white dwarf star, in which fusion reactions have essentially stopped, becomes massive enough to start fusing the carbon that was created back when it was still on the main sequence.
So you have a sudden wave of carbon fusion that occurs everywhere throughout the star, causing an enormous increase in luminosity and also blowing the star apart. This is, not surprising, referred to as a 'carbon detonation' supernova, or Type 1a supernova, which is what the article was talking about. This thing's right under the critical mass at which that'll happen, so a bit more accumulation of stellar matter from its companion star, and 'boom.'
Re:Uh Oh (Score:2)
So I guess the summary is using "up close" as a relative term. Or like with most
Re:Penny-Arcade Found a Supernova? (Score:3, Informative)
I'm not sure I would use the word "discover", since Brahe's star was visible all throughout the northern hemisphere even during the daytime. Brahe, a drunken and rowdy old fool at the time (his nose had a gold tip, as he lost the flesh one in a drunken brawl), darling of the danish king and surrounded by cronies and hangers-on in his opulent estate, just happened to witness the event with not the slightest idea of what he was looking at, just
Re:It may have already happened! (Score:2, Informative)