Scientists Spot Rare 'In Between' Black Hole 182
An anonymous reader writes "Scientists have found a doomed star orbiting what appears to be a medium-sized black hole. This black hole appears to be a theorized 'in-between' category of black hole that has eluded confirmation and frustrated scientists for more than a decade."
Wouldn't that be a... (Score:5, Funny)
Re:Wouldn't that be a... (Score:2)
Re:Wouldn't that be a... (Score:1)
Re:Wouldn't that be a... (Score:4, Funny)
Seeing as how stars are white
My star's yellow [wikipedia.org], you (insensitive || extrasolar) clod!
not to be anal (Score:2)
Re:not to be anal (Score:2)
of which you are making fun ...
You have a problem with split infinitives?
Re:not to be anal (Score:2)
Corrected.
An' if'n that ain't a mouthful...
p.s. grammar rox
Pure White (Score:2)
Re:Pure White (Score:2)
-- The Solar Spectrum [utk.edu]
Re:Pure White (Score:2)
Re:Wouldn't that be a... (Score:5, Funny)
Re:Wouldn't that be a... (Score:2)
Its always after midnight.
Re:Wouldn't that be a... (Score:2, Funny)
No, the in-between space is the taint. An in-between hole would either be an anal fistula or a vaginal fistula. A super massive black hole would be goatse, and a standard black hole has already wiped out more crap than you would care to consider. A wormhole is a vaginal-to-anal fistula, and hyperspace gate triggers are made by Hitachi [amazon.com].
Be sure to tune in tomorrow when we offer penetrating insights into what trans-dimensional travel implies for space-borne dildo use.
Re:Wouldn't that be a... (Score:2)
Wow. (Score:2, Informative)
Re:Wow. (Score:2)
Is it because... the website's name is scienceblog.com?
anyways, someone care to explain this for me?
Re:Wow. (Score:5, Informative)
Yes- The gas circling the black hole, outside the event horizon, heats up due to friction. It gets hot enough to emit light along with UV, xrays, and often gamma rays. This gas isn't inside the black hole, so light can still get out. Once it falls into the black hole, no more light comes from it, but before then, there is usually a lot of light.
Re:Wow. (Score:5, Interesting)
A thought just occured to me. They say nothing can escape from a black hole due to it's huge gravity. Not even light. We know photons are the carriers of the electromagnetic force, one of the 4 fundamental forces in nature. I believe we have identified the carriers of the nuclear strong force and the nuclear weak force as well. But the suposed graviton has remained elusive and unidentified. By their very nature, though, shouldn't we be able to conclude that in order for black holes to generate such intense gravitational fields, they must allow their own gravitons to interact with nearby objects? In other words, the carriers for the force of gravity must be allowed to escape the black hole in order to exert that very force. Wait a minute....I can't be saying that right. Let's try again, suppose communication through an event horizon is possible - with gravity waves.
?????
Profit?
Re:Wow. (Score:2, Funny)
Re:Wow. (Score:4, Informative)
Re:Wow. (Score:3, Insightful)
Gravitons are hypothetical; no one has ever observed a graviton. Gravitons, if they exist, allow their force to escape black holes, which would seem to imply that gravitons do not act on each other (since they are not pulling themselves into the black hole).
IANA theoretical physicist, would one please chime in?
Re:Wow. (Score:2)
IANA theoretical physicist and would appreciate any corrections.
Re:Wow. (Score:5, Informative)
Re:Wow. (Score:2)
Re:Wow. (Score:3, Interesting)
Re:Wow. (Score:2)
IOW, we're still about the same place as we were in Newton's time. OTOH, that means there are still some open frontiers in science.
Re:Wow. (Score:2)
Re:Wow. (Score:2)
With the added fudge factors of dark matter and dark energy, of course.
Re:Wow. (Score:4, Interesting)
http://www.npr.org/templates/story/story.php?stor
Gravitons and BH (Score:2, Informative)
Re:Holy Crap (Score:2)
Re:Wow. (Score:2)
Still no information can emerge (according to current theories) - the output is (as far as we can tell) entirely random.
Re:Wow. (Score:2)
Re:Wow. (Score:2)
Re:Wow. (Score:2)
Re:Wow. (Score:2)
Re:Wow. (Score:2)
If you google hard enough you may yet be able to find a pdf of the lecture notes used by the bright young physicist/mathematician who presented the new proof of the mathematical theory. I forget what his name is but reading through the referenced materials in those two articles could lead you to him very quickly.
Re:Wow. (Score:4, Informative)
Re:Wow. (Score:2, Informative)
Or it might be slightly smaller than that, perhaps the size of RHIC [bnl.gov], according to an earlier story [slashdot.org]?
Re:Wow. (Score:2)
But I remember reading that a black hole can have exactly three properties: mass, electric charge and spin. Since electric charge is caried by (virtual) photons, does that mean photons do escape a black hole?
Re:Wow. (Score:2)
http://scienceworld.wolfram.com/physics/BlackHole
I was thinking (Score:2)
If you don't get it, look up where this is located in the sky.
Re:Wow. (Score:5, Informative)
In fact, you said it perfectly yourself without realizing it. Light is escapeing from the vicinity of the black hole, not the black hole itself.
Event Horizon (Score:2)
I realize that's the current gospel but I've often wondered if the event horizon isn't dynamic.
Consider the earth/moon gravity wells. There's an imaginary line that divides the two wells. A dust mote on one side of the line falls towards the earth while a mote on the other side falls towards the moon. The line that divides the two gravity wells is dynamic. As the moon orbits the earth, dust motes that were falling towards the earth can find themselve
Re:Wow. (Score:2)
There is no more event horizon [google.com]. Read the Newscientist and BBC articles from 2004.
Re:Wow. (Score:1)
Re:Wow. (Score:2)
Admiral Akbar says: (Score:4, Funny)
Re:Admiral Akbar says: (Score:1)
Re:Oh yeah? (Score:2)
article text (Score:5, Informative)
Dying Star Reveals More Evidence for New Kind of Black Hole
Submitted by BJS on Sun, 2006-01-08 11:58.
Posted in space | login or register to post comments | printer friendly page
Scientists using NASA's Rossi X-ray Timing Explorer have found a doomed star orbiting what appears to be a medium-sized black hole - a theorized "in-between" category of black hole that has eluded confirmation and frustrated scientists for more than a decade.
With the discovery of the star and its orbital period, scientists are now one step away from measuring the mass of such a black hole, a step which would help verify its existence. The star's period and location already fit into the main theory of how these black holes could form.
A team led by Prof. Philip Kaaret of the University of Iowa, Iowa City, announced these results today in Science Express. The results will also appear in the Jan. 27 issue of Science.
"We caught this otherwise ordinary star in a unique stage in its evolution, toward the end of its life when it has bloated into a red giant phase," said Kaaret. "As a result, gas from the star is spilling into the black hole, causing the whole region to light up. This is a well-studied region of the sky, and we spotted the star with a little luck and a lot of perseverance."
A black hole is an object so dense and with a gravitational force so intense that nothing, not even light, can escape its pull once within its boundary. A black hole region becomes visible when matter falls toward it and heats to high temperatures. This light is emitted before the matter crosses the border, called the event horizon.
Our galaxy is filled with millions of stellar-mass black holes, each with the mass of a few suns. These form from the collapse of very massive stars. Most galaxies possess at their core a supermassive black hole, containing the mass of millions to billions of suns confined to a region no larger than our solar system. Scientists do not know how these form, but it likely entails the collapse of enormous quantities of primordial gas.
"In the past decade, several satellites have found evidence of a new class of black holes, which could be between 100 and 10,000 solar masses," said Dr. Jean Swank, Rossi Explorer project scientist at NASA's Goddard Space Flight Center, Greenbelt, Md. "There has been debate about the masses and how these black holes would form. Rossi has provided major new insight."
These suspected mid-mass black holes are called ultra-luminous X-ray objects because they are bright sources of X-rays. In fact, most of these black hole mass estimates have been based solely on a calculation of how strong a gravitational pull is needed to produce light of a given intensity.
Kaaret's group at the University of Iowa, which includes Prof. Cornelia Lang and Melanie Simet, an undergraduate, made a measurement that can be used in the equation to directly calculate mass. Using straightforward Newtonian physics, scientists can calculate an object's mass once they know an orbital period and velocity of smaller objects rotating around it.
"We found a rise and fall in X-ray light every 62 days, likely caused by the orbit of the companion star around the black hole," said Simet. "The velocity will be hard to determine, however, because the star is located in such a dust-obscured area. This makes it hard for optical and infrared telescopes to observe the star and make velocity calculations. Yet for now, knowing just the orbital period is very revealing."
The suspected mid-mass black hole, known as M82 X-1, is a well-studied ultra-luminous X-ray object in a nearby star cluster containing about a million stars packed into a region only about 100 light years across. A leading theory proposes that a multitude of star collisions over a short period in a crowded region will create a short-lived gigantic star that collapses into a 1,000-solar-mass black hole. The cluster near M82 X-1 has a high-enough density to f
slightly OT (Score:3, Interesting)
How do/did the heaviest elements, which are/were formed in the largest stars, escape from those stars that ultimately become/became neutron stars and black holes? I know that elements are flung out from the star via super novae, but wouldn't the heaviest elements be at the core of the star that remains? how would they get out? Shouldn't they all be trapped in the stellar remnants?
Re:slightly OT (Score:2)
And its perfectly possible for heavy objects to be at the edges, think about gliders flying on convection.
Re:slightly OT (Score:1)
I know, but the ones that just go poof and die - I thought - would only produce elements up to carbon or so. Though, yes, I suppose you are right that the possiblity that heavier elements could be on the outside of the H/He shell explosion is possible.
Re:slightly OT (Score:2)
Re:slightly OT (Score:4, Informative)
Um. No. A fusion reaction can create any substance up to uranium and beyond. In fact, humans are continually creating substances beyond uranium (plutonium being one) through fusion reactions. It's just that fusion reactions to produce elements heavier than iron require energy, rather than giving off energy.
In the early stages of a star's life, it's fusing hydrogen atoms to produce helium. This is the most energetic fusion reaction, and is the only fusion reaction we're likely to be able to sustainably exploit to our own ends through artificial means. As the star grows older, and has less hydrogen, it will increasingly generate its energy through other fusion reactions, producing elements up to iron. (These reactions will occur throughout the star's life; it's just that they will become proportionally more important as the star ages.)
Eventually, the energy produced through these fusions will die off, and the star will undergo gravitational collapse. During this phase, the energy consuming fusion reactions will occur, generating the heavier-than-iron elements. This phase only occurs in massive supernova; it won't happen in our sun -- it's not big enough.
Re:slightly OT (Score:2)
Re:slightly OT (Score:2)
I found this on NASA's web site: http://imagine.gsfc.nasa.gov/docs/teachers/lesson s /xray_spectra/background-elements.html [nasa.gov]
It suggests that heavier atoms are created during supernovae, as well as in the ISM during "day to day operations." Maybe the relative lack of heavier atoms in space has something to do with the fact they are all sucked into black holes?
Re:slightly OT (Score:5, Informative)
Re:slightly OT (Score:5, Informative)
Re:slightly OT (Score:2)
IANAP, but I do seem to remember from physics/chemistry that the determining factor in element number is the number of protons, not the number of neutrons. Picking up more neutrons will change the isotope, not the element. (For instance, deuterium is just an isotope of hydrogen with an added neutron.)
Re:slightly OT (Score:3, Informative)
That's where the beta decay comes in. Beta decay turns neutrons into protons.
Heavier elements (Score:3, Interesting)
Re:slightly OT (Score:5, Funny)
What you describe is the r (rapid) process. A very high neutron flux adds neutrons very quickly. Once the neutron pulse has passed, the highly-neutron-rich nuclei beta-decay (neturon turns to proton) multiple times until a stable element is reached.
The s (slow) process has a low neutron flux, so that there is sufficient time after each neutron is absorbed for beta decay to occur. The neutrons come from a comparatively neutron-rich nucleus left over from the CNO cycle for burning hydrogen (N15?) At sufficient temperature/pressure, it starts to lose its excess neutron. The new heavy nuclei can then convect to the surface of the star and escape in the stellar wind. The detection of technetium (which has no stable isotope) in the spectra of these stars is the smoking gun proving this scenario.
I don't know much about the p process.
The r and p processes occur in supernovae. The s process occurs in red giant stars (strictly, asymptotic giant branch stars.) In terms of importance in creating heavy elements on the earth, s process is most important, followed by r process and then p process. From memory, it is something like 90% s proccess, 9% r process, 1% p process, but that is *very* rough.
Now we need a q process, so we can p, q, r and s processes. (Or S, P, Q, R if you're a Romanophile.)
Doomed (Score:4, Funny)
Ah what a body of work the universe is (Score:2, Interesting)
Given the possible variation in black hole sizes this poses some interesting problems for long term space travel. Mini-holes will pose major danger during high speed travel unless some fast detection method is found. This has resonances with Arthur C Clarke's story about the star mangled spanner...
Re:Ah what a body of work the universe is (Score:2)
I don't mean to be boring or anything, but you do realize humanity is still at the "how do we get out of our miserable gravity well and go further than the moon on chemical power" stage, right?
So I think we can safely set aside the high-speed mini-hole collision hazard problem for now.
Re:Ah what a body of work the universe is (Score:1)
Re:Ah what a body of work the universe is (Score:2)
Besides, if you're moving fast enough for it to be a problem without ripping apart you can more or less treat the entire vessel as a single particle. If you get close to C, then your mass will be insanely high with enough energy to ignore most things.
As with all current or theoretical physics, your mileage may vary.
Re:Ah what a body of work the universe is (Score:2)
The abstract (Score:3, Interesting)
---
Reading this and the article, I'm not sure if the claim is necessarily valid. What's to stop this being a smaller black hole, a smaller star orbiting closer (with the same period), and beamed emission? An intermediate black hole is still the simplest explanation, but doesn't seem unique.
Re:The abstract (Score:2)
[TMB]
Sorry people, explanation (Score:2, Informative)
However, it's just a dot in the sky, you can't tell how much energy in total is being given out just by measuring how much is coming in the direction of Earth - you don't know if it's a 60W lightbulb shining in all directions or a 5W torch pointing at you. For instance, black holes can have jets (rather like pulsars) and a smaller black hole
Goatse (Score:2, Funny)
PARENT MODERATION UNFAIR! (Score:2, Informative)
Re: (Score:1)
Re:I have a black hole "in between" my... (Score:2)
Re:I have a black hole "in between" my... (Score:2)
I'm happy to know now that it was really mother nature trying to fill the blackhole void between your ears.
The scientific name for this phenomena is (Score:2)
Animation Automation (Score:2)
I can't help but think that an intern did some tweening with a newfound graphics program.
Eluded confirmation? (Score:2, Informative)
Was this simply further examples of similarly sized black holes?
Re:Eluded confirmation? (Score:2)
Even the
Who did it this time? (Score:1, Offtopic)
Someone please think of the servers (Score:3, Informative)
In between what ? (Score:3, Funny)
Hmm, maybe they did spot it inbetween breakfast and lunch, the statistics of that happening are high.
HUH? (Score:2)
"With the discovery of the star and its orbital period, scientists are now one step away from measuring the mass of such a black hole, a step which would help verify its existence."
Is it just me or is even science journalism getting sloppy...
It seems to me that measuring the mass of something would not only help verify its existence, but prove it beyond the shadow of doubt.
sourcing (Score:5, Insightful)
Re:sourcing (Score:3, Funny)
Experts say we're better off without those extra 5-7 words of information.
Who are you to argue with the experts?
Re:sourcing (Score:2)
You are talking about median intelligence. Half the world is dumber that the guy of median intelligence by definition. All it takes is a few really smart guys and a lot of mediocre ones, and 90% of the world can be dumber than someone with average intelligence.
Human beings do not follow a power law (Score:2)
Re:Human beings do not follow a power law (Score:2)
Actually no.
Group 1. variable x
Group 2. variable is x^2
Both groups are exactly the same size.
If one group is normal, the other is not.
You may be confusing a large group with the sum of a large number of distributions. The sum of a large number of distributions (which need not be at all normal) goes to a normal distribution as the number of distributions in the family goes to infinity. It is the infinite tail of the family that is normal, no
Re:Human beings do not follow a power law (Score:2)
Actually yes. bstadil's GP post was talking about large groups of human beings, who exhibit normal distribution under most circumstances and do not "go to infinity".
Re:Human beings do not follow a power law (Score:2)
Annual income.
If the distribution is normal,
"The rich get richer and the poor get poorer"
is an impossibility.
Average income and median income should be extremely close to each other.
Life Expectncy -- everybody dies eventually
I don't think that is anything like normal.
What IS tending toward normal is to add up all these various distributions.
What that would wbe good for, I have no idea.
Re:sourcing (Score:5, Funny)
From TFA, "A team led by Prof. Philip Kaaret of the University of Iowa, Iowa City, announced these results today in Science Express."
> What scientists were frustrated?
Although TFA doesn't specify, I think they're talking about "scientists" in general. Much as your comment talks about "stories"... in general, I presume.
You know, reading TFA wouldn't break the bank and it would really make your comment feel less lazy.
So.. (Score:3, Insightful)
Speaking of keeping an eye on it, has anyone managed to find any actual pictures?
Re:Uh oh... (Score:3, Funny)
Re:Didn't say where the black hole is, but (Score:2, Funny)
Re:Didn't say where the black hole is, but (Score:2)
Re:Just Wondering (Score:2)
Re:Just Wondering (Score:2)
Bloody good question. Theory is unclear on this point. If you're betting, then the smart money's on 'they just merge and form a larger black hole', but things get all quantum when you try to actually prove it.
I read a while back that part of the problem is that it's common to view the event horizon of a black hole as the shell of photons emitted by the star just as it contracted below the Schwarzschild radius; these photons are trapped right on the edge, forever