Dead Star Set to Escape the Milky Way 132
slackah wrote to mention a NewScientist.com article discussing a fast-moving stellar corpse on its way out of our galaxy. From the article: "The object, called B1508+55, is a rotating neutron star, or pulsar. It is the superdense core of a massive star that exploded as a supernova about 2.5 million years ago. The explosion seems to have ejected the pulsar with such force that it will eventually escape the Milky Way entirely, says team member Shami Chatterjee, an astronomer with NRAO and CfA."
Rogue star (Score:1, Funny)
Re:Rogue star (Score:3, Funny)
Re:Rogue star (Score:1)
Re:Rogue star (Score:2, Funny)
Re:not long (Score:1)
Hmm? (Score:1)
It can't be a space station. (Score:4, Funny)
Careful (Score:4, Funny)
Re:Careful (Score:1)
"Somebody set us up the bomb!"
Re:Careful (Score:2)
http://www.x-entertainment.com/messages/262.html [x-entertainment.com]
Re:It can't be a space station. (Score:3, Informative)
Don't say that, a neutron star [wikipedia.org] has a diameter of about 25 km.
Re:It can't be a space station. (Score:2)
Re:Hmm? (Score:1)
Tracking (Score:4, Insightful)
Comment removed (Score:4, Funny)
Re:Tracking (Score:5, Insightful)
Fast, for a star, but it's 1/300th of c. So it'll be at least 300,000 years to get 1000 ly out, getting to the edge of the galaxy. By then we'll either be extinct or know all about the dark matter.
Insighful (Score:1, Insightful)
Re:Insighful (Score:1)
That's still a blink of an eye compared to the billions it's been around.
Re:Insighful (Score:1)
Galaxies must be a lot more dynamic than I thought (Score:4, Interesting)
It also occurs to me that this isn't really news: depending on how far away the star is/was, there's a fair chance that it left our galaxy millions of years ago
Re:Galaxies must be a lot more dynamic than I thou (Score:1, Informative)
Galactic colission simulations (Score:3, Interesting)
for what it's worth, here's a simulation of Our milky way hitting Andromeda.
Things like this happen all the time.
Re:Galactic colission simulations (Score:2)
This animation almost makes the galaxies appear to be alive.
Mirror link (Score:2)
You can change other parameters as well, such as number of galaxies, their size, even their colors!
Solomon Chang
Re:Galactic colission simulations (Score:2)
Re:Galactic colission simulations (Score:2)
Re:Galactic colission simulations (Score:2)
You mean like on my screensaver [tuwien.ac.at]?
Re:Galaxies must be a lot more dynamic than I thou (Score:4, Interesting)
7700 years, anyway, according to the article.
But it's never a good idea to take these announcements at face value. It's far from clear the thing has anything to do with a supernova, or that it's a neutron star at all -- presuming any of them exist at all. What we do know is that its light (radio, x-rays, etc.) pulses at a rate too fast for them to understand unless it's a tiny thing spinning.
The reason they insist it has to be something spinning is that they have studied almost no plasma fluid dynamics, so they can't understand something blasting out radio, light, and x-rays that doesn't have a star in the middle of it. They don't understand fluid instabilities and current oscillations, so they're at a complete loss to understand the (quite common) sudden, often temporary changes in oscillation rate in pulsars.
What little they have studied, typically, is a trivial approximation to plasma fluid dynamics known as "magneto- hydro-dynamics" (MHD) which assumes space is superconducting and magnetic fields can't change distribution or strength. (They talk in all earnestness of magnetic fields "frozen" in place -- even in the sun!) Therefore, they can't understand how large flows of charged particles -- currents, which they insist on calling "jets" -- produce their own magnetic fields and flow along them, or how these flows' fields can interact in marvelously complex ways.
Everything you read about "dark matter", "supermassive black holes", and "neutron stars" amounts to a desperate attempt to find some way to make the extremely weak and purely attractional gravity account for the complicated things they see. The mathematics behind plasma fluid dynamics is too hard for them, and they just can't stand that. It makes their press releases funny to read, but it's sad, too. (Think of the lives wasted on planetary epicycles.)
Re:Galaxies must be a lot more dynamic than I thou (Score:2)
Re:Galaxies must be a lot more dynamic than I thou (Score:2)
There are plenty of papers published by serious plasma researchers. Astrophysicists don't read them. That's what makes it sad, but it's also what makes the press releases positively comical.
Birkeland currents have been studied for more than a century, ever since they were elucidated as the process behind the Aurora Borealis. Next time you meet an astrophysicist, ask why Birke
Re:Galaxies must be a lot more dynamic than I thou (Score:1)
They ARE important, and beyond the simplistic things that astrophysicists deign to deal with like the Coulomb Barrier in s
Re:Galaxies must be a lot more dynamic than I thou (Score:2)
The reason they insist it has to be something spinning is that they have studied almost no plasma fluid dynamics, so they can't understand something blasting
Re:Galaxies must be a lot more dynamic than I thou (Score:2)
Evidently the only thing that could carry that much momentum must be neutronium, because it has to be imagined physically tiny. That model fails, though, to account for recently discovered pulsars that would have to spin fast enough to break up even a neutron star. W
Re:Galaxies must be a lot more dynamic than I thou (Score:2)
1) New Orleans is below sea level
2) It's almost right on the gulf. So close as to not to matter.
3) People have known the danger for *years*. So much so that I saw a tv special last year on the dangers of a hurricane to New Orleans. I live in california.
4) We saw this thing heading right for New orleans on TV days in advance.
Now, taking all these facts together, I wouldn't even be *living* in new orleans. But sa
Re:Galaxies must be a lot more dynamic than I thou (Score:3, Interesting)
Mistake avoided, as its fairly obvious
Spoken like someone who has never spent a significant part of their life without a car in a country where a car is virtually a necessity.
What transportation are you going to "find" if you can't afford any? Even if you got a couple hundred dollars, so you blow it on a rental or a taxi to get to the next major city. Now you're
Re:Galaxies must be a lot more dynamic than I thou (Score:2)
While I do have a car, I do not typically drive it. In fact, right now I'd imagine the battery is dead. Again. I do understand what it's like not to have a car handy. The only bits of information I'm missing here is why anybody believed they were safe in that city during a hurricane.
What transportation are you going to "find" if you can't afford any? Even if you got a
You know your life is sad... (Score:4, Funny)
Re:no time to waste! (Score:2, Funny)
I want a name like that! (Score:2, Funny)
Abraham (Score:2)
Of course, we'd end up naming you fairly boring and common names like David and Sarah.
Re:Abraham (Score:2)
Amazing (Score:3, Interesting)
Strange how one can be so impressed by something, he knows so little about...
The concept of escaping the galaxy is awsome, but it would be nice to know more about it...
So I did some research: Milky Way Galaxy is: ~100,000 light years in diameter; ~3,000 light years in thickness; ~250,000 light years in circumference.
Basically, its huge. The ratio of our solar system to the milky way galaxy is 1:65,000,000.
From this I believe that just about anything can escape the galaxy, it would just take an extremely long time. However, as I have stated, my knowledge on the subject is limited, so it is possible that the planets and stars are arranged in such a way, that the gravitational pull would always redirct any object to go back. (i.e.: meteors and asteroids pass Earth in patterns and intervals, without leaving the galaxy).
The subject is very interesting, and if someone could bring more light on it, it would be helpful...
orbits (Score:2)
It is exceptional that something got the escape velocity to leave the galaxy in a kind of time frame that we're able to see it happen in.
This pulsar is the new speed record holder for an object of its class.
Cops on the freeway will love this one... (Score:1)
Re:Amazing (Score:5, Funny)
Wow. I knew we had a central black hole, but I didn't realise it distorted space that much. What value is the pi where you live?
Re:Amazing (Score:3, Informative)
http://en.wikipedia.org/wiki/Circumference [wikipedia.org]
Wikipedia confirms the poster's numbers BTW.
http://en.wikipedia.org/wiki/Milky_Way [wikipedia.org]
Re:Amazing (Score:2)
About three to five bucks, depending on size and filling.
Re:Amazing (Score:1)
You need to look at the concept of "escape velocity". There are two ways to approach this concept - as an expression of a time series of decreasing velocities, or on an energetics basis. The energy basis is simpler to explain - consider that an object moving in a gravitational field has a particular amount of kinetic energy as a consequence of it's motion. The same object would require a certain amo
In other news... (Score:5, Funny)
Let me be the first to say... (Score:1)
Comment removed (Score:4, Funny)
Re:Did anyone else... (Score:2, Funny)
Re:Did anyone else... (Score:2)
(My God... that's the second consecutive post I've made on
Re:Did anyone else... (Score:2)
Re:Did anyone else... (Score:2)
Re:Did anyone else... (Score:1)
Re:ELE? (Score:2, Insightful)
Cool (Score:2)
How is this possible? (Score:2)
Anyone care to explain it to a long-time-ago astrology student?
Re:How is this possible? (Score:3, Informative)
Re:How is this possible? (Score:5, Informative)
After the collapse, the kinetic energy of the quasi free falling neutron matter will overcompress the neutron star core, and then it will oscillate.
As the collapse istn something perfectly symetrical, there will be significant amplitude of the first harmonic of the oscillation. Thus (for example) the matter hitting the star on one hemisphere will have the core expanding in their direction with quite some speed, while the other side will see it receeding). As the impact isnt very long, there wont be time to average out. In the moment the hull impacts, the core will "push" itself away from that quasi-spherical shell thats hitting it.
(you have to remember: there is significant mass in that shell. Only a small part of the star actually ends of in the neutron star, so there IS enough mass in the hull for conservation of momentum)
Re:How is this possible? (Score:3, Informative)
The slingshot principle has been used for a number of spacecrafts and there is a number of trajectories which could transfer momentum between two objects traveling in a common gravity well (e.g. galaxy or solar system).
Yours Yazeran
Plan: To go to Mars one day
Re:How is this possible? (Score:2)
I know, i know. Had to calculate such a slingshot in lagrange coordinates years ago, its a bitch...
But for neutron stars:
Calculate the odds for such a slingshot, and the needed trajectories....
1000km/s is FAST, the other partner would need to be a black hole to get speeds like that ( a normal star wouldnt survive, but merge with the neutron star).
The crossection is SO small, the needed target so rare, the needed deltaV so large, thats there not much chance of something like this happening in a galaxy ever.
Re:How is this possible? (Score:2)
Yours Yazeran
Plan: To go to Mars one day with a hammer.
Re:How is this possible? (Score:2)
You are forgetting the super-massive black hole in the center of the galaxy, and any black-holes (or neutron-stars) which may very probably be in orbit around it. (lookup AGN - active-galactic nuclei)
In fact, I'm not sure that the slingshot option isn't rather more probable than the fast-supernova-remnant hypothesis. Remember that the star-dens
Re:How is this possible? (Score:1)
At least I hope that our destinies will not be affected by the fact that a dead star is leaving our galaxy.
Re:How is this possible? (Score:1)
Astrology?
Hmmm.
Okay, this may suit you...
For an explanation of how neutron stars achieve such high speeds, read the first chapter of Robert L Forward's _Dragon's Egg_. It fills in all the actual details missing from TFA.
Go on... look in Wiki. You know you want to!
Re:How is this possible? (Score:1)
Thats nothing unususal (Score:5, Informative)
Now if such a collapse isnt absolutly symetrical, there will be higher spherical hermonics in the neutron core oszillation, and thus the impact of the hull on the core will give it a random impuls vector (the first harmonic being the 2 hemispheres oszilating with 180degree phase difference).
The observation of those fast moving neutron stars helped the understanding of this processes, as there isnt much that can accelerate them after their creation to this speeds.
A common speed of a class2 supernova product is in the 100-1000 km/s range (about 2 orders of magnitures lower than the speed of the the ejected hull, thus the visible SNR still seemingly have the neutron star in the center), which is way enough for most to leave our galaxy (300 or so is needed)
Re:Thats nothing unususal (Score:2)
OMG (Score:3, Funny)
OMG! DON't LET IT GET AWAY! SEND THE AMERICANS TO RETRIEVE IT!
ON second thought.. I slightly recall the "retrieving"-abilities of the US army and some guy who's bin pretty laden.
Re:OMG (Score:2)
You have billions in funds for the US army, and have the most advanced weapons. Yet you couldn't retrieve a guy on a camel.
Re:OMG (Score:2)
Escape the Milky Way? (Score:1)
Sorry, ladies and gentlemen (Score:2)
Has to be done (Score:3, Funny)
"Bring out your dead!"
Roger Wilco strikes again (Score:2)
I know what it is (Score:1)
Whoa! (Score:2)
Old news? (Score:2)
Anyway it would be nice to project its path ahead to see what civs need bailing out. Then NASA's warp drive project has a goal! Maybe we should keep our scopes and neutrino detectors on that region of space to see if any other civs already have mounted a hypervelocity rescue effort? Note the star is seen 7000 years in the past, so it is actually 20 light years or so closer to its vict
Nemesis (Score:2)
Milky Way? (Score:2)
Freakin' Fast! (Score:1)
1 100 (kilometers per second) = 2 460 629.92 miles per hour
Damn.
Anyone up for ride ? (Score:2, Interesting)
Hmmm... (Score:1)
Stellar probes for dark matter (Score:5, Interesting)
There are two things that excite me about this. 1) B1508+55 is a massive radio emitting object which is boldly going into the intergalactic space where all that putative dark matter is supposed to be. If its path bends we might end up discovering a "dark galaxy". Of course someone with access to human astronomy records must be around to observe this when it happens.
2) Cygnus spits out a lot of these objects. Maybe if we get a very much faster one, we can have a more convenient probe.
Re:Stellar probes for dark matter (Score:4, Informative)
Indeed, pulsars are used to probe the interstellar medium to get at how much mass is tied up in ionized hydrogen, which scatters incident radio waves, causing scintillation which can be observed with a radio telescope. (Scintillation is the same effect the Earth's atmosphere has on visible light from stars, known as twinkling.) One of the ways we estimate the electron density in interstellar space is by comparing the dispersion of the pulsar signal to the distance to the pulsar. (This assumes you can get an accurate measurement of the distance, which is hard and uncertain for all but the most nearby pulsars.) There aren't great constraints on how much mass is tied up in interstellar gas, although it's not a terribly hot prospect for the missing baryonic mass.
There are about 40 known pulsars that are substantially above the plane of the milky way (galactic altitude > 3 kpc or 9000 light years; this pulsar is 2.4 kpc away, according to the paper, for an altitude of 1.9 kpc). Most of these are in globular clusters or the Large and Small Magellenic Clouds, two small, nearby galaxies that orbit the Milky Way. What's remarkable about this pulsar is that it formed in the galactic plane and was kicked up that high.
Pulsars typically move at velocities of ~100 - 500 km/s, so they cover a lot of space quickly, which lets you see the changes in the scintillation pattern on solar system size scales over the course of a few months. If you want to look at big scales, you look at many different lines of sight (i.e. many different pulsars).
(Yes, I am a pulsar/interstellar medium astronomer, or at least a grad student who works in this area and knows very little.) ;)
Interstellar "gas" medium (Score:2)
Such curre
Re:Yippie! (Score:1)
Re:Yippie! (Score:1)
Re:Yippie! (Score:1)
Re:Yippie! (Score:1)