NASA | Fermi Catches a 'Transformer' Pulsar

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  • čas přidán 21. 07. 2014
  • In late June 2013, an exceptional binary system containing a rapidly spinning neutron star underwent a dramatic change in behavior never before observed. The pulsar's radio beacon vanished, while at the same time the system brightened fivefold in gamma rays, the most powerful form of light, according to measurements by NASA's Fermi Gamma-ray Space Telescope.
    The system, known as AY Sextantis, is located about 4,400 light-years away in the constellation Sextans. It pairs a 1.7-millisecond pulsar named PSR J1023+0038 -- J1023 for short -- with a star containing about one-fifth the mass of the sun. The stars complete an orbit in only 4.8 hours, which places them so close together that the pulsar will gradually evaporate its companion.
    To better understand J1023's spin and orbital evolution, the system was routinely monitored in radio. These observations revealed that the pulsar's radio signal had turned off and prompted the search for an associated change in its gamma-ray properties.
    What's happening, astronomers say, are the last sputtering throes of the pulsar spin-up process. Researchers regard the system as a unique laboratory for understanding how millisecond pulsars form and for studying details of how accretion takes place on neutron stars.
    In J1023, the stars are close enough that a stream of gas flows from the sun-like star toward the pulsar. The pulsar's rapid rotation and intense magnetic field are responsible for both the radio beam and its powerful pulsar wind. When the radio beam is detectable, the pulsar wind holds back the companion's gas stream, preventing it from approaching too closely.
    But now and then the stream surges, pushing its way closer to the pulsar and establishing an accretion disk. When gas from the disk falls to an altitude of about 50 miles (80 km), processes involved in creating the radio beam are either shut down or, more likely, obscured. Some of the gas may be accelerated outward at nearly the speed of light, forming dual particle jets firing in opposite directions. Shock waves within and along the periphery of these jets are a likely source of the bright gamma-ray emission detected by Fermi.
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Komentáře • 89

  • @LabNYorkie
    @LabNYorkie Před 10 lety +40

    This is yet another reason I love astronomy. Thankful that NASA Goddard has its own channel.

  • @mikey7257
    @mikey7257 Před 10 lety +6

    I can watch stuff like this all day long

  • @BinkieMcFartnuggets
    @BinkieMcFartnuggets Před 10 lety +16

    Michael Bay can't wait to get one of these into his next movie.

  • @rippi37
    @rippi37 Před 4 lety +2

    Thoroughly intriguing. The universe is awesome !!!!!

  • @donnagreven2775
    @donnagreven2775 Před 10 lety +6

    I am so glad I discovered Universe Today on my phone since I have missed all the good astronomy stuff and NASA since I lost internet on my computer (Windows xp). Being more of an astronomy tourist than anything else. I'm not very good at all the techno stuff. Thank you NASA.

  • @Jia1337
    @Jia1337 Před 10 lety +10

    I thought I was hearing mass effect soundtrack.

  • @TheDerpWhales
    @TheDerpWhales Před 10 lety +1

    Fascinating

  • @ddorman365
    @ddorman365 Před 7 lety +2

    Sweeet!!, thank you NASA, peace and love, Doug.

  • @TPYXIDIS
    @TPYXIDIS Před 10 lety +2

    Great man.
    Wish I could fly or work for NASA

  • @ronaldwest2264
    @ronaldwest2264 Před 5 lety +1

    Golly! The universe is an awesome work of art.

    • @jesus4400
      @jesus4400 Před 2 měsíci

      Of photoshop 😂😂

  • @inSpihr
    @inSpihr Před 10 lety +2

    Fluck that was intense.

  • @stdfreesteve
    @stdfreesteve Před 10 lety +1

    soo cool!!!!

  • @eejay534
    @eejay534 Před 6 lety +2

    the phases probably come from the star having an elliptical orbit so when the star gets close enough the pulsar steals gas from the star then when the stars orbit goes further from the pulsar the gravity isn't enough to steal gas from the star only just blowing it away

  • @912582
    @912582 Před 10 lety

    Pretty cool

  • @VGAstudent
    @VGAstudent Před 4 lety

    An eliptical orbit that grazes the stress threshold of the companion's atmosphere may be the reason for the blockage of radio waves until the orbit has the material cleared through either falling onto the star or being electromagnetically sorted by the charge of the highly influential magnetic field of the pulsar itself. An atmosphere of a superconductive material will be less affected than a polarized ion or atom of a charged element or a polarized elemental particle. Gama rays are strong enough to punch through a polarized elemental cloud of particles, but the radio pulses may actually be conducted directly by a superconductive surface of the neutron star if it get's shorted into a pulse that grounds out immediately at the poles.
    This would make a pulse in the gama-ray burst itself in changing enegy levels when it was superconducted or resisted, causing a higher level of gama-ray burst or a higher temperature of the nebula cloud enveloping the pulsar. Either mechanism would eventually cause added momentum to be accumulated in the act of pulling the matter into the surface at an accellerated pace in addition to gravity, but electromagnetically, like a huge hadron collider, creating heavier and stronger forms of radiation, that span into the microwave, x-ray and gama-ray energy emissions; I can't get close enough to map the electromagnetic lines of force inside a neutron star, but I suspect they are phenominally mind boggling in their strengths locally.

  • @anjachan
    @anjachan Před 3 měsíci

    this is absolutely crazy ...

  • @dianachesta3873
    @dianachesta3873 Před 9 lety

    Interesting and amazing

  • @max-wf3bo
    @max-wf3bo Před 10 lety +1

    Wow cool

  • @LattiMonstaaa
    @LattiMonstaaa Před 8 lety +8

    that music tho

  • @hygrobiology
    @hygrobiology Před 2 lety

    I have no idea why I knew this before and I love green, yellow and violet colors

  • @alberto8014
    @alberto8014 Před 10 lety

    May it be just a silly thought, but...having a third star in the system would counter the neutron star's gravitational pull temporarily while passing opposite the neutron star and close to the sunlike one. As the mass between the neutron star and the sunlike isn't too different, the pull of a third one could affect the pair significantly.

  • @yopinwu2082
    @yopinwu2082 Před 2 lety +1

    Wow

  • @erdemmemisyazici3950
    @erdemmemisyazici3950 Před 5 lety

    So really the switch in modes is just the time it takes for the neutron star to chew the other star.

  • @manishkmrp
    @manishkmrp Před 3 lety

    Yes, two gases compound created or creating by this method.

  • @Reed1
    @Reed1 Před 5 lety

    it makes sense that as the neutron star collects gas and increases its spin, its magnetic field would increase in strength, which would then push away the material from its companion star. After the material is no longer in an accretion disk, the neutron star's magnetic field would slow down the star's spin, and therefore the field, allowing for the gas to collect again.

  • @gigicaly
    @gigicaly Před 10 lety +11

    "closely" is not the word I would use when observing something from 4.4k ly away :)

    • @inSpihr
      @inSpihr Před 10 lety +4

      "Word" is not the word I would use to describe two words.

    • @HozAbubakir
      @HozAbubakir Před 10 lety

      inSpihr
      epic burns

    • @gigicaly
      @gigicaly Před 10 lety +1

      inSpihr closely was the word i was talking about... but ok I see your point... thank you for the awesomeness you're making me aspire to.

  • @MegaBanne
    @MegaBanne Před 5 lety

    Pure conjecture.

  • @gomerpile5708
    @gomerpile5708 Před 3 lety

    Reverse ionization ? 🤔 maybe during polarity reversal ?

  • @Stammer6
    @Stammer6 Před 10 lety

    That's -really- cool stuff. Why didn't I take astronomy...

  • @christianmoya2631
    @christianmoya2631 Před 10 lety

    ¡¡Realmente impresionante y fascinante!!

  • @misterapplememe8263
    @misterapplememe8263 Před 3 lety

    Sextans is my favorite

  • @RolyRamirez
    @RolyRamirez Před 10 lety

    Pueden hacer el videos pero con audio en ESPAÑOL please

  • @Scotian6444
    @Scotian6444 Před 7 lety

    forward spin of the companion star is decelerating back side is accelerating.. as to not digesting the star in one go? seeing the pinch point would be on the back side of the orbiting companion.. its shape constantly gets pushed forward out of the rest it has found.. creating a rotation around its own orbit at this point? allowing it to migrate away in orbit.. the pulses in gamma could very well be the pinch in the wobble?
    but than the pulse would be delayed in timing.. and take longer and longer.. but than again math has a funny way of balancing the natural world when it comes to ratios
    but than again.. if its acting like a stopper to a disk that has grown outward and is increasing in density. you may just find that a overflow actually changes the axis of the companion..
    I just can not see a nice orbit that decays and than expands in such a violent system.. figure eights.. lossing a orbital period.. being pushed off of a orbital plane.. sounds more like it
    just the shape the companion would assume.. seeing in one orbit that would continually move towards the pull. we need to know the rotaional speed of the companion.. something tells me it changes.. as so far as going retro.
    im more interested in the companion star now. ty

  • @carlose6010
    @carlose6010 Před 10 lety +1

    Sweet, looks tasty

  • @albertuskundratis1
    @albertuskundratis1 Před 9 lety

    Is it possible, even if remotely, that that binary companion, by losing enough mass, will lose its ability to periodically resist the pulsar, and therefore SUDDENLY COLLIDE INTO THAT PULSAR PRODUCING AN ODD SUPERNOVA?

  • @ShaunKeefe
    @ShaunKeefe Před 10 lety

    Probably the different phases are caused by the aphelion and perihelion of the orbit of the star.

    • @nnobster
      @nnobster Před 9 lety

      I realise that this may sound pedantic but, when it comes to science, precision is key:
      Apoapsis & periapsis, not aphelion and perihelion. "Helio" refers to OUR sun.

  • @assaltmaster89
    @assaltmaster89 Před 9 lety

    how does a pulsere win when a nutron star is heavier and more dense?

    • @lillianbanda4033
      @lillianbanda4033 Před 8 lety

      No a pulsar and neutron star are simular.

    • @damic4201
      @damic4201 Před 7 lety

      a neutron and pulsar are very similar, except a pulsar spins much, much faster.

    • @celestial3328
      @celestial3328 Před 7 lety

      Lillian Banda Pulsars are types of Neutron Stars

  • @cybermagzctm
    @cybermagzctm Před 10 lety

    wishing to be travel tour sponsored to see again w/ my father who is now a senior citizen for the second time his eversince wayback travel der in 1982 = the launching rocket pad of NASA Kennedy Space Center,Orlando Florida U.S.A.! many tnx! nevertheless to say its only a dream!

  • @artawesome30
    @artawesome30 Před 4 lety +1

    Naruto at the end of Shippuden be like

  • @SmoKeSome357
    @SmoKeSome357 Před 9 lety

    they havnt observed the transformation in progress..hmmm...

  • @transformersandfnaftoyhunt4801

    do one of Uranus

  • @carinajavier54
    @carinajavier54 Před 5 lety

    the pulsar is now a black hole

  • @BRAWGWill
    @BRAWGWill Před 8 lety

    Couldn't a type 1a supernova result from this?

    • @mouth7137
      @mouth7137 Před 7 lety

      Any Old Biscuit no only white dwarves makes type 1a supernovas

    • @BRAWGWill
      @BRAWGWill Před 7 lety

      Weed Beer What if neutron stars have a critical mass, though?

    • @mouth7137
      @mouth7137 Před 7 lety

      Any Old Biscuit they have

    • @BRAWGWill
      @BRAWGWill Před 7 lety

      So then a type 1a supernova could result.

    • @mouth7137
      @mouth7137 Před 7 lety

      Any Old Biscuit no it will just shrink into a black hole and release gamma rays

  • @pONtosanAz
    @pONtosanAz Před 9 lety

    !

  • @pratherat
    @pratherat Před 9 lety

    I suggest that before you make any more fancy graphics, you find out what is really happening in this interaction.

  • @tammyleederwhitaker649

    🎵🌌⌛

  • @jamesbeatty-wilson5290

    Transcripts from a sonic eonic

  • @julienzealator8006
    @julienzealator8006 Před 10 lety

    We provide the universe with valuable information about how life in some signature arrangement so that it an update, if it chooses to, the system's evidence to conform to it. We're gods, So shut up and start living like one.

  • @kharnakcrux2650
    @kharnakcrux2650 Před 9 lety

    that stream of gas is just damn beautiful. i kinda sorta made my own model of it in my own videos. I'll have to add some kind of mist effect. It's only my impression czcams.com/video/JaLmfgkla2w/video.html

  • @ryan56721
    @ryan56721 Před 9 lety

    Isn't this similar to how a Sun dies ???? It just sucks up everything into a neutron star or something like that ???????????? ............ IDK

  • @loveldlu426
    @loveldlu426 Před 5 lety

    It's something that Warner Brothers has never attacked him and we can understand why with Batman kids Batman should had kids suddenly he's in his right and then he needs these for kids he does not know that he's a father to these children their ages and somehow he women that he was dating Sonic came forward and told him these your kids first he's upset mixed up mad all confusion at once then after he process it he comes down and start to get to know his children that he never raised now you can understand why still bringing more fans for Batman new Once upgraded to a new level

  • @JohnSmith-ji9bw
    @JohnSmith-ji9bw Před 2 lety

    .

  • @potatomanboooi3105
    @potatomanboooi3105 Před 3 lety

    transformers robots in discuise

  • @killzy7636
    @killzy7636 Před 3 lety

    Who easel is here in 2021

  • @26071984g
    @26071984g Před 9 lety

    is the wedding of two stars

  • @j3i3m333
    @j3i3m333 Před 10 lety

    I only came here when i saw "Transformer signal".

  • @zes7215
    @zes7215 Před 7 lety

    wrong

  • @tombowen8091
    @tombowen8091 Před 4 lety

    turn that stupid music off , please

  • @tanerollins4705
    @tanerollins4705 Před 9 lety +6

    Amazing what God made for us to witness.

  • @MarceloTurby
    @MarceloTurby Před 9 lety

    we are tired of yur computer generated images. Just take the real pictures and show them to the world. its discouraging that people needs to use their imagination for us to see something cool from NASA. You guys are so boring. i guess thats you want.

    • @joshuachioco7615
      @joshuachioco7615 Před 8 lety

      oh silly, you cant view a pulsar in atelescope in a 4,004 light years away

    • @joshuachioco7615
      @joshuachioco7615 Před 8 lety

      you can detect them by an infrared telescope but you cant pan in it