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Second Gravitational Wave Detected From Ancient Black Hole Collision (theguardian.com) 220

An anonymous reader quotes a report from The Guardian: Physicists have detected ripples in the fabric of spacetime that were set in motion by the collision of two black holes far across the universe more than a billion years ago. The event marks only the second time that scientists have spotted gravitational waves, the tenuous stretching and squeezing of spacetime predicted by Einstein more than a century ago. The faint signal received by the twin instruments of the Laser Interferometer Gravitational Wave Observatory (LIGO) in the US revealed two black holes circling one another 27 times before finally smashing together at half the speed of light. The cataclysmic event saw the black holes, one eight times more massive than the sun, the other 14 times more massive, merge into one about 21 times heavier than the sun. In the process, energy equivalent to the mass of the sun radiated into space as gravitational waves. Writing in the journal Physical Review Letters on Wednesday, the LIGO team describes how a second rush of gravitational waves showed up in their instrument a few months after the first, at 3.38am UK time on Boxing Day morning 2015. An automatic search detected the signals and emailed the LIGO scientists within minutes to alert them. The latest signals arrived at the Livingston detector 1.1milliseconds before they hit the Hanford detector, allowing scientists on the team to roughly work out the position of the collision in the sky. In February, LIGO scientists officially announced the first-ever observation of gravity waves.
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Second Gravitational Wave Detected From Ancient Black Hole Collision

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  • Why did it take so long to detect these? I know that there have been plenty of experiments attempting to measure them before. Are the waves smaller than expect, thus harder to detect? What was the thing preventing discovery?
    • Re:Why? (Score:5, Informative)

      by Edis Krad ( 1003934 ) on Wednesday June 15, 2016 @11:03PM (#52326877)

      Are the waves smaller than expect, thus harder to detect?

      Indeed. They're very small. We're talking about a shift in space the size of a very small fraction of a proton [space.com]. So yes, with the current detectors they're pretty hard to detect.

      • Re:Why? (Score:5, Informative)

        by MightyMartian ( 840721 ) on Wednesday June 15, 2016 @11:33PM (#52326955) Journal

        The current detectors are the most sensitive instruments ever developed by humanity, and in and of themselves mark a major leap forward in technical ability.

      • Re:Why? (Score:5, Interesting)

        by quenda ( 644621 ) on Thursday June 16, 2016 @12:31AM (#52327149)

        But gravity waves are like elephants in your fridge compared to the problem of detecting gravity particles.

        a detector with the mass of Jupiter and 100% efficiency, placed in close orbit around a neutron star, would only be expected to observe one graviton every 10 years, ...

        https://en.wikipedia.org/wiki/... [wikipedia.org]

        • But I'm detecting gravitons all the time! I wouldn't be sitting in this seat if it wasn't for gravitons. I think someone misunderstood something here. Possibly me ;-)

    • Comment removed based on user account deletion
      • Larry Niven was a friend of Robert Forward [wikipedia.org], a physicist and aerospace engineer who made various proposals for gravity wave detectors and other over-the-horizon technologies throughout the 1960s to 1990s. He (Forward) is considered one of the doyens of "hard" SF. (As is Niven himself.)
    • Re:Why? (Score:5, Informative)

      by The Evil Atheist ( 2484676 ) on Wednesday June 15, 2016 @11:09PM (#52326901)
      It took so long because the signal is mind-bogglingly weak. No detector was sensitive enough or well designed enough to rule out false positives. The LIGO experiment is much more sensitive and a lot of effort put in to detect false positives (including some social engineering). The detectors also underwent a very extensive testing phase before they were considered ready. We also weren't sure how frequent these events were, but now we are expecting a few more events.

      But, it must be said indirect evidence of gravitational waves already were detected through the observation of two pulsars orbiting and closing in on each other at a rate predicted by the theory.
      • The LIGO experiment is much more sensitive and a lot of effort put in to detect false positives (including some social engineering).

        How can social engineering be useful at all in this case?

        • If I had to hazard a guess, with incredibly fine instruments, there's a risk of experimenter effect [wikipedia.org].

        • Re: Why? (Score:2, Informative)

          by Anonymous Coward

          They had a system to inject test data into the final stage analysis. The people doing it did it blind to publication ready point. Partly it was to ensure nobody leaked before the 'envelope was opened'.

      • We also weren't sure how frequent these events were, but now we are expecting a few more events.

        I'm no statistician, but assuming that the intervals between detectable events are exponentially distributed (seems reasonable to me), the fact that we detected the first event pretty quickly within a certain time period would seem to suggest that too high or too low values of lambda (not fitting the first successful observation) are unlikely.

    • Re:Why? (Score:5, Informative)

      by bjorniac ( 836863 ) on Wednesday June 15, 2016 @11:23PM (#52326923)

      Noise. All kinds of noise.

      The system is an interferometer - basically two lasers set up in a large L shape with mirrors (massive simplification). When the lengths of the arms are the same, the beams cancel, when they differ a signal is recorded.

      Now, the differences in length due to a gravitational wave is tiny, and the problem that kept LIGO from their detection is that there are huge numbers of sources of vibrations around the same frequencies as expected from gravitational waves that have far larger amplitudes. Thermal vibrations, for example, are a killer for experiments like this.

      The waves themselves have almost exactly the waveforms that were predicted - the template fits from simulations match amazingly well in terms of amplitudes, frequencies and their evolution. What stopped experiments like this from making the observation was simply a lack of technical skill to make a precise enough instrument. Following the development of LIGO over the last decade, this is precisely what everyone working on the project said - once the noise curve is reduced to form Advanced LIOG (recent upgrade) the noise would be sufficiently small than an integrated signal against a template would be clearly visible, and now it is.

      • And why isn't it detecting waves on a daily basis? The universe is supposed to contain billions of black holes.

        • LIGO is detecting the gravitational storm that happens when two black holes, each 10-30 times the mass of the sun, actually collide and merge. Standalone black holes shouldn't generate gravity waves unless disturbed by something massive close by.

          Orbital binary systems should generate gravity waves, but those would be a couple of orders of magnitude less powerful than two colliding black holes and LIGO isn't sensitive enough to detect those out of the noise.

          • Wouldn't it be able to detect weaker events if they happen closer to us?

            • Re: Why? (Score:5, Informative)

              by Bengie ( 1121981 ) on Thursday June 16, 2016 @07:24AM (#52328099)
              Yes, but it's how much weaker. For a brief moment, those two blackholes released more energy that the rest of the entire observable Universe, that includes all of those quasars. Even gamma ray bursts only outshine their local galaxy.
            • It detects weaker events all the time. They can detect the gardeners mowing the lawn outside. But the gardeners aren't interesting to astronomers, black holes are.
               

        • And why isn't it detecting waves on a daily basis? The universe is supposed to contain billions of black holes.

          The black hole merger that was first detected had a peak power output that was 50 times greater than the total power output of all the stars in the observable universe.

          The waves from that merger caused the arms of the LIGO detectors to differ in length by 0.000000000000000000001 meters, which is roughly like the earth getting wider by 10 protons.

          This latest merger involved less massive black holes which should mean it had a lot less peak power.

        • And why isn't it detecting waves on a daily basis? The universe is supposed to contain billions of black holes.

          I went to a talk by one of the LIGO scientists where pretty much this questions was asked.

          It's a simple answer. Two black holes colliding is fantastically rare, but very the universe is fantastically big, so it happens a hell of a lot if it happens at all.
          The LIGO experiment is limited by noise and can 'see' out to some distance. So all the events happening within the sphere of that radius get detected. The rate of detection is a function of the radius of detection. The rate of detection tells us something

      • For a while I was starting to wonder if we would need space-based interferometers to solve the noise/vibration problem. But fortunately that wasn't needed.

    • The waves aren't smaller than expected, this recent upgrade is actually the first time they had an instrument they thought would be sensitive enough to detect a gravity wave.

  • Is it just me or black holes just slightly bigger than the sun sound small?
    • Provided that if the Sun were to become a black hole, its diameter would only be 6 km ... (ie 200,000 times less), the thing that gives a current-Sun size black hole is gigantic! (one [space.com] two [windows2universe.org]).
      • To be precise, it's size would be zero. It's a singularity, no actual size.

        The diameter given when describing size of a black hole is the diameter of event horizon created by the black hole. It's still just "empty space", but that's a point-of-no-return, and whatever's inside, will not escape (minus Hawking Radiation, but that's nitpicking) and that's an important characteristic that describes a limit beyond which everything is "as good as inside the black hole", the 3km from the center not doing a squat of

        • by Rob Riggs ( 6418 )
          Unless you have a testable theory to show that its size is is anything less than the event horizon, you just have faith that its size is 0 and nothing more.
        • It's unlikely there is a literal singularity at the center of a black hole, but we have no theories that can make sense of what's actually going on beyond the event horizon.

    • Is it just me or black holes just slightly bigger than the sun sound small?

      I think it's a reference to the overall idea there are two size ranges of black holes. Small (stellar) and super massive. For technical reasons there seem to be a lack of many holes in the 100 to 100k solar mass size range. Supermassive mergers are thought to happen sometime after galaxies merge, but this is far less common than thier smaller counterpart mergers. Intermediate holes seem to be quite rare. [wikipedia.org]

      • by Maritz ( 1829006 )
        It could be that intermediates are just very hard to spot with conventional astronomy. Judging by the results of LIGO so far, we might be starting to "see" a more expected amount.
  • there are two detectors not one, one is based in Australia the other in the USA. Also many of the parts used in both sensor arrays were designed and created in Australia.

    https://en.wikipedia.org/wiki/AIGO
    • by dargaud ( 518470 )
      And what about VIRGO in Italy which is also part of the collaboration ? It was offline during the 1st detection; did it catch it this time ?
    • Re: (Score:3, Informative)

      by Anonymous Coward

      There are three main detectors; two in the USA (LIGO) and one in Italy (Virgo). Currently, a detector is under construction in Japan and a fifth one using LIGO components will be built in India. Additionally, there is a smaller detector in Germany that is only sensitive in higher frequencies. It is mainly used to test technology, but it is also used for certain types of sources.

      Having multiple detectors is very useful, because coincidence is used to determine the sky position. A single detector can only det

  • Every time they get closer to the design sensitivity the detector can spot signals coming from farther away, as the wave amplitude follows the inverse square law.

    This increase in range will result in a great increase in the _volume_ they can observe, and remember that these detectors do not need to be pointed they way telescopes do.

    The project can clearly follow the Type 1a supernova project (which brought the Nobel Prize to Saul Perlmutter) and go from detecting one signal every few months to detecting a f

    • by TMB ( 70166 )

      Counter-intuitively, the strain amplitude goes as the inverse of the distance, not the inverse square!

      • by TMB ( 70166 )

        Actually, let me rephrase that -- it's not counter-intuitive at all that amplitude goes as 1/r, but what's odd is that with gravitational waves, you directly detect the wave amplitude, so detectability falls off as 1/r. For most waves, you detect the wave intensity, which goes as amplitude squared and therefore 1/r^2.

  • I guess I wouldn't want to observe something like that if i was only a light year away.

  • "Collision" might be a bit of a stretch. It implies immediacy. I didn't RTFA and I am no physicist, however I expect that the "Collision" took an extraordinary amount of time (galactic even as opposed to geologic time periods). Millions of years maybe? I have no idea. Seems if that is the case the summary is a bit sensational, in that it could more accurately be described as the waves of two black holes that slowly eventually merged into one... The end may have happened a lot quicker I suppose, but the lead

    • Yes, the black holes had been circling each other for billions of years and slowly leaking energy in the form of gravity waves which resulted in them gradually moving towards each other. As their orbits tightened their orbital velocities increased and it was only in the very last fraction of a second before this long process ended that they were orbiting fast enough to create waves we could detect.

  • Both supposed gravitational wave detections were >400 megaparsecs (1.3 billion light years) distant. That is really, really far.

    For example, the CfA2 Great Wall [wikipedia.org] of galaxies is only 300 million light years from Earth.

    Are there really no black hole collisions happening closer to us? Are these really so rare?

    • We are only detecting the last split second of a multi billion year process, so yeah pretty rare that the orbiting black holes are in a detectable state.

  • These gravity waves were not from two black holes colliding. It was just Chuck Norris doing push-ups again.

Stellar rays prove fibbing never pays. Embezzlement is another matter.

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