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Science

Astronomers Strike Gravitational Gold In Colliding Neutron Stars (npr.org) 109

For the first time, scientists have caught two neutron stars in the act of colliding, revealing that these strange smash-ups are the source of heavy elements such as gold and platinum. From a report: The discovery, announced today at a news conference and in scientific reports written by some 3,500 researchers, solves a long-standing mystery about the origin of these heavy elements -- which are found in everything from wedding rings to cellphones to nuclear weapons. It's also a dramatic demonstration of how astrophysics is being transformed by humanity's newfound ability to detect gravitational waves, ripples in the fabric of space-time that are created when massive objects spin around each other and finally collide. "It's so beautiful. It's so beautiful it makes me want to cry. It's the fulfillment of dozens, hundreds, thousands of people's efforts, but it's also the fulfillment of an idea suddenly becoming real," says Peter Saulson of Syracuse University, who has spent more than three decades working on the detection of gravitational waves. Albert Einstein predicted the existence of these ripples more than a century ago, but scientists didn't manage to detect them until 2015. Until now, they'd made only four such detections, and each time the distortions in space-time were caused by the collision of two black holes. That bizarre phenomenon, however, can't normally be seen by telescopes that look for light. Neutron stars, by contrast, spew out visible cosmic fireworks when they come together. These incredibly dense stars are as small as cities like New York and yet have more mass than our sun. Further reading: 'A New Rosetta Stone for Astronomy' (The Atlantic), and Gravitational Wave Astronomers Hit Mother Lode (Scientific American).
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Astronomers Strike Gravitational Gold In Colliding Neutron Stars

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  • by hey! ( 33014 ) on Monday October 16, 2017 @11:53AM (#55377823) Homepage Journal

    "Chance favors the prepared mind."

    This is an example of that at it's purest, the culmination of years of effort by hundreds of people, all for a moment that might not have happened in their lifetimes.

    • "Luck Is What Happens When Preparation Meets Opportunity" - Seneca

  • by jfdavis668 ( 1414919 ) on Monday October 16, 2017 @11:59AM (#55377861)
    I can't seem to find the result of the collision in any of the articles. Did they merge to form a black hole or a larger neutron star?
    • by Anonymous Coward on Monday October 16, 2017 @12:05PM (#55377929)

      This came up in the press conference, and at present they can't say either way. The merger product could be among the most massive neutron stars or lightest black holes.

      • It would be truly mind blowing if this created neither, but instead a strange/quark star.
      • Is it yuuuuge?

  • >>>"These incredibly dense stars are as small as cities like New York and yet have more mass than our sun."

    Please use standard units! How many football fields is that?
  • But no. Looks like that will been in about 4 hours. I am expecting to be disappointed. With the ESO website using terminology like, "ESO HQ Announcing Unprecedented Discovery" and "groundbreaking observations of an astronomical phenomenon that has never been witnessed before." It unusual for a scientific establishment to use wording like that. Crossing my fingers it will actually be something amazing. I imagine there will be a Slashdot headline.

    http://www.eso.org/public/anno... [eso.org]
    • It unusual for a scientific establishment to use wording like that.

      LOL. Every scientific announcement uses that exactly that kind of wording. BTW, here's the press release in question:https://www.eso.org/public/announcements/ann17075/

  • I thought gold was just created the same as everything else heavier than iron, in a supernova. So a quick google shows that colliding neutron stars would provide a new mechanism but it doesn't discount the old mechanism https://www.smithsonianmag.com... [smithsonianmag.com]

    • by Anonymous Coward

      The section of the Wikipedia article on supernova nucleosynthesis about the r-process [wikipedia.org] and the article on the r-process itself have a version of the periodic table showing the origin of each element.

      It shows merging neutron stars as the main source of gold, platinum, iodine and others, and the only source of bismuth, thorium and uranium.

    • I learned quite a bit about nucleosynthesis, but haven't revisited it in decades.

      There are three main processes for synthesizing heavy elements. In the s-process [wikipedia.org] (slow), neutrons are absorbed by heavy nuclei slowly enough that the nucleus has time to beta decay, if it is too neutron rich to be stable. The s-process happens in red giant stars, and the products can be released by stellar winds and planetary nebula formation.

      In the r-process [wikipedia.org] (rapid), neutrons are added very quickly to heavy nuclei, which absor

  • The actual news is that for the first time a collision event was detected with both gravitational waves and light simultaneously. The Atlantic article even has an image. This produced a wealth of knowledge, including how gold is created, alluded in the title.
    • "The Atlantic article even has an image."

      Kerry-Lee from Hull, Daily Mail, p. 3 , showed how two large orbs made her some gold.

      • Kerry-Lee from Hull, Daily Mail, p. 3 , showed how two large orbs made her some gold.

        All you need to do now is detect her gravitational waves.

  • A source, not the source. Kind of like how The Doctor from Doctor Who may be a Doctor but not the only doctor.
  • which are found in everything from wedding rings to cellphones to nuclear weapons.

    No, they're found in the ground. They're taken out of the ground and put in those other things.

  • It's pretty heavy stuff.

  • With an optical telescope, you just point it at the thing in the sky you want to watch. With a radio telescope, you get a much bigger collector than an optical lens, and you also point it in the sky at the thing you want to watch. I'm not quite sure how you know exactly what you're looking at with a radio telescope, particularly if the thing you're observing is not visible optically, but I can make a guess.

    But my question is, this neutron star collision was detected by the LIGO and Virgo gravitational wave

    • But my question is, this neutron star collision was detected by the LIGO and Virgo gravitational wave interferometers, which don't even point at anything. Do they find the location of the source of the wave by comparing its arrival at different sites, then somehow computing a physical location that must be the origin? Wouldn't you need several of these devices to pinpoint that source accurately? Finally, how do they know that the g wave they observed corresponds with neutron stars colliding, and not any of a variety of other kinds of events?

      The time delays between the three observatories are the main way to determine the source of a gravitational wave. More detectors allows for better localizing, with three being the minimum for a decent triangulation. But, there are other properties of the waves that can be used.

      Here's a good explanation: https://profmattstrassler.com/... [profmattstrassler.com]

      Today, we learned that [a neutron star merger] has happened. LIGO, with the world’s first two gravitational observatories, detected the waves from two merging neutron

As you will see, I told them, in no uncertain terms, to see Figure one. -- Dave "First Strike" Pare

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