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Keyword: kilonova

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  • James Webb Space Telescope finds neutron star mergers forge gold in the cosmos: 'It was thrilling'

    02/21/2024 8:26:51 PM PST · by Red Badger · 24 replies
    SPACE.com ^ | 21 FEB 2024 | By Robert Lea
    "This is the first time we've been able to verify that metals heavier than iron and silver were freshly made in front of us." An illustration of two neutron stars colliding and merging to create a kilonova blast. (Image credit: Robin Dienel/Carnegie Institution for Science) Scientists have analyzed an unusually long blast of high-energy radiation, known as a gamma-ray burst (GRB), and determined that it originated from the collision of two ultradense neutron stars. And, importantly, this result helped the team observe a flash of light emanating from the same event that confirms these mergers are the sites that create...
  • Cosmic Gold Factory: Single Kilonova Produced 1,000x the Mass of the Earth in Very Heavy Elements

    08/09/2023 1:06:39 PM PDT · by Red Badger · 11 replies
    Scitech Daily ^ | AUGUST 8, 2023 | By UNIVERSITY OF BIRMINGHAM
    Artist’s impression of GRB 211211A. Scientists have linked this unusual gamma-ray burst from a nearby galaxy to a neutron star merger. Credit: Soheb Mandhai @TheAstroPhoenix An unusually powerful gamma-ray burst (GRB 211211A), detected from a nearby galaxy, has been linked to a neutron star merger by an international team of scientists. This burst, notable for its excess of infrared light, was shown to originate from a kilonova, an event thought to occur when neutron stars collide. Scientists have linked a highly unusual blast of high-energy light from a nearby galaxy to a neutron star merger. The event, detected in December...
  • Here’s Something Strange, the Afterglow From Last Year’s Kilonova is Continuing to Brighten

    01/23/2018 9:22:31 AM PST · by BenLurkin · 15 replies
    Universe Today ^ | 01/2202018 | Matt Williams
    X-ray observations are consistent with radiowave data reported last month by another team of scientists, who also indicated that it was continuing to brighten during the three months since the collision. During this same period, X-ray and optical observatories were unable to monitor GW170817/GRB because it was too close to the Sun at the time. However, once this period ended, Chandra was able to gather data again, which was consistent with these other observations. As John Ruan explained: “When the source emerged from that blind spot in the sky in early December, our Chandra team jumped at the chance to...