Astronomers have tracked down the source of a gravitational wave and discovered the first observed kilonova: a nuclear furnace 100 million times brighter than the Sun producing thousands of times the entire mass of the Earth in heavy elements such as precious metals.
press released on October 16, 2017 by Ìý
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Three-color false-color composite images showing the time evolution of the optical and near-infrared counterpart of GW170817 made using data from the Subaru Telescope (z-band, blue) and IRSF (H-band, green; Ks-band, red).
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On August 17, 2017 the LIGO-Virgo collaboration alerted more than 90 astronomy teams around the world, that they had detected a signal (GW170817) consistent with the inspiral and merger of two neutron stars. Raffaele Flaminio (NAOJ and CNRS/LAPP), a scientist from the Virgo and KAGRA collaborations, explains that "Thanks to the combination of the data from the LIGO detectors in the US and the Virgo detector in Europe, this was the best ever localized gravitational wave source."
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J-GEM (Japanese collaboration of Gravitational wave Electro-Magnetic follow-up) is a research project to search for optical counterparts of gravitational wave sources because optical observations give us different information than gravitational wave observations. Indeed multi-messenger astronomy, observing the same phenomenon with both gravitational waves and normal light, is needed to paint the full picture of the phenomenon.
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Neutron star mergers are expected to have strong optical and infrared light emissions, so J-GEM sprang in to action. Using a network of telescopes around the world, including the Subaru Telescope in Hawai'i and the 1.4-m IRSF telescope in South Africa (run by ÅÝܽÊÓƵ and Kagoshima University), they observed the source located 130 million light-years away in the constellation Hydra, trying to discern its true nature. As they watched the object change day by day, they realized that they were observing the first ever confirmed kilonova.
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Astronomers have long searched for sites in the Universe where the heavy elements were produced by rapid neutron capture (r-process) reactions. One possible candidate was kilonova explosions which are predicted to produce 10,000 times the mass of the Earth in rare earth elements and precious metals.
The time evolution of the color and brightness of the object at the origin of the gravitational waves were too rapid to be a supernova, but matched the simulations of a kilonova made by the ATERUI supercomputer at the National Astronomical Observatory of Japan.
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"We were so excited to see the rapid brightness evolution revealed day by day through observations at facilities operated by Japanese institutes distributed all over the world." said Yousuke Utsumi (Hiroshima University), a scientist in the J-GEM collaboration.
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Artist's impression of the GW170817 kilonova.
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Article:
1.Ìý Yousuke Utsumi, Masaomi Tanaka,...Fumio Abe, et al., "J-GEM observations of an electromagnetic counterpart to the nertron star merger GW170817",ÌýPublications of the Astronomical Society of Japan, DOI:
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2.ÌýÌýMasaomi Tanaka, Yousuke Utsumi...Fumio Abe, et al., "Kilonova from post-merger ejecta as an optical and near-infrared counterpart of GW170817",ÌýPublications of the Astronomical Society of Japan, DOI:
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Fumio Abe is an Associate Professor of , ÅÝܽÊÓƵ
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Related Links:
, located at Suhterland, South Africa (run by ÅÝܽÊÓƵ and Kagoshima University)
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,ÌýNational Astronomical Observatory of Japan (NAOJ)
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,ÌýCenter for Computational Astrophysics, NAOJ
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, Gravitational Wave Project Office, NAOJ
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, School of Science, University of Tokyo
