Rare Earth Element Synthesis Confirmed In Neutron Star Mergers

Eddie Gonzales Jr. – MessageToEagle.com – A group of researchers has, for the first time, identified rare earth elements produced by neutron star mergers.

When two neutron stars spiral inwards and merge, the resulting explosion produces a large amount of the heavy elements that make up our universe.

 two neutron stars spiral inwards and merge, the resulting explosion produces a large amount of the heavy elements that make up our universe. The first confirmed example of this process was an event in 2017 named GW 170817. Yet, even now five years later, identifying the specific elements created in neutron star mergers has eluded scientists, except for strontium identified in the optical spectra. A research group led by Nanae Domoto, a graduate student at the Graduate School of Science at Tohoku University and a research fellow at the Japan Society for the Promotion of Science (JSPS), has systematically studied the spectra from this kilonova—bright emissions caused by the radioactive decay of freshly synthesized nuclei that were ejected during the GW 170817 merger. Based on comparisons of detailed kilonovae spectra simulations produced by the supercomputer ATERUI II at the National Astronomical Observatory of Japan, the team found that the rare earth elements lanthanum and cerium can reproduce the near-infrared spectral features seen in 2017. Until now, the existence of rare earth elements has only been hypothesized based on the overall evolution of the brightness of the kilonova, but not confirmed from the spectral features. "This is the first direct identification of rare elements in the spectra of neutron star mergers, and it advances our understanding of the origin of elements in the universe," Dotomo said. "This study used a simple model of ejected material. Looking ahead, we want to factor in multi-dimensional structures to grasp a bigger picture of what happens when stars collide," Dotomo added. These results appeared as Domoto et al, "Lanthanide Features in Near-infrared Spectra of Kilonovae" in The Astrophysical Journal on October 26, 2022. Explore further First identification of a heavy element born from neutron star collision More information: Nanae Domoto et al, Lanthanide Features in Near-infrared Spectra of Kilonovae, The Astrophysical Journal (2022). DOI: 10.3847/1538-4357/ac8c36. iopscience.iop.org/article/10. … 847/1538-4357/ac8c36 Journal information: Astrophysical Journal Provided by National Astronomical Observatory of Japan Facebook Twitter Email Feedback to editors Featured Last Comments Popular Electrons with Planckian scattering in strange metals follow standard rules of orbital motion in a magnet 11 HOURS AGO 0 Synthesizing quantum nanomagnets via metal-free multi-porphyrin systems 12 HOURS AGO 0 Whole body 3D images of avian skeletons highlight the role of ecology in evolution OCT 27, 2022 0 A molecular-based, finite-state machine OCT 27, 2022 0 KT Eridani is a recurrent nova, study finds OCT 27, 2022 0 NASA's Lunar Flashlight ready to search for the Moon's water ice 7 HOURS AGO Artificial intelligence and molecule machine join forces to generalize automated chemistry 8 HOURS AGO Heat waves driven by climate change have cost global economy trillions since the 1990s 9 HOURS AGO Researchers design soil-inspired multifunctional chemical system 10 HOURS AGO Breakthrough in CRISPR research may lead to more effective and safer gene editing 11 HOURS AGO Safe, sustainable photo-on-demand synthesis of polypeptide precursors 11 HOURS AGO Hubble captures rare 'light echo' from star explosion 11 HOURS AGO Relevant PhysicsForums posts The James Webb Space Telescope 3 HOURS AGO Our Beautiful Universe - Photos and Videos OCT 27, 2022 Solar Activity and Space Weather Update thread OCT 25, 2022 Hydrostatic pressure in a bottle of water on ISS OCT 24, 2022 Ivuna meteorite from edge of solar system to Tanzania? OCT 22, 2022 Would light travel in a circle at the edge of the observable Universe? OCT 22, 2022 More from Astronomy and Astrophysics 1 2 Medical Xpress Medical research advances and health news Tech Xplore The latest engineering, electronics and technology advances Science X The most comprehensive sci-tech news coverage on the web Newsletters Email Science X Daily and the Weekly Email Newsletter are free features that allow you to receive your favorite sci-tech news updates in your email inbox Follow us Top Home Search Mobile version Help FAQ About Contact Science X Account Sponsored Account Archive News wire Android app iOS app RSS feeds Push notification © Phys.org 2003 - 2022 powered by Science X Network Privacy policy Terms of use 1 / 1Artist’s conception of a neutron star merger and the resulting kilonova. Credit: Tohoku University

Artist’s conception of a neutron star merger and the resulting kilonova. Credit: Tohoku University

The first confirmed example of this process was an event in 2017 named GW 170817. Yet, even now five years later, identifying the specific elements created in neutron star mergers has eluded scientists, except for strontium identified in the optical spectra.

A research group led by Nanae Domoto, a graduate student at the Graduate School of Science at Tohoku University and a research fellow at the Japan Society for the Promotion of Science (JSPS), has systematically studied the spectra from this kilonova—bright emissions caused by the radioactive decay of freshly synthesized nuclei that were ejected during the GW 170817 merger.

Based on comparisons of detailed kilonovae spectra simulations produced by the supercomputer ATERUI II at the National Astronomical Observatory of Japan, the team found that the rare earth elements lanthanum and cerium can reproduce the near-infrared spectral features seen in 2017.

Until now, the existence of rare earth elements has only been hypothesized based on the overall evolution of the brightness of the kilonova, but not confirmed from the spectral features.

“This is the first direct identification of rare elements in the spectra of neutron star mergers, and it advances our understanding of the origin of elements in the universe,” Dotomo said.

“This study used a simple model of ejected material. Looking ahead, we want to factor in multi-dimensional structures to grasp a bigger picture of what happens when stars collide,” Dotomo added.

These results appeared as Domoto et al, “Lanthanide Features in Near-infrared Spectra of Kilonovae” in The Astrophysical Journal on October 26, 2022.

Written by Eddie Gonzales Jr. – MessageToEagle.com Staff