<?xml version='1.0' encoding='UTF-8'?><metadata xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns="http://dublincore.org/documents/dcmi-terms/"><dcterms:title>Simulation data on the long-term evolution of the Solar System following a stellar flyby</dcterms:title><dcterms:identifier>https://doi.org/10.26165/JUELICH-DATA/LGBORQ</dcterms:identifier><dcterms:creator>Wagner, Frank W.</dcterms:creator><dcterms:creator>Pfalzner, Susanne</dcterms:creator><dcterms:publisher>Jülich DATA</dcterms:publisher><dcterms:issued>2025-09-10</dcterms:issued><dcterms:modified>2025-11-05T08:50:58Z</dcterms:modified><dcterms:description>Simulation data are provided on the long-term evolution of the Solar System following a stellar flyby. The simulation begins at 12,000 years after the periastron passage of a perturber star and models the Sun and the four giant planets, tracking the orbital paths of several thousand massless test particles over 1 Gyr. The data can be used for visualising particle properties. The data are openly available via the DESTINY project.</dcterms:description><dcterms:subject>Astronomy and Astrophysics</dcterms:subject><dcterms:language>English</dcterms:language><dcterms:isReferencedBy>Pfalzner, S., Wagner, F. W. &amp; Gibbon, P. Trans-Neptunian Object Colors as Evidence for a Past Close Stellar Flyby to the Solar System. ApJL 992, L32 (2025)., doi, 10.3847/2041-8213/ae0e74</dcterms:isReferencedBy><dcterms:contributor>Wagner, Frank</dcterms:contributor><dcterms:dateSubmitted>2025-08-01</dcterms:dateSubmitted><dcterms:relation>Wagner, Frank W.; Pfalzner, Susanne, 2025, "Simulation data on the effects of a stellar encounter on the protoplanetary disk of the early Solar System", https://doi.org/10.26165/JUELICH-DATA/9Z9K47, Jülich DATA, V1</dcterms:relation><dcterms:type>Simulation Data</dcterms:type><dcterms:license>CC0</dcterms:license><dcterms:rights>CC0 Waiver</dcterms:rights></metadata>