<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-06-28T20:28:33Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/71964" metadataPrefix="qdc">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/71964</identifier><datestamp>2023-08-06T01:25:57Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_15</setSpec></header><metadata><qdc:qualifieddc xmlns:qdc="http://dspace.org/qualifieddc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://purl.org/dc/elements/1.1/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dc.xsd http://purl.org/dc/terms/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dcterms.xsd http://dspace.org/qualifieddc/ http://www.ukoln.ac.uk/metadata/dcmi/xmlschema/qualifieddc.xsd">
   <dc:title>The Closest Past Flyby of a Known Star to the Solar System: HD 7977, UCAC4 237-008148 or WISE J072003.20-084651.2?</dc:title>
   <dc:creator>Fuente Marcos, Raúl de la</dc:creator>
   <dc:creator>Fuente Marcos, Carlos de la</dc:creator>
   <dcterms:abstract>It is argued that the closest past flyby of a known star to the solar system was that of Scholz's star (WISE J072003.20-084651.2). Here, we show that the distribution of distances of closest approach of this star has a median value of 0.330 pc with a 90% probability of coming within 0.317–0.345 pc of the Sun; the associated time of perihelion passage is determined to be between 78.6–81.1 kyr ago with 90% confidence, with a most likely value of 79.9 kyr. Using Gaia DR3 data and the latest planetary ephemerides, we found that UCAC4 237-008148 (RUWE = 0.927) approached even closer with a median perihelion distance of 0.259 pc and a 90% confidence interval of 0.249–0.269 pc, 1.158 Myr ago. HD 7977 might have passed 0.15 pc from the Sun 2.77 Myr ago, but it has RUWE = 2.015.</dcterms:abstract>
   <dcterms:dateAccepted>2023-06-22T10:58:41Z</dcterms:dateAccepted>
   <dcterms:available>2023-06-22T10:58:41Z</dcterms:available>
   <dcterms:created>2023-06-22T10:58:41Z</dcterms:created>
   <dcterms:issued>2022-07</dcterms:issued>
   <dc:type>journal article</dc:type>
   <dc:identifier>https://hdl.handle.net/20.500.14352/71964</dc:identifier>
   <dc:identifier>2515-5172</dc:identifier>
   <dc:identifier>10.3847/2515-5172%2Fac842b</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:rights>https://creativecommons.org/licenses/by/3.0/es/</dc:rights>
   <dc:rights>open access</dc:rights>
   <dc:rights>Atribución 3.0 España</dc:rights>
   <dc:publisher>American Astronomical Society</dc:publisher>
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