{"id":83423,"date":"2025-03-20T14:28:27","date_gmt":"2025-03-20T13:28:27","guid":{"rendered":"https:\/\/helloproject.es\/vigilancia\/descubren-oxigeno-en-la-galaxia-mas-lejana-conocida\/"},"modified":"2025-03-20T14:28:27","modified_gmt":"2025-03-20T13:28:27","slug":"descubren-oxigeno-en-la-galaxia-mas-lejana-conocida","status":"publish","type":"post","link":"https:\/\/helloproject.es\/vigilancia\/descubren-oxigeno-en-la-galaxia-mas-lejana-conocida\/","title":{"rendered":"Descubren ox\u00edgeno en la galaxia m\u00e1s lejana conocida"},"content":{"rendered":"<p>Descubierta el a\u00f1o pasado, <a href=\"https:\/\/www.agenciasinc.es\/Noticias\/El-Webb-detecta-la-galaxia-muerta-mas-antigua-conocida\" target=\"_blank\">JADES-GS-z14-0<\/a> es la galaxia confirmada m\u00e1s distante que se ha observado hasta ahora: est\u00e1 tan lejos que su luz tard\u00f3 13 400 millones de a\u00f1os en llegar a la Tierra, lo que significa que se ve tal y como era cuando el universo ten\u00eda menos de 300 millones de a\u00f1os, aproximadamente el 2 % de su edad actual.<\/p>\n<p>La nueva detecci\u00f3n de ox\u00edgeno con\u00a0<a href=\"https:\/\/www.eso.org\/public\/spain\/teles-instr\/alma\/\" target=\"_blank\">ALMA<\/a>, un conjunto de telescopios instalado en el desierto de Atacama, en Chile, sugiere que la galaxia es qu\u00edmicamente mucho m\u00e1s madura de lo esperado.<\/p>\n<p><img decoding=\"async\" src=\"https:\/\/www.agenciasinc.es\/bundles\/app\/images\/quotebefore.png\" \/><\/p>\n<p>Los resultados muestran que la galaxia se ha formado muy r\u00e1pidamente<\/p>\n<p>Sander Schouws, Observatorio de Leiden<br \/>\n<img decoding=\"async\" src=\"https:\/\/www.agenciasinc.es\/bundles\/app\/images\/quoteafter.png\" \/><\/p>\n<p>\u201cEs como encontrar a un adolescente donde solo esperar\u00edas encontrar beb\u00e9s\u201d, declara Sander Schouws, doctorando en el Observatorio de Leiden (Pa\u00edses Bajos) y primer autor de uno de los estudios que han descrito el hallazgo, este publicado en\u00a0The Astrophysical Journal. \u201cLos resultados muestran que la galaxia se ha formado muy r\u00e1pidamente y tambi\u00e9n est\u00e1\u00a0madurando a gran velocidad\u201d, a\u00f1ade.<\/p>\n<p><a><\/a><\/p>\n<h2>Primero hidr\u00f3geno y helio<\/h2>\n<p>Las galaxias suelen comenzar su vida cargadas de estrellas j\u00f3venes, formadas principalmente por elementos ligeros como el hidr\u00f3geno y el helio. A medida que las estrellas evolucionan, crean elementos m\u00e1s pesados como el ox\u00edgeno, que se dispersan por su galaxia anfitriona despu\u00e9s de morir.<\/p>\n<p>La comunidad cient\u00edfica pensaba que, cuando el universo ten\u00eda unos 300 millones de a\u00f1os, a\u00fan era demasiado joven para contener galaxias llenas de elementos pesados. Sin embargo, los dos estudios de ALMA indican que JADES-GS-z14-0 tiene aproximadamente 10 veces m\u00e1s elementos pesados de lo esperado.<\/p>\n<p>                    <img decoding=\"async\" src=\"https:\/\/cdn.agenciasinc.es\/var\/ezwebin_site\/storage\/images\/_aliases\/img_1col\/media\/images\/galaxia-jade\/12223910-1-esl-MX\/galaxia-jade.jpg\" alt=\"Reproducci\u00f3n art\u00edstica de la galaxia JADES-GS-z14-0. \/ ESO | M. Kornmesser\" \/><\/p>\n<p>Reproducci\u00f3n art\u00edstica de la galaxia JADES-GS-z14-0. \/ ESO | M. Kornmesser<\/p>\n<p>    document.addEventListener(\u00abDOMContentLoaded\u00bb, function() {<br \/>\n        var img = document.querySelector(&#8216;.image-container img&#8217;);<br \/>\n        if (img) {<br \/>\n            img.alt = \u00abReproducci\u00f3n art\u00edstica de la galaxia JADES-GS-z14-0. \/ ESO | M. Kornmesser\u00bb;<br \/>\n        }<br \/>\n    });<\/p>\n<p>\u201cEstos resultados abren una nueva visi\u00f3n sobre las primeras fases de la evoluci\u00f3n de las galaxias\u201d, afirma Stefano Carniani, de la Escuela Normal Superiore de Pisa (Italia) y autor principal del art\u00edculo publicado en\u00a0Astronomy &amp; Astrophysics.<\/p>\n<p>La detecci\u00f3n de ox\u00edgeno tambi\u00e9n ha permitido a la comunidad astron\u00f3mica hacer que sus mediciones de distancia a JADES-GS-z14-0 sean mucho m\u00e1s precisas.<\/p>\n<p>Referencias:<\/p>\n<p>Stefano Carniani et al. \u201cThe eventful life of a luminous galaxy at z=14: metal enrichment, feedback, and low gas fraction?\u201d. <a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/202452451\" target=\"_blank\">Astronomy &amp; Astrophysics<\/a> (2025).<\/p>\n<p>Sander Schouws et al. \u201cDetection of [OIII]88\u00b5m in JADES-GS-z14-0 at z=14.1793\u201d. The Astrophysical Journal.<\/p>","protected":false},"excerpt":{"rendered":"<p>Descubierta el a\u00f1o pasado, JADES-GS-z14-0 es la galaxia confirmada m\u00e1s distante que se ha observado hasta ahora: est\u00e1 tan lejos que su luz tard\u00f3 13 400 millones de a\u00f1os en llegar a la Tierra, lo que significa que se ve tal y como era cuando el universo ten\u00eda menos de 300 millones de a\u00f1os, aproximadamente [&hellip;]<\/p>\n","protected":false},"author":5,"featured_media":0,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"default","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","ast-disable-related-posts":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"footnotes":""},"categories":[5],"tags":[],"class_list":["post-83423","post","type-post","status-publish","format-standard","hentry","category-noticias"],"yoast_head":"<!-- This site is optimized with the Yoast SEO Premium plugin v20.9 (Yoast SEO v27.4) - 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