{"id":1590,"date":"2024-05-03T15:39:39","date_gmt":"2024-05-03T15:39:39","guid":{"rendered":"https:\/\/nucleomilenioeris.cl\/?p=1590"},"modified":"2024-05-03T15:39:46","modified_gmt":"2024-05-03T15:39:46","slug":"determinando-la-edad-de-las-estrellas","status":"publish","type":"post","link":"https:\/\/nucleomilenioeris.cl\/es\/news\/determinando-la-edad-de-las-estrellas\/","title":{"rendered":"Determinando la edad de las estrellas"},"content":{"rendered":"<p>Un reciente estudio titulado &#8220;<a href=\"https:\/\/arxiv.org\/abs\/2401.02328\">Exploring the dependence of chemical traits on metallicity: chemical trends for red giant stars with asteroseismic ages<\/a>&#8221; ha arrojado luz sobre la determinaci\u00f3n de la edad de las estrellas a trav\u00e9s de sus&nbsp; abundancias qu\u00edmicas. La investigaci\u00f3n, liderada por la cient\u00edfica Sara Vitali, ha utilizado un m\u00e9todo que se basa en la medici\u00f3n de las abundancias qu\u00edmicas de estrellas individuales mediante espectroscop\u00eda, revelando as\u00ed informaci\u00f3n crucial sobre su edad.<\/p>\n\n\n\n<p>Seg\u00fan la autora principal del estudio, &#8220;La edad es algo que en una estrella es mucho m\u00e1s dif\u00edcil de medir, porque se debe tener conocimiento de la masa, del radio, de propiedades mucho m\u00e1s dif\u00edciles de lograr&#8221;. Sin embargo, mediante el an\u00e1lisis de elementos qu\u00edmicos presentes en las estrellas, se puede inferir su edad de manera emp\u00edrica, proporcionando una herramienta poderosa para la investigaci\u00f3n astron\u00f3mica.<\/p>\n\n\n\n<p>El estudio se centr\u00f3 en estrellas cercanas, particularmente aquellas dentro del disco de nuestra galaxia y en proximidades al Sol. Estas estrellas fueron observadas desde Chile, utilizando el telescopio VLT del observatorio Paranal, perteneciente a la ESO. Los datos utilizados en el estudio fueron recolectados y analizados por el equipo de investigaci\u00f3n, desde la observaci\u00f3n hasta la fase de an\u00e1lisis.<\/p>\n\n\n\n<p>&#8220;Detr\u00e1s de un paper siempre hay m\u00e1s gente de la que aparece&#8221;, se\u00f1ala la autora principal, destacando el trabajo colaborativo y el apoyo recibido durante el proceso de investigaci\u00f3n y redacci\u00f3n del art\u00edculo. El proyecto, que inici\u00f3 en febrero de 2023, pas\u00f3 por diversas etapas que incluyeron el an\u00e1lisis de datos, la redacci\u00f3n del paper y la revisi\u00f3n por pares, etapa en la que se encuentra actualmente el art\u00edculo.<\/p>\n\n\n\n<p>&#8220;Este paper confirma la idea de que el estudio qu\u00edmico de las estrellas para determinar su edad no es algo universal&#8221;, concluye la autora principal. &#8220;Estas relaciones no son universales, no se puede mirar cualquier tipo de estrella, en cualquier posici\u00f3n de la galaxia&#8221;, agrega, subrayando la importancia de considerar diversos factores como la posici\u00f3n de la estrella en la galaxia.<\/p>\n\n\n\n<p>Como primera autora, esta publicaci\u00f3n marca el segundo paper de la cient\u00edfica, quien tambi\u00e9n anticipa la pr\u00f3xima publicaci\u00f3n de otra investigaci\u00f3n en la que participa como segunda autora. El equipo actualmente se encuentra implementando comentarios para finalizar este pr\u00f3ximo trabajo, demostrando as\u00ed su continuo compromiso con el avance del conocimiento cient\u00edfico en el campo de la astrof\u00edsica.<\/p>","protected":false},"excerpt":{"rendered":"<p>Un reciente estudio titulado &#8220;Exploring the dependence of chemical traits on metallicity: chemical trends for red giant stars with asteroseismic ages&#8221; ha arrojado luz sobre la determinaci\u00f3n de la edad de las estrellas a trav\u00e9s de sus&nbsp; abundancias qu\u00edmicas. La investigaci\u00f3n, liderada por la cient\u00edfica Sara Vitali, ha utilizado un m\u00e9todo que se basa en [&hellip;]<\/p>","protected":false},"author":5,"featured_media":1591,"comment_status":"closed","ping_status":"open","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":"","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":"set","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":[6],"tags":[],"class_list":["post-1590","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-news"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v23.4 - https:\/\/yoast.com\/wordpress\/plugins\/seo\/ -->\n<title>Determinando la edad de las estrellas | ERIS<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/nucleomilenioeris.cl\/es\/news\/determinando-la-edad-de-las-estrellas\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Determinando la edad de las estrellas | ERIS\" \/>\n<meta property=\"og:description\" content=\"Un reciente estudio titulado &#8220;Exploring the dependence of chemical traits on metallicity: chemical trends for red giant stars with asteroseismic ages&#8221; ha arrojado luz sobre la determinaci\u00f3n de la edad de las estrellas a trav\u00e9s de sus&nbsp; abundancias qu\u00edmicas. 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