{"id":186319,"date":"2026-05-07T19:27:11","date_gmt":"2026-05-07T19:27:11","guid":{"rendered":"http:\/\/69fcb370e9313cddedb53478"},"modified":"2026-05-07T19:27:11","modified_gmt":"2026-05-07T19:27:11","slug":"el-universo-esta-lleno-de-agujeros-negros-imposibles-ahora-sabemos-por-que","status":"publish","type":"post","link":"https:\/\/sarmiento24h.com\/?p=186319","title":{"rendered":"El universo est\u00e1 lleno de agujeros negros \u201cimposibles\u201d. Ahora sabemos por qu\u00e9"},"content":{"rendered":"<p>Un equipo internacional de astrof\u00edsicos encontr\u00f3 evidencia de que el universo recicla agujeros negros para fusionarlos entre s\u00ed y formar otros m\u00e1s grandes. Las ondas gravitacionales registradas durante los \u00faltimos a\u00f1os muestran que algunos de los agujeros negros m\u00e1s pesados dentro de c\u00famulos estelares presentan se\u00f1ales claras de ser de \u201csegunda generaci\u00f3n\u201d, productos de colisiones pasadas y, por lo tanto, no pudieron nacer del colapso de una estrella masiva.<\/p>\n<h2>Los agujeros negros imposibles<\/h2>\n<p>La teor\u00eda evolutiva de las estrellas explica que, al final de la vida de las m\u00e1s masivas, su n\u00facleo se comprime hasta formar un punto tan denso que curva el espacio\u2011tiempo hasta el infinito. Este es el agujero negro cl\u00e1sico, con masas de entre 10 y 40 veces la del Sol. Tambi\u00e9n existen <a href=\"https:\/\/es.wired.com\/articulos\/los-agujeros-negros-supermasivos-dejaron-de-crecer-tan-rapido-como-antes-por-fin-sabemos-por-que\">los supermasivos<\/a>, en el centro de las galaxias, con millones o miles de millones de masas solares, cuyo origen se relaciona con procesos ocurridos en los primeros instantes del universo.<\/p>\n<p>Entre ambos extremos aparece una categor\u00eda en disputa: los agujeros negros de entre 40 y 100 masas solares. Resultan demasiado pesados para nacer <a href=\"https:\/\/es.wired.com\/articulos\/esta-estrella-gigante-se-convirtio-en-agujero-negro-sin-explotar-muestran-los-calculos\">tras la muerte de una estrella<\/a>, pero tampoco alcanzan las dimensiones necesarias para surgir del colapso de una nube gigantesca de materia. La f\u00edsica estelar convencional los considera \u201cimposibles\u201d, y aun as\u00ed aparecen con frecuencia en las detecciones.<\/p>\n<figure class=\"AssetEmbedWrapper-iJvQnD cOWUYC asset-embed\">\n<div class=\"AssetEmbedAssetContainer-fnduJP iaVSwI asset-embed__asset-container\"><span class=\"SpanWrapper-kFnjvc eKnjjD responsive-asset AssetEmbedResponsiveAsset-gaAbQ hXaxHA asset-embed__responsive-asset\"><picture class=\"ResponsiveImagePicture-jKunQM gjCCFj AssetEmbedResponsiveAsset-gaAbQ hXaxHA asset-embed__responsive-asset responsive-image\"><img decoding=\"async\" alt=\"Un agujero negro de tama\u00f1o \u201cnormal\u201d aislado en el espacio.\" loading=\"lazy\" class=\"ResponsiveImageContainer-dkeESL cQPiWi responsive-image__image\" srcset=\"https:\/\/media.es.wired.com\/photos\/69fcc8fde9313cddedb534f4\/master\/w_120,c_limit\/1877x1052.png 120w, https:\/\/media.es.wired.com\/photos\/69fcc8fde9313cddedb534f4\/master\/w_240,c_limit\/1877x1052.png 240w, https:\/\/media.es.wired.com\/photos\/69fcc8fde9313cddedb534f4\/master\/w_320,c_limit\/1877x1052.png 320w, https:\/\/media.es.wired.com\/photos\/69fcc8fde9313cddedb534f4\/master\/w_640,c_limit\/1877x1052.png 640w, https:\/\/media.es.wired.com\/photos\/69fcc8fde9313cddedb534f4\/master\/w_960,c_limit\/1877x1052.png 960w, https:\/\/media.es.wired.com\/photos\/69fcc8fde9313cddedb534f4\/master\/w_1280,c_limit\/1877x1052.png 1280w, https:\/\/media.es.wired.com\/photos\/69fcc8fde9313cddedb534f4\/master\/w_1600,c_limit\/1877x1052.png 1600w\" sizes=\"100vw\" src=\"https:\/\/media.es.wired.com\/photos\/69fcc8fde9313cddedb534f4\/master\/w_1600%2Cc_limit\/1877x1052.png\"><\/picture><\/span><\/div>\n<div class=\"CaptionWrapper-bpPcvW iDPSlt caption AssetEmbedCaption-eZIMNW gMgneI asset-embed__caption\" data-testid=\"caption-wrapper\" readability=\"6.5\"><span class=\"BaseText-fEwdHD CaptionText-cQpRdU kRTNAB hbiMYj caption__text\" readability=\"28\"><\/p>\n<p>Un agujero negro de tama\u00f1o \u201cnormal\u201d, aislado en el espacio.<\/p>\n<p><\/span><span class=\"BaseText-fEwdHD CaptionCredit-cUgOGk iQbGEh hRFzlA caption__credit\">Space Telescope Science Institute Office of Public Outreach<\/span><\/div>\n<\/figure>\n<p>Los astrof\u00edsicos proponen que estos agujeros negros pesados podr\u00edan formarse al sumar dos o m\u00e1s objetos ultradensos m\u00e1s peque\u00f1os. La idea resulta coherente, pero necesitaba pruebas y hasta hace relativamente poco, no exist\u00eda una forma de obtenerlas.<\/p>\n<p>Entonces entraron en escena los detectores de <a href=\"https:\/\/es.wired.com\/articulos\/el-universo-palpita-en-tus-atomos-las-ondas-gravitacionales-dejan-huella-en-la-luz-que-emites\">ondas gravitacionales<\/a>. Estos instrumentos usan l\u00e1seres para medir la microdistorsi\u00f3n del espacio\u2011tiempo generada por la colisi\u00f3n de objetos extremadamente densos. La primera detecci\u00f3n, en 2015, confirm\u00f3 una fusi\u00f3n entre agujeros negros. Desde entonces, cada nueva se\u00f1al permiti\u00f3 caracterizar mejor estas estructuras y revelar que estos choques ocurren con mucha m\u00e1s frecuencia de lo que imagin\u00e1bamos.<\/p>\n<h2>La firma de la segunda generaci\u00f3n<\/h2>\n<p>El estudio, publicado hoy en <a href=\"https:\/\/www.nature.com\/articles\/s41550-026-02847-0\"><em>Nature Astronomy<\/em><\/a>, analiz\u00f3 un cat\u00e1logo transitorio de ondas gravitacionales generado por los tres observatorios m\u00e1s importantes del mundo. La base de datos inclu\u00eda 153 detecciones confiables de fusiones de agujeros negros, y entre ellas, 34 correspond\u00edan a objetos especialmente pesados.<\/p>\n<p>Al comparar todas las se\u00f1ales, el equipo identific\u00f3 dos poblaciones distintas. Los agujeros negros m\u00e1s ligeros, de hasta unas 40 masas solares, mostraron giros peque\u00f1os y alineados, como se espera de objetos nacidos del colapso de una estrella. Pero a partir de cierto punto, alrededor de las 45 masas solares, apareci\u00f3 una poblaci\u00f3n completamente diferente: agujeros negros m\u00e1s pesados, que giran r\u00e1pido y en direcciones ca\u00f3ticas, una firma estad\u00edstica que solo puede surgir cuando el objeto ya particip\u00f3 en una fusi\u00f3n previa.<\/p>\n<p>\u201cEsta es la firma exacta que esperar\u00edas si los agujeros negros se fusionaran repetidamente en densos c\u00famulos estelares\u201d, dijo la doctora Isobel M. Romero-Shaw, coautora de la investigaci\u00f3n, en un <a data-offer-url=\"https:\/\/www.cardiff.ac.uk\/news\/view\/3043715-biggest-black-holes-built-up-in-busy-star-clusters-after-series-of-violent-merging-events,-research-finds\" class=\"external-link\" data-event-click=\"{&quot;element&quot;:&quot;ExternalLink&quot;,&quot;outgoingURL&quot;:&quot;https:\/\/www.cardiff.ac.uk\/news\/view\/3043715-biggest-black-holes-built-up-in-busy-star-clusters-after-series-of-violent-merging-events,-research-finds&quot;}\" href=\"https:\/\/www.cardiff.ac.uk\/news\/view\/3043715-biggest-black-holes-built-up-in-busy-star-clusters-after-series-of-violent-merging-events,-research-finds\" rel=\"nofollow noopener\" target=\"_blank\">comunicado<\/a> de la Universidad de Cardiff.<\/p>\n<hr>\n<div class=\"ContentCardEmbedWrapper-hkvhYu kMYDit content-card-embed content-card-embed--stacked\" data-testid=\"ContentCardEmbedWrapper\" readability=\"19.130136986301\">\n<div class=\"ContentCardEmbedImage-bqahne fjmzkP content-card-embed__image\" data-testid=\"ContentCardEmbedImage\"><span class=\"SpanWrapper-kFnjvc eKnjjD responsive-asset\"><picture class=\"ResponsiveImagePicture-jKunQM gjCCFj responsive-image\"><img decoding=\"async\" alt=\"choque de agujeros negros\" loading=\"lazy\" class=\"ResponsiveImageContainer-dkeESL cQPiWi responsive-image__image\" srcset=\"https:\/\/media.es.wired.com\/photos\/68754a0705023a285d95a46d\/master\/w_120,c_limit\/GettyImages-1807948647.jpg 120w, https:\/\/media.es.wired.com\/photos\/68754a0705023a285d95a46d\/master\/w_240,c_limit\/GettyImages-1807948647.jpg 240w, https:\/\/media.es.wired.com\/photos\/68754a0705023a285d95a46d\/master\/w_320,c_limit\/GettyImages-1807948647.jpg 320w, https:\/\/media.es.wired.com\/photos\/68754a0705023a285d95a46d\/master\/w_640,c_limit\/GettyImages-1807948647.jpg 640w\" sizes=\"100vw\" src=\"https:\/\/media.es.wired.com\/photos\/68754a0705023a285d95a46d\/master\/w_775%2Cc_limit\/GettyImages-1807948647.jpg\"><\/picture><\/span><\/div>\n<div class=\"ContentCardEmbedInfo-buyHWH gWLOee\" readability=\"20.041095890411\">\n<div class=\"BaseText-fEwdHD ContentCardEmbedHed-kDKGDs fUtEc dlHXUJ content-card-embed__hed\" data-testid=\"ContentCardEmbedHed\"><a class=\"BaseLink-haTOKm ContentCardEmbedHedLink-iBZsco gAoKdC hhUFQU content-card-embed__hed-link link\" href=\"https:\/\/es.wired.com\/articulos\/astronomos-han-detectado-el-choque-de-los-agujeros-negros-mas-masivos-hasta-la-fecha\" data-testid=\"ContentCardEmbedHedLink\">Astr\u00f3nomos han detectado el choque de los agujeros negros m\u00e1s masivos hasta la fecha<\/a><\/div>\n<p>La red de observatorios de ondas gravitacionales confirm\u00f3 el choque de dos agujeros negros de entre 100 y 140 veces la masa del Sol.<\/p>\n<\/div>\n<\/div>\n<hr>\n<p>Hasta ahora no hemos observado directamente ninguno de estos agujeros negros \u201cimposibles\u201d. No aparecen en rayos X ni en el espectro visible, a diferencia de los supermasivos. Sin embargo, sabemos que existen porque sus colisiones hacen vibrar el espacio\u2011tiempo, y esa vibraci\u00f3n revela masas que la f\u00edsica estelar no puede explicar.<\/p>\n<p>Este estudio muestra que los agujeros negros m\u00e1s pesados se construyen en lugar de nacer. Surgen de generaciones previas de colisiones, ensamblados en los entornos m\u00e1s densos del cosmos.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Un equipo internacional de astrof\u00edsicos encontr\u00f3 evidencia&#46;&#46;&#46;<\/p>\n","protected":false},"author":1,"featured_media":186320,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_jetpack_memberships_contains_paid_content":false,"footnotes":"","jetpack_publicize_message":"","jetpack_publicize_feature_enabled":true,"jetpack_social_post_already_shared":true,"jetpack_social_options":{"image_generator_settings":{"template":"highway","default_image_id":0,"font":"","enabled":false},"version":2}},"categories":[46],"tags":[],"class_list":["post-186319","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-tecnologia"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.3 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>El universo est\u00e1 lleno de agujeros negros \u201cimposibles\u201d. 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