{"id":200485,"date":"2026-03-16T15:28:17","date_gmt":"2026-03-16T14:28:17","guid":{"rendered":"https:\/\/helloproject.es\/vigilancia\/detectan-un-planeta-con-caracteristicas-quimicas-y-geologicas-ineditas-en-la-via-lactea\/"},"modified":"2026-03-16T15:28:17","modified_gmt":"2026-03-16T14:28:17","slug":"detectan-un-planeta-con-caracteristicas-quimicas-y-geologicas-ineditas-en-la-via-lactea","status":"publish","type":"post","link":"https:\/\/helloproject.es\/vigilancia\/detectan-un-planeta-con-caracteristicas-quimicas-y-geologicas-ineditas-en-la-via-lactea\/","title":{"rendered":"Detectan un planeta con caracter\u00edsticas qu\u00edmicas y geol\u00f3gicas in\u00e9ditas en la V\u00eda L\u00e1ctea"},"content":{"rendered":"

Un equipo internacional de cient\u00edficos, liderado por la Universidad de Oxford (Reino Unido), ha identificado una nueva clase de planeta fuera del Sistema Solar que no encaja en ninguna de las categor\u00edas conocidas hasta ahora, caracterizado por albergar enormes cantidades de azufre en las profundidades de un oc\u00e9ano permanente de magma.<\/p>\n

El planeta, denominado L 98-59 d, orbita una estrella situada a unos 35 a\u00f1os luz de la Tierra; presenta una densidad sorprendentemente baja y una atm\u00f3sfera rica en gases de azufre, lo que desconcert\u00f3 inicialmente a los astr\u00f3nomos, que hoy han publicado los resultados de su investigaci\u00f3n en la revista Nature Astronomy<\/a>.<\/p>\n

El planeta, denominado L 98-59 d, orbita una estrella situada a unos 35 a\u00f1os luz de la Tierra; presenta una densidad sorprendentemente baja y una atm\u00f3sfera rica en gases de azufre<\/p>\n

El descubrimiento del nuevo planeta, que tiene 1,6 veces el tama\u00f1o de la Tierra, podr\u00eda ampliar significativamente lo que se conoce hasta ahora sobre la diversidad de mundos en la galaxia, han subrayado los investigadores, que han utilizado las observaciones realizadas con el\u00a0telescopio espacial James Webb, junto con observatorios terrestres, para revelar la presencia de sulfuro de hidr\u00f3geno y otros compuestos de azufre en la atm\u00f3sfera del planeta.<\/p>\n

<\/a><\/p>\n

Una nueva categor\u00eda de mundos<\/h2>\n

Estas caracter\u00edsticas no encajan con las categor\u00edas habituales en las que se clasifican los planetas peque\u00f1os, como las enanas gaseosas rocosas con atm\u00f3sferas de hidr\u00f3geno o los mundos ricos en agua formados por oc\u00e9anos profundos e hielo, y para entender este extra\u00f1o mundo, los investigadores utilizaron avanzadas simulaciones inform\u00e1ticas que recrean la evoluci\u00f3n del planeta durante casi cinco mil millones de a\u00f1os.<\/p>\n

Los modelos sugieren que el manto del planeta est\u00e1 formado principalmente por silicatos fundidos, similares a la lava, creando un oc\u00e9ano global de magma que podr\u00eda extenderse miles de kil\u00f3metros bajo su superficie<\/p>\n

Los modelos sugieren que el manto del planeta est\u00e1 formado principalmente por silicatos fundidos, similares a la lava terrestre, creando un oc\u00e9ano global de magma que podr\u00eda extenderse miles de kil\u00f3metros bajo su superficie, y ese gigantesco reservorio fundido act\u00faa como un almac\u00e9n de azufre, capaz de retenerlo durante escalas de tiempo geol\u00f3gicas.<\/p>\n


\n \"Vacaciones
\n <\/a><\/p>\n

<\/a><\/p>\n

Vacaciones en un exoplaneta: c\u00f3mo la NASA invent\u00f3 el turismo interestelar<\/h3>\n

<\/p>\n


\n Javier Yanes
\n <\/a> <\/p>\n

<\/a><\/p>\n

Atm\u00f3sfera densa rica en hidr\u00f3geno<\/h2>\n

Adem\u00e1s, ese oc\u00e9ano de magma contribuye a mantener una atm\u00f3sfera densa rica en hidr\u00f3geno, donde se encuentran gases como el sulfuro de hidr\u00f3geno, y aunque normalmente ese gas se perder\u00eda en el espacio debido a la radiaci\u00f3n procedente de la estrella anfitriona, el intercambio qu\u00edmico entre el interior fundido y la atm\u00f3sfera ha permitido conservarlo durante miles de millones de a\u00f1os.<\/p>\n

El primer firmante del estudio, Harrison Nicholls, ha explicado que el descubrimiento podr\u00eda obligar a replantear las categor\u00edas actuales con las que los astr\u00f3nomos han descrito los planetas peque\u00f1os, y ha explicado que aunque es poco probable que un planeta fundido como este pueda albergar vida, su estudio revela la enorme diversidad de mundos que existen fuera del Sistema Solar y plantea la posibilidad de que haya muchos m\u00e1s planetas similares a\u00fan por descubrir.<\/p>\n

Aunque un mundo fundido como este no ser\u00eda habitable, su estudio sugiere que podr\u00edan existir muchos m\u00e1s planetas similares por descubrir<\/p>\n

Las observaciones realizadas en 2024 con el telescopio espacial James Webb detectaron di\u00f3xido de azufre en las capas altas de la atm\u00f3sfera del planeta, y los modelos indican que estos gases se generan cuando la radiaci\u00f3n ultravioleta de su estrella desencadena reacciones qu\u00edmicas en la atm\u00f3sfera.<\/p>\n

Al mismo tiempo, el oc\u00e9ano de magma bajo la superficie act\u00faa como un gigantesco dep\u00f3sito que absorbe y libera estos compuestos a lo largo del tiempo, y esa interacci\u00f3n entre el interior del planeta y su atm\u00f3sfera es la que explicar\u00eda las propiedades inusuales detectadas por los telescopios.<\/p>\n

El telescopio espacial sigue as\u00ed proporcionando informaci\u00f3n clave sobre exoplanetas, y las futuras misiones espaciales, como Ariel y PLATO, ambas de la ESA, para estudiar cientos de exoplanetas. Su estudio podr\u00eda ampliar a\u00fan m\u00e1s este conocimiento y comprender mejor c\u00f3mo se forman y evolucionan y predecir cu\u00e1les podr\u00edan ser habitables.<\/p>\n

Referencia:<\/p>\n

Harrison Nicholls el al. \u00abVolatile-rich evolution of molten super-Earth L 98-59 d\u00bb. Nature Astronomy<\/a>, 2026.<\/p>","protected":false},"excerpt":{"rendered":"

Un equipo internacional de cient\u00edficos, liderado por la Universidad de Oxford (Reino Unido), ha identificado una nueva clase de planeta fuera del Sistema Solar que no encaja en ninguna de las categor\u00edas conocidas hasta ahora, caracterizado por albergar enormes cantidades de azufre en las profundidades de un oc\u00e9ano permanente de magma. El planeta, denominado L […]<\/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-200485","post","type-post","status-publish","format-standard","hentry","category-noticias"],"yoast_head":"\nDetectan un planeta con caracter\u00edsticas qu\u00edmicas y geol\u00f3gicas in\u00e9ditas en la V\u00eda L\u00e1ctea - bip4ex<\/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:\/\/helloproject.es\/vigilancia\/detectan-un-planeta-con-caracteristicas-quimicas-y-geologicas-ineditas-en-la-via-lactea\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Detectan un planeta con caracter\u00edsticas qu\u00edmicas y geol\u00f3gicas in\u00e9ditas en la V\u00eda L\u00e1ctea\" \/>\n<meta property=\"og:description\" content=\"Un equipo internacional de cient\u00edficos, liderado por la Universidad de Oxford (Reino Unido), ha identificado una nueva clase de planeta fuera del Sistema Solar que no encaja en ninguna de las categor\u00edas conocidas hasta ahora, caracterizado por albergar enormes cantidades de azufre en las profundidades de un oc\u00e9ano permanente de magma. 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