{"id":19151,"date":"2019-05-03T10:34:25","date_gmt":"2019-05-03T14:34:25","guid":{"rendered":"http:\/\/www.astrofisicamas.cl\/?p=19151"},"modified":"2023-10-06T18:46:05","modified_gmt":"2023-10-06T18:46:05","slug":"urano","status":"publish","type":"post","link":"https:\/\/astrofisicamas.cl\/en\/urano\/","title":{"rendered":"Urano"},"content":{"rendered":"<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-9d6595d7 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:66.66%\">\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"813\" src=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/URANO-1024x813.png\" alt=\"\" class=\"wp-image-30250\" srcset=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/URANO-1024x813.png 1024w, https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/URANO-300x238.png 300w, https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/URANO-768x609.png 768w, https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/URANO-15x12.png 15w, https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/URANO.png 1027w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><\/figure>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:33.33%\">\n<p>Urano se encuentra al doble de la distancia que separa Saturno del Sol. Este planeta est\u00e1 compuesto principalmente por hidr\u00f3geno y helio, pero tambi\u00e9n posee trazas de metano, al que se debe su caracter\u00edstico color azul-verdoso. Al igual que los otros planetas gaseosos del Sistema Solar (J\u00fapiter, Saturno y Neptuno) Urano muestra huracanes y tormentas en su atm\u00f3sfera, visibles como manchas claras u oscuras. \u00c9stas duran unos meses, a veces a\u00f1os y luego desaparecen. Urano fue descubierto por Herschel, accidentalmente, en 1781, mirando a trav\u00e9s de un telescopio.<\/p>\n\n\n\n<figure class=\"wp-block-audio\"><audio controls src=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/Urano-final.mp3\"><\/audio><\/figure>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns has-white-color has-text-color has-background is-layout-flex wp-container-core-columns-is-layout-9d6595d7 wp-block-columns-is-layout-flex\" style=\"background-color:#187295\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\"><div class=\"wp-block-image\">\n<figure class=\"aligncenter size-full\"><img loading=\"lazy\" decoding=\"async\" width=\"300\" height=\"213\" src=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/FOTO-1-3-300x213-1.png\" alt=\"\" class=\"wp-image-30252\" srcset=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/FOTO-1-3-300x213-1.png 300w, https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/FOTO-1-3-300x213-1-18x12.png 18w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><figcaption class=\"wp-element-caption\">Urano tambi\u00e9n tiene anillos, pero a diferencia de los de Saturno, estos est\u00e1n compuestos de peque\u00f1os granos de roca que no reflejan eficientemente la luz del Sol y por eso son dif\u00edciles de observar [cr\u00e9dito Keck Observatory]<\/figcaption><\/figure>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\"><div class=\"wp-block-image\">\n<figure class=\"aligncenter size-full\"><img loading=\"lazy\" decoding=\"async\" width=\"300\" height=\"212\" src=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/FOTO-2-3-300x212-1.png\" alt=\"\" class=\"wp-image-30253\" srcset=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/FOTO-2-3-300x212-1.png 300w, https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/FOTO-2-3-300x212-1-18x12.png 18w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><figcaption class=\"wp-element-caption\">Imagen de despedida de Urano en fase creciente al alejarse de \u00e9l la sonda Voyager 2 en 1986 [cr\u00e9dito NASA]<\/figcaption><\/figure>\n<\/div><\/div>\n<\/div>\n\n\n\n<h2 class=\"wp-block-heading\">CURIOSIDADES<\/h2>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-9d6595d7 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\"><div class=\"wp-block-image\">\n<figure class=\"aligncenter size-full\"><img loading=\"lazy\" decoding=\"async\" width=\"188\" height=\"141\" src=\"http:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/CURIOSIDAD-1-4.png\" alt=\"\" class=\"wp-image-30251\" srcset=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/CURIOSIDAD-1-4.png 188w, https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/CURIOSIDAD-1-4-16x12.png 16w\" sizes=\"auto, (max-width: 188px) 100vw, 188px\" \/><figcaption class=\"wp-element-caption\">Urano tiene 27 sat\u00e9lites naturales, cuyos nombres proceden de los personajes de las obras de Shakespeare y Pope. El m\u00e1s grande, Titania, tiene 1580 km de di\u00e1metro y el m\u00e1s peque\u00f1o, Tr\u00ednculo, s\u00f3lo 10 km.<\/figcaption><\/figure>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\"><div class=\"wp-block-image\">\n<figure class=\"aligncenter size-full\"><img loading=\"lazy\" decoding=\"async\" width=\"300\" height=\"141\" src=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/CURIOSIDAD-2-5-300x141-1.png\" alt=\"\" class=\"wp-image-30256\" srcset=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/CURIOSIDAD-2-5-300x141-1.png 300w, https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/CURIOSIDAD-2-5-300x141-1-18x8.png 18w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><figcaption class=\"wp-element-caption\">Urano da una vuelta al Sol en 84 a\u00f1os. Al ser el planeta acostado, cada hemisferio experimenta un verano de Sol cont\u00ednuo durante 21 a\u00f1os y un invierno oscuro igualmente largo.<\/figcaption><\/figure>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-column is-vertically-aligned-top is-layout-flow wp-block-column-is-layout-flow\"><div class=\"wp-block-image\">\n<figure class=\"aligncenter size-full is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/CURIOSIDAD-3-4.png\" alt=\"\" class=\"wp-image-30257\" width=\"181\" height=\"123\" srcset=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/CURIOSIDAD-3-4.png 169w, https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/10\/CURIOSIDAD-3-4-18x12.png 18w\" sizes=\"auto, (max-width: 181px) 100vw, 181px\" \/><figcaption class=\"wp-element-caption\">Urano tiene olor a huevo podrido, debido a la presencia de sulfuro de hidr\u00f3geno en su atm\u00f3sfera.<\/figcaption><\/figure>\n<\/div><\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-9d6595d7 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<div class=\"wp-block-buttons has-custom-font-size has-small-font-size is-layout-flex wp-block-buttons-is-layout-flex\">\n<div class=\"wp-block-button\"><a class=\"wp-block-button__link wp-element-button\" href=\"https:\/\/astrofisicamas.cl\/saturno\/\">Volver a Saturno<\/a><\/div>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\"><\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<div class=\"wp-block-buttons has-custom-font-size has-small-font-size is-content-justification-right is-layout-flex wp-container-core-buttons-is-layout-765c4724 wp-block-buttons-is-layout-flex\">\n<div class=\"wp-block-button\"><a class=\"wp-block-button__link wp-element-button\" href=\"https:\/\/astrofisicamas.cl\/neptuno\/\">Hacia Neptuno<\/a><\/div>\n<\/div>\n<\/div>\n<\/div>","protected":false},"excerpt":{"rendered":"<p>Urano se encuentra al doble de la distancia que separa Saturno del Sol. Este planeta est\u00e1 compuesto principalmente por hidr\u00f3geno y helio, pero tambi\u00e9n posee trazas de metano, al que se debe su caracter\u00edstico color azul-verdoso. Al igual que los otros planetas gaseosos del Sistema Solar (J\u00fapiter, Saturno y Neptuno)&#8230;<\/p>","protected":false},"author":3,"featured_media":26811,"comment_status":"open","ping_status":"open","sticky":false,"template":"templates\/single3.php","format":"standard","meta":{"_coblocks_attr":"","_coblocks_dimensions":"","_coblocks_responsive_height":"","_coblocks_accordion_ie_support":"","_eb_attr":"","footnotes":""},"categories":[64],"tags":[],"class_list":["post-19151","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-sistema-solar"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.2 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Urano - Instituto Milenio de Astrof\u00edsica MAS<\/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:\/\/astrofisicamas.cl\/en\/urano\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Urano - Instituto Milenio de Astrof\u00edsica MAS\" \/>\n<meta property=\"og:description\" content=\"Urano se encuentra al doble de la distancia que separa Saturno del Sol. Este planeta est\u00e1 compuesto principalmente por hidr\u00f3geno y helio, pero tambi\u00e9n posee trazas de metano, al que se debe su caracter\u00edstico color azul-verdoso. Al igual que los otros planetas gaseosos del Sistema Solar (J\u00fapiter, Saturno y Neptuno)...\" \/>\n<meta property=\"og:url\" content=\"https:\/\/astrofisicamas.cl\/en\/urano\/\" \/>\n<meta property=\"og:site_name\" content=\"Instituto Milenio de Astrof\u00edsica MAS\" \/>\n<meta property=\"article:published_time\" content=\"2019-05-03T14:34:25+00:00\" \/>\n<meta property=\"article:modified_time\" content=\"2023-10-06T18:46:05+00:00\" \/>\n<meta property=\"og:image\" content=\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/05\/urano_2.png\" \/>\n\t<meta property=\"og:image:width\" content=\"45\" \/>\n\t<meta property=\"og:image:height\" content=\"45\" \/>\n\t<meta property=\"og:image:type\" content=\"image\/png\" \/>\n<meta name=\"author\" content=\"Makarena Estrella Pacheco\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Written by\" \/>\n\t<meta name=\"twitter:data1\" content=\"Makarena Estrella Pacheco\" \/>\n\t<meta name=\"twitter:label2\" content=\"Est. reading time\" \/>\n\t<meta name=\"twitter:data2\" content=\"1 minute\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\"@context\":\"https:\/\/schema.org\",\"@graph\":[{\"@type\":\"Article\",\"@id\":\"https:\/\/astrofisicamas.cl\/urano\/#article\",\"isPartOf\":{\"@id\":\"https:\/\/astrofisicamas.cl\/urano\/\"},\"author\":{\"name\":\"Makarena Estrella Pacheco\",\"@id\":\"https:\/\/astrofisicamas.cl\/#\/schema\/person\/0a23b23af648e746893cb7cd7efae1e4\"},\"headline\":\"Urano\",\"datePublished\":\"2019-05-03T14:34:25+00:00\",\"dateModified\":\"2023-10-06T18:46:05+00:00\",\"mainEntityOfPage\":{\"@id\":\"https:\/\/astrofisicamas.cl\/urano\/\"},\"wordCount\":252,\"commentCount\":0,\"publisher\":{\"@id\":\"https:\/\/astrofisicamas.cl\/#organization\"},\"image\":{\"@id\":\"https:\/\/astrofisicamas.cl\/urano\/#primaryimage\"},\"thumbnailUrl\":\"https:\/\/astrofisicamas.cl\/wp-content\/uploads\/2023\/05\/urano_2.png\",\"articleSection\":[\"Sistema Solar\"],\"inLanguage\":\"en-US\"},{\"@type\":\"WebPage\",\"@id\":\"https:\/\/astrofisicamas.cl\/urano\/\",\"url\":\"https:\/\/astrofisicamas.cl\/urano\/\",\"name\":\"Urano - 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