{"id":12801,"date":"2022-07-20T11:09:01","date_gmt":"2022-07-20T09:09:01","guid":{"rendered":"https:\/\/www.mdscc.nasa.gov\/?p=12801"},"modified":"2022-07-20T11:09:03","modified_gmt":"2022-07-20T09:09:03","slug":"las-ondas-de-choque-de-una-supernova","status":"publish","type":"post","link":"https:\/\/www.mdscc.nasa.gov\/index.php\/2022\/07\/20\/las-ondas-de-choque-de-una-supernova\/","title":{"rendered":"Las ondas de choque de una supernova"},"content":{"rendered":"\n<p class=\"wp-block-paragraph\">Las supernovas son las muertes explosivas de las estrellas m\u00e1s masivas del universo. Al morir, estos objetos lanzan poderosas ondas hacia el cosmos, destruyendo gran parte del polvo que las rodea.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Esta composici\u00f3n de 2007 del Telescopio Espacial Spitzer de la NASA y el Observatorio de rayos X Chandra, muestra el remanente de tal explosi\u00f3n, conocida como N132D, y el entorno en el que se est\u00e1 expandiendo. En esta imagen, la luz infrarroja de 4,5 micras se asigna al azul, 8,0 micras al verde y 24 micras al rojo. Mientras tanto, la luz de rayos X de banda ancha se mapea de color p\u00farpura. El remanente en s\u00ed se ve como una tenue capa de gas rosa en el centro de esta imagen. El color rosado revela una interacci\u00f3n entre las ondas de choque de alta energ\u00eda de la explosi\u00f3n (originalmente p\u00farpura) y los granos de polvo circundantes.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Fuera del remanente central, las peque\u00f1as mol\u00e9culas org\u00e1nicas llamadas hidrocarburos arom\u00e1ticos polic\u00edclicos o PAH, se muestran como tintes de verde. Los puntos azules representan estrellas dentro que se encuentran a lo largo de la l\u00ednea de visi\u00f3n entre los observatorios y N132D.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><strong><a href=\"https:\/\/www.nasa.gov\/image-feature\/a-supernovas-shockwaves\">Noticia original (en ingl\u00e9s)<\/a><\/strong><\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><em>Edici\u00f3n: R. Castro.<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Cr\u00e9ditos: rayos X: NASA\/SAO\/CXC; Infrarrojo: NASA\/JPL-Caltech\/A. Tappe y J. Rho.<\/p>\n","protected":false},"author":2,"featured_media":12802,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[79,252],"tags":[],"class_list":["post-12801","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-noticias","category-ultimas-noticias"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/posts\/12801","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/comments?post=12801"}],"version-history":[{"count":1,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/posts\/12801\/revisions"}],"predecessor-version":[{"id":12803,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/posts\/12801\/revisions\/12803"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/media\/12802"}],"wp:attachment":[{"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/media?parent=12801"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/categories?post=12801"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/tags?post=12801"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}