{"id":104859,"date":"2008-10-26T07:43:00","date_gmt":"2008-10-26T07:43:00","guid":{"rendered":"http:\/\/weblogs.madrimasd.org\/\/astrofisica\/archive\/2008\/10\/26\/104859.aspx"},"modified":"2008-10-26T07:43:00","modified_gmt":"2008-10-26T07:43:00","slug":"hubble-space-telescope-y-xmm-newton-vuelven-a-la-vida","status":"publish","type":"post","link":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/2008\/10\/26\/104859","title":{"rendered":"Hubble Space Telescope y XMM-Newton vuelven a la vida"},"content":{"rendered":"<div align=\"justify\">David ByN<\/p>\n<p>Despu\u00e9s de d\u00edas (o semanas) de preocupaci\u00f3n, dos de los observatorios m\u00e1s potentes, HST y XMM-Newon, vuelven a la normalidad y resumen sus operaciones cient\u00edficas.<\/div>\n<p><!--more--><\/p>\n<div align=\"justify\">Ambos telescopios han producido una gran cantidad de r<A href=\"http:\/\/weblogs.madrimasd.org\/astrofisica\/archive\/2008\/02\/07\/84036.aspx\">esultados cient\u00edficos de gran importancia<\/a>, y es de esperar que continuen as\u00ed, de no presentarse problemas adicionales, durante bastante tiempo. Ambos cubren rangos de longitudes de onda esenciales (ultravioleta-infrarrojo cercano en el caso del HST, rayos-X en el de XMM-Newton), que o bien no son accesibles desde la superficie de la Tierra, o bien no con esa sensibilidad y resoluci\u00f3n angular.<\/p>\n<p>M\u00e1s informaci\u00f3n en las notas de prensa de NASA y la Agencia Espacial Europea:<\/p>\n<p><a temp_href=\"http:\/\/www.nasa.gov\/mission_pages\/hubble\/servicing\/SM4\/news\/status_rpt_7_20081025.html \" href=\"http:\/\/www.nasa.gov\/mission_pages\/hubble\/servicing\/SM4\/news\/status_rpt_7_20081025.html%20\">NASA sobre HST<\/a><\/p>\n<p><a temp_href=\"http:\/\/www.esa.int\/esaSC\/SEM268RTKMF_index_0.html \" href=\"http:\/\/www.esa.int\/esaSC\/SEM268RTKMF_index_0.html%20\">ESA sobre XMM-Newton<\/a><\/p>\n<p>PD (2008\/X\/30): <br \/><a href=\"http:\/\/hubblesite.org\/newscenter\/archive\/releases\/2008\/37\/fastfacts\/\">Primeras (y espectaculares) im\u00e1genes del HST despu\u00e9s del incidente<\/a><\/div>\n","protected":false},"excerpt":{"rendered":"<p>David ByN Despu\u00e9s de d\u00edas (o semanas) de preocupaci\u00f3n, dos de los observatorios m\u00e1s potentes, HST y XMM-Newon, vuelven a la normalidad y resumen sus operaciones cient\u00edficas.<\/p>\n","protected":false},"author":32,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"ngg_post_thumbnail":0},"categories":[557,553],"tags":[],"blocksy_meta":{"styles_descriptor":{"styles":{"desktop":"","tablet":"","mobile":""},"google_fonts":[],"version":4}},"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/wp-json\/wp\/v2\/posts\/104859"}],"collection":[{"href":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/wp-json\/wp\/v2\/users\/32"}],"replies":[{"embeddable":true,"href":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/wp-json\/wp\/v2\/comments?post=104859"}],"version-history":[{"count":0,"href":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/wp-json\/wp\/v2\/posts\/104859\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/wp-json\/wp\/v2\/media?parent=104859"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/wp-json\/wp\/v2\/categories?post=104859"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/wp-json\/wp\/v2\/tags?post=104859"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}