{"id":38,"date":"2015-11-23T13:02:31","date_gmt":"2015-11-23T12:02:31","guid":{"rendered":"http:\/\/wwwmaory.bo.astro.it\/?page_id=38"},"modified":"2025-12-16T17:53:07","modified_gmt":"2025-12-16T16:53:07","slug":"home","status":"publish","type":"page","link":"http:\/\/wwwmorfeo.oabo.inaf.it\/index.php\/home\/","title":{"rendered":"HOME"},"content":{"rendered":"<p>MORFEO\u00a0 (Multi-conjugate adaptive Optics Relay For ELT Observation ) formerly know as MAORY, is one of the first light instruments for the\u00a0<a href=\"https:\/\/elt.eso.org\/\"> Extremely Large Telescope (ELT)<\/a>, the 39 m diameter optical-infrared telescope that the <a href=\"http:\/\/www.eso.org\/\">European Southern Observatory<\/a>\u00a0(ESO) \u00a0will build in the next decade in collaboration with its community of member States.<\/p>\n<p>MORFEO is a post-focal adaptive optics module. It supports the <a href=\"http:\/\/www.mpe.mpg.de\/ir\/micado\">MICADO<\/a>\u00a0 near-infrared camera by offering two adaptive optics modes: Multi-Conjugate Adaptive Optics (MCAO) and Single-Conjugate Adaptive Optics (SCAO).<\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_833\" aria-describedby=\"caption-attachment-833\" style=\"width: 702px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" class=\"wp-image-833\" src=\"http:\/\/wwwmaory.oabo.inaf.it\/wp-content\/uploads\/2021\/03\/MAORY-Overview.png\" alt=\"\" width=\"702\" height=\"448\" srcset=\"http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2021\/03\/MAORY-Overview.png 1177w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2021\/03\/MAORY-Overview-300x191.png 300w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2021\/03\/MAORY-Overview-1024x653.png 1024w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2021\/03\/MAORY-Overview-768x490.png 768w\" sizes=\"(max-width: 702px) 100vw, 702px\" \/><figcaption id=\"caption-attachment-833\" class=\"wp-caption-text\">General overview of the MORFEO instrument (thermal cover in transparency) installed on the Nasmyth platform with MICADO<\/figcaption><\/figure>\n<p>In the MC<span style=\"font-size: 1rem;\">AO m<\/span><span style=\"font-size: 1rem;\">ode, wavefront sensing is performed by a system based on up to six Laser Guide Stars for high-order wavefront sensing and three Natural Guide Stars for low-<\/span><span style=\"font-size: 1rem;\">order wavefront sensing; wavefront compensation is achieved by up to two deformable mirrors in MORFEO, which work together with the telescope adaptive and tip-tilt mirrors M4 and M5 respectively. In the SCAO mode, wavefront distortions are measured by a single Natural Guide Star wavefront sensor and compensated by the telescope M4 and M5 mirrors, while the deformable mirrors inside MORFEO are kept flat.<\/span><\/p>\n<p>MORFEO also offers provision for a second port for a future instrument, as yet undefined.<\/p>\n<p>The international consortium that will develop MORFEO from phase B (preliminary design) to phase E (commissioning) includes <a href=\"http:\/\/www.inaf.it\/\">INAF<\/a> (lead institute responsible for the design and construction of the instrument at system level) ,\u00a0\u00a0IPAG (France), NUIG (Ireland), NRC (Canada), NAOJ (Japan), Kyoto University (Japan) and Osaka University (Japan).<\/p>\n<p>ESO is the project customer and is also a supplier of components for the instrument construction.<\/p>\n<p><img loading=\"lazy\" class=\"wp-image-239 alignleft\" src=\"http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/12\/logo_inaf_2015.png\" alt=\"\" width=\"59\" height=\"59\" \/><\/p>\n<p><img loading=\"lazy\" class=\"wp-image-125 alignleft\" src=\"http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/IPAG_logo.png\" alt=\"\" width=\"74\" height=\"52\" srcset=\"http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/IPAG_logo.png 1181w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/IPAG_logo-300x212.png 300w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/IPAG_logo-1024x724.png 1024w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/IPAG_logo-150x106.png 150w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/IPAG_logo-400x283.png 400w\" sizes=\"(max-width: 74px) 100vw, 74px\" \/><img loading=\"lazy\" class=\"wp-image-1365 alignleft\" src=\"http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2025\/12\/logo-JPIs.png\" alt=\"\" width=\"194\" height=\"66\" srcset=\"http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2025\/12\/logo-JPIs.png 1983w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2025\/12\/logo-JPIs-300x102.png 300w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2025\/12\/logo-JPIs-1024x347.png 1024w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2025\/12\/logo-JPIs-768x260.png 768w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2025\/12\/logo-JPIs-1536x521.png 1536w\" sizes=\"(max-width: 194px) 100vw, 194px\" \/><\/p>\n<p><img loading=\"lazy\" class=\"wp-image-817 alignleft\" style=\"font-size: 1rem;\" src=\"http:\/\/wwwmaory.oabo.inaf.it\/wp-content\/uploads\/2021\/03\/nuig.png\" alt=\"\" width=\"160\" height=\"49\" \/><a href=\"https:\/\/www.eso.org\/public\/\"><img loading=\"lazy\" class=\"wp-image-128 alignright\" src=\"http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/eso-logo.jpg\" alt=\"\" width=\"37\" height=\"48\" srcset=\"http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/eso-logo.jpg 981w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/eso-logo-230x300.jpg 230w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/eso-logo-785x1024.jpg 785w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/eso-logo-115x150.jpg 115w, http:\/\/wwwmorfeo.oabo.inaf.it\/wp-content\/uploads\/2015\/11\/eso-logo-400x522.jpg 400w\" sizes=\"(max-width: 37px) 100vw, 37px\" \/><\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>MORFEO\u00a0 (Multi-conjugate adaptive Optics Relay For ELT Observation ) formerly know as MAORY, is one of the first light instruments for the\u00a0 Extremely Large Telescope (ELT), the 39 m diameter optical-infrared telescope that the European Southern Observatory\u00a0(ESO) \u00a0will build in the next decade in collaboration with its community of member States. MORFEO is a post-focal &hellip; <\/p>\n<p class=\"link-more\"><a href=\"http:\/\/wwwmorfeo.oabo.inaf.it\/index.php\/home\/\" class=\"more-link\">Continue reading<span class=\"screen-reader-text\"> &#8220;HOME&#8221;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"guten_post_layout_featured_media_urls":{"full":false,"thumbnail":false,"medium":false,"medium_large":false,"large":false,"1536x1536":false,"2048x2048":false,"guten_post_layout_landscape_large":false,"guten_post_layout_portrait_large":false,"guten_post_layout_square_large":false,"guten_post_layout_landscape":false,"guten_post_layout_portrait":false,"guten_post_layout_square":false,"twentyseventeen-featured-image":false,"twentyseventeen-thumbnail-avatar":false},"_links":{"self":[{"href":"http:\/\/wwwmorfeo.oabo.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/38"}],"collection":[{"href":"http:\/\/wwwmorfeo.oabo.inaf.it\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"http:\/\/wwwmorfeo.oabo.inaf.it\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"http:\/\/wwwmorfeo.oabo.inaf.it\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"http:\/\/wwwmorfeo.oabo.inaf.it\/index.php\/wp-json\/wp\/v2\/comments?post=38"}],"version-history":[{"count":37,"href":"http:\/\/wwwmorfeo.oabo.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/38\/revisions"}],"predecessor-version":[{"id":1382,"href":"http:\/\/wwwmorfeo.oabo.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/38\/revisions\/1382"}],"wp:attachment":[{"href":"http:\/\/wwwmorfeo.oabo.inaf.it\/index.php\/wp-json\/wp\/v2\/media?parent=38"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}