{"id":18295,"date":"2025-05-19T09:46:25","date_gmt":"2025-05-19T07:46:25","guid":{"rendered":"https:\/\/micromega-dynamics.com\/project\/astronomy\/"},"modified":"2025-05-19T09:46:28","modified_gmt":"2025-05-19T07:46:28","slug":"astronomy","status":"publish","type":"project","link":"https:\/\/micromega-dynamics.com\/it\/project\/astronomy\/","title":{"rendered":"Astronomia"},"content":{"rendered":"<p>[et_pb_section fb_built=&#8221;1&#8243; admin_label=&#8221;Header&#8221; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; background_image=&#8221;https:\/\/micromega-dynamics.com\/files\/uploads\/2024\/11\/Cover-Usecase-1-1.jpg&#8221; parallax=&#8221;on&#8221; custom_padding=&#8221;8vw||0vw||false|false&#8221; border_radii=&#8221;off|||0vw|0vw&#8221; collapsed=&#8221;on&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_row custom_padding_last_edited=&#8221;on|phone&#8221; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; max_width=&#8221;1800px&#8221; custom_padding=&#8221;|237px||||&#8221; custom_padding_tablet=&#8221;|237px||||&#8221; custom_padding_phone=&#8221;|0px|||false|false&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;4.22.0&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;2a1fa9e3-278a-4815-a8b6-86e3861ec73b&#8221; text_text_color=&#8221;#3C9100&#8243; header_text_color=&#8221;#ffffff&#8221; header_font_size=&#8221;56px&#8221; header_4_font=&#8221;|600|||||||&#8221; header_4_text_color=&#8221;#ffffff&#8221; header_4_font_size=&#8221;23px&#8221; background_color=&#8221;rgba(10,10,10,0.5)&#8221; max_width=&#8221;1440px&#8221; custom_margin=&#8221;||||true|true&#8221; custom_padding=&#8221;10px|10px|10px|10px|true|true&#8221; border_radii=&#8221;on|5px|5px|5px|5px&#8221; global_colors_info=&#8221;{}&#8221;]<\/p>\n<h1>Astronomia<\/h1>\n<h4><span class=\"OYPEnA font-feature-liga-off font-feature-clig-off font-feature-calt-off text-decoration-none text-strikethrough-none\">Servizi di ingegneria : Attuatori<\/span><\/h4>\n<p>[\/et_pb_text][et_pb_button button_url=&#8221;@ET-DC@eyJkeW5hbWljIjp0cnVlLCJjb250ZW50IjoicG9zdF9saW5rX3VybF9wYWdlIiwic2V0dGluZ3MiOnsicG9zdF9pZCI6IjEzMjczIn19@&#8221; button_text=&#8221;Contattaci&#8221; _builder_version=&#8221;4.27.4&#8243; _dynamic_attributes=&#8221;button_url&#8221; _module_preset=&#8221;8904402d-84ed-403f-be1c-6de59b1d4dcb&#8221; button_bg_color=&#8221;#0071BB&#8221; button_border_radius=&#8221;5px&#8221; button_on_hover=&#8221;off&#8221; custom_padding=&#8221;11px|32px|11px|32px|true|true&#8221; hover_enabled=&#8221;0&#8243; global_colors_info=&#8221;{}&#8221; sticky_enabled=&#8221;0&#8243;][\/et_pb_button][\/et_pb_column][\/et_pb_row][\/et_pb_section][et_pb_section fb_built=&#8221;1&#8243; admin_label=&#8221;About&#8221; _builder_version=&#8221;4.24.0&#8243; _module_preset=&#8221;default&#8221; custom_padding=&#8221;||3px|||&#8221; collapsed=&#8221;on&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_row column_structure=&#8221;2_3,1_3&#8243; _builder_version=&#8221;4.24.0&#8243; _module_preset=&#8221;default&#8221; max_width=&#8221;1800px&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;2_3&#8243; _builder_version=&#8221;4.22.0&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;d4beb851-2ed0-4803-97e0-f2d50020575e&#8221; global_colors_info=&#8221;{}&#8221;]<\/p>\n<h2><span class=\"OYPEnA font-feature-liga-off font-feature-clig-off font-feature-calt-off text-decoration-none text-strikethrough-none\">Astronomia<\/span><\/h2>\n<p>[\/et_pb_text][et_pb_text _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;52afce6b-0212-4de0-94d1-88b79e261070&#8243; global_colors_info=&#8221;{}&#8221;]Per raggiungere l&#8217;altissima risoluzione necessaria per osservare oggetti astronomici lontani, gli specchi dei grandi telescopi astronomici devono mantenere la loro forma in ogni circostanza, nonostante i continui cambiamenti di orientamento e di temperatura. Per raggiungere questo obiettivo, gli specchi sono solitamente molto spessi, il che li rende costosi, pesanti e richiede strutture meccaniche molto robuste e rigide per sostenerli. Al giorno d&#8217;oggi, i produttori di telescopi preferiscono specchi pi\u00f9 sottili e leggeri che sono dotati di una rete di attuatori per la modellazione dello specchio per compensare la loro insufficiente rigidit\u00e0 e mantenere costantemente la superficie riflettente dello specchio nelle condizioni pi\u00f9 perfette possibili.[\/et_pb_text][\/et_pb_column][et_pb_column type=&#8221;1_3&#8243; _builder_version=&#8221;4.22.0&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_image src=&#8221;https:\/\/micromega-dynamics.com\/files\/uploads\/2024\/11\/ry-10.jpg&#8221; alt=&#8221;Astronomia Controllo delle vibrazioni&#8221; title_text=&#8221;Astronomia Controllo delle vibrazioni&#8221; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; custom_margin=&#8221;34px|||||&#8221; border_radii=&#8221;on|8px|8px|8px|8px&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_image][\/et_pb_column][\/et_pb_row][\/et_pb_section][et_pb_section fb_built=&#8221;1&#8243; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; background_color=&#8221;#f9f9f9&#8243; custom_padding=&#8221;14px||20px|||&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_row column_structure=&#8221;1_2,1_2&#8243; _builder_version=&#8221;4.24.3&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;1_2&#8243; _builder_version=&#8221;4.24.3&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;d4beb851-2ed0-4803-97e0-f2d50020575e&#8221; global_colors_info=&#8221;{}&#8221;]<\/p>\n<h3><strong><span class=\"OYPEnA font-feature-liga-off font-feature-clig-off font-feature-calt-off text-decoration-none text-strikethrough-none\">Cosa facciamo<\/span><\/strong><\/h3>\n<div class=\"flex max-w-full flex-col flex-grow\">\n<div data-message-author-role=\"assistant\" data-message-id=\"c7f50d3f-bbc0-43e0-9f03-e40e25aa0859\" dir=\"auto\" class=\"min-h-8 text-message flex w-full flex-col items-end gap-2 whitespace-normal break-words [.text-message+&amp;]:mt-5\">\n<div class=\"flex w-full flex-col gap-1 empty:hidden first:pt-[3px]\">\n<div class=\"markdown prose w-full break-words dark:prose-invert light\">\n<ul>\n<li>Progettazione e produzione di<a href=\"https:\/\/micromega-dynamics.com\/engineering-services\/actuators\/\" title=\"Progettazione e produzione di attuatori per la sagomatura degli specchi in base a specifiche molto severe dei clienti (range di forza e precisione, dissipazione di potenza, rigidit\u00e0 parassita...). \">attuatori<\/a> per la sagomatura degli specchi<span> <\/span><span> <\/span> in base a specifiche molto severe del cliente (range di forza e precisione, dissipazione di potenza, rigidit\u00e0 parassita, ecc.)<\/li>\n<li><a href=\"https:\/\/micromega-dynamics.com\/it\/engineering-services\/calibration\/\" title=\"Calibrazione degli attuatori per la sagomatura degli specchi\">Calibrazione<\/a><span> <\/span>degli attuatori per la sagomatura degli specchi<\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<p>[\/et_pb_text][\/et_pb_column][et_pb_column type=&#8221;1_2&#8243; _builder_version=&#8221;4.24.3&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;d4beb851-2ed0-4803-97e0-f2d50020575e&#8221; global_colors_info=&#8221;{}&#8221;]<\/p>\n<h3><strong><span class=\"OYPEnA font-feature-liga-off font-feature-clig-off font-feature-calt-off text-decoration-none text-strikethrough-none\">Vantaggi<\/span><\/strong><\/h3>\n<div class=\"flex max-w-full flex-col flex-grow\">\n<div data-message-author-role=\"assistant\" data-message-id=\"c7f50d3f-bbc0-43e0-9f03-e40e25aa0859\" dir=\"auto\" class=\"min-h-8 text-message flex w-full flex-col items-end gap-2 whitespace-normal break-words [.text-message+&amp;]:mt-5\">\n<div class=\"flex w-full flex-col gap-1 empty:hidden first:pt-[3px]\">\n<div class=\"markdown prose w-full break-words dark:prose-invert light\">\n<ul>\n<li>Know-how integrato (meccanica, elettronica integrata, software in tempo reale)<\/li>\n<li>Sviluppo di sensori e attuatori dedicati con elettronica di condizionamento e guida<\/li>\n<li>Qualificazione del meccanismo (ad es. test di prestazione, temperatura e vibrazione)<\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section][et_pb_section fb_built=&#8221;1&#8243; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_row _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; header_2_font_size=&#8221;54px&#8221; global_colors_info=&#8221;{}&#8221;]<\/p>\n<h2 style=\"text-align: center;\">Casi d&#8217;uso<\/h2>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][et_pb_row column_structure=&#8221;1_2,1_2&#8243; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;1_2&#8243; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;52afce6b-0212-4de0-94d1-88b79e261070&#8243; global_colors_info=&#8221;{}&#8221;]<\/p>\n<h2>Telescopio solare DKIST<\/h2>\n<p>Il Daniel K. Inouye Solar Telescope (DKIST) \u00e8 il<a href=\"https:\/\/www.nso.edu\/telescopes\/dki-solar-telescope\/\" title=\"il telescopio solare pi\u00f9 grande del mondo\">telescopio solare pi\u00f9 grande del mondo<\/a><span> <\/span>.<\/p>\n<p>La progettazione e la produzione dello specchio primario di 4,2 metri di diametro e della cella che lo circonda sono state affidate all&#8217;azienda<span> <\/span><a href=\"https:\/\/www.amos.be\/project\/mirror-cell-for-dkist\" title=\"AMOS\">AMOS<\/a>.<\/p>\n<p>In qualit\u00e0 di subappaltatore di AMOS, Micromega ha progettato e prodotto i 142 attuatori idraulici e pneumatici che correggono continuamente la forma del sottile specchio primario con una precisione migliore di 45 nm RMS.<\/p>\n<p>La cella \u00e8 stata integrata e testata nel telescopio nel 2017. Nel gennaio 2020, il Daniel K. Inouye Solar Telescope ha svelato le immagini pi\u00f9 dettagliate mai realizzate della superficie del nostro sole. <\/p>\n<p>[\/et_pb_text][\/et_pb_column][et_pb_column type=&#8221;1_2&#8243; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_image src=&#8221;https:\/\/micromega-dynamics.com\/files\/uploads\/2024\/11\/ry-11.jpg&#8221; alt=&#8221;Astronomia Controllo e monitoraggio delle vibrazioni&#8221; title_text=&#8221;Astronomia Controllo e monitoraggio delle vibrazioni&#8221; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_image][\/et_pb_column][\/et_pb_row][\/et_pb_section][et_pb_section fb_built=&#8221;1&#8243; _builder_version=&#8221;4.24.3&#8243; _module_preset=&#8221;default&#8221; custom_padding=&#8221;0px|||||&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_row _builder_version=&#8221;4.24.3&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;4.24.3&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text _builder_version=&#8221;4.24.3&#8243; _module_preset=&#8221;default&#8221; header_3_font=&#8221;|600|||||||&#8221; header_3_font_size=&#8221;31px&#8221; global_colors_info=&#8221;{}&#8221;]<\/p>\n<h3>Scopri altri progetti<\/h3>\n<p>[\/et_pb_text][et_pb_portfolio fullwidth=&#8221;off&#8221; posts_number=&#8221;4&#8243; include_categories=&#8221;current&#8221; show_categories=&#8221;off&#8221; show_pagination=&#8221;off&#8221; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; title_font=&#8221;|700|||||||&#8221; title_line_height=&#8221;1.8em&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_portfolio][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Astronomia Servizi di ingegneria : AttuatoriAstronomiaPer raggiungere l&#8217;altissima risoluzione necessaria per osservare oggetti astronomici lontani, gli specchi dei grandi telescopi astronomici devono mantenere la loro forma in ogni circostanza, nonostante i continui cambiamenti di orientamento e di temperatura. Per raggiungere questo obiettivo, gli specchi sono solitamente molto spessi, il che li rende costosi, pesanti e [&hellip;]<\/p>\n","protected":false},"author":13,"featured_media":18299,"comment_status":"open","ping_status":"closed","template":"","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"","_et_gb_content_width":"","footnotes":""},"project_category":[210],"project_tag":[],"class_list":["post-18295","project","type-project","status-publish","has-post-thumbnail","hentry","project_category-monitoraggio-delle-vibrazioni"],"yoast_head":"<!-- This site is optimized with the Yoast SEO Premium plugin v27.5 (Yoast SEO v27.5) - https:\/\/yoast.com\/product\/yoast-seo-premium-wordpress\/ -->\n<title>Astronomia: Attuatori di ottica adattativa - Micromega Dynamics<\/title>\n<meta name=\"description\" content=\"Gli specchi leggeri dei telescopi utilizzano attuatori per mantenere una riflessione perfetta, adattandosi ai cambiamenti di orientamento e di temperatura.\" \/>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/micromega-dynamics.com\/it\/project\/astronomy\/\" \/>\n<meta property=\"og:locale\" content=\"it_IT\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Astronomia\" \/>\n<meta property=\"og:description\" content=\"Gli specchi leggeri dei telescopi utilizzano attuatori per mantenere una riflessione perfetta, adattandosi ai cambiamenti di orientamento e di temperatura.\" \/>\n<meta property=\"og:url\" content=\"https:\/\/micromega-dynamics.com\/it\/project\/astronomy\/\" \/>\n<meta property=\"og:site_name\" content=\"Micromega Dynamics\" \/>\n<meta property=\"article:modified_time\" content=\"2025-05-19T07:46:28+00:00\" \/>\n<meta property=\"og:image\" content=\"https:\/\/micromega-dynamics.com\/files\/uploads\/2024\/11\/ry-1-2.jpg\" \/>\n\t<meta property=\"og:image:width\" content=\"900\" \/>\n\t<meta property=\"og:image:height\" content=\"900\" \/>\n\t<meta property=\"og:image:type\" content=\"image\/jpeg\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Tempo di lettura stimato\" \/>\n\t<meta name=\"twitter:data1\" content=\"5 minuti\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\"@context\":\"https:\\\/\\\/schema.org\",\"@graph\":[{\"@type\":\"WebPage\",\"@id\":\"https:\\\/\\\/micromega-dynamics.com\\\/it\\\/project\\\/astronomy\\\/\",\"url\":\"https:\\\/\\\/micromega-dynamics.com\\\/it\\\/project\\\/astronomy\\\/\",\"name\":\"Astronomia: Attuatori di ottica adattativa - 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