{"id":22609,"date":"2025-02-18T09:21:05","date_gmt":"2025-02-18T09:21:05","guid":{"rendered":"https:\/\/www.starhuntereos.com\/heliophysics\/?page_id=22609"},"modified":"2025-02-22T00:57:05","modified_gmt":"2025-02-22T00:57:05","slug":"spektroskopi","status":"publish","type":"page","link":"https:\/\/www.starhuntereos.com\/heliophysics\/spektroskopi\/","title":{"rendered":"Spektroskopi"},"content":{"rendered":"<section class=\"wpb-content-wrapper\"><p>[vc_row row_type=&#8221;row&#8221; use_row_as_full_screen_section=&#8221;no&#8221; type=&#8221;full_width&#8221; text_align=&#8221;left&#8221; background_animation=&#8221;none&#8221; padding_bottom=&#8221;45&#8243; css_animation=&#8221;&#8221;][vc_column][vc_column_text]Spektroskopi adalah teknik saintifik menganalisis cahaya yang digunakan bagi mengkaji objek jauh di angkasa.<\/p>\n<p>Tujuan: Membantu saintis memahami saiz, jarak, kelajuan pergerakan, dan komposisi kimia bagi objek seperti lubang hitam, bintang neutron dan galaksi aktif.[\/vc_column_text][vc_separator type=&#8221;transparent&#8221; border_style=&#8221;&#8221; up=&#8221;20&#8243; down=&#8221;0&#8243; icon_pack=&#8221;font_awesome&#8221;][\/vc_column][\/vc_row][vc_row row_type=&#8221;row&#8221; use_row_as_full_screen_section=&#8221;no&#8221; type=&#8221;full_width&#8221; text_align=&#8221;left&#8221; background_animation=&#8221;none&#8221; padding_bottom=&#8221;45&#8243; css_animation=&#8221;&#8221;][vc_column width=&#8221;1\/2&#8243;][vc_column_text]Spektra: Graf atau carta yang menunjukkan intensiti cahaya yang dipancarkan pada pelbagai tenaga.<\/p>\n<p>Penganalisisan Cahaya: Spektra boleh dihasilkan untuk semua jenis cahaya, dari gelombang radio berenergi rendah hingga sinar gamma yang sangat berenergi tinggi.<\/p>\n<p>Manfaat: Membantu saintis mengetahui bagaimana objek menghasilkan cahaya, kelajuan pergerakan, dan unsur yang terkandung di dalamnya.<\/p>\n<p>Spektroskop adalah alat penting untuk meneroka alam semesta dan memahami objek angkasa yang jauh.<br \/>\n[\/vc_column_text][vc_separator type=&#8221;transparent&#8221; border_style=&#8221;&#8221; up=&#8221;20&#8243; down=&#8221;0&#8243; icon_pack=&#8221;font_awesome&#8221;][\/vc_column][vc_column width=&#8221;1\/2&#8243;][vc_single_image image=&#8221;22876&#8243; img_size=&#8221;full&#8221; qode_css_animation=&#8221;&#8221;][\/vc_column][\/vc_row]<\/p>\n<\/section>","protected":false},"excerpt":{"rendered":"<p>[vc_row row_type=&#8221;row&#8221; use_row_as_full_screen_section=&#8221;no&#8221; type=&#8221;full_width&#8221; text_align=&#8221;left&#8221; background_animation=&#8221;none&#8221; padding_bottom=&#8221;45&#8243; css_animation=&#8221;&#8221;][vc_column][vc_column_text]Spektroskopi adalah teknik saintifik menganalisis cahaya yang digunakan bagi mengkaji objek jauh di angkasa. Tujuan: Membantu saintis memahami saiz, jarak, kelajuan pergerakan, dan komposisi kimia bagi objek seperti lubang hitam, bintang neutron dan galaksi aktif.[\/vc_column_text][vc_separator type=&#8221;transparent&#8221; border_style=&#8221;&#8221; up=&#8221;20&#8243; down=&#8221;0&#8243; icon_pack=&#8221;font_awesome&#8221;][\/vc_column][\/vc_row][vc_row row_type=&#8221;row&#8221; use_row_as_full_screen_section=&#8221;no&#8221; type=&#8221;full_width&#8221; text_align=&#8221;left&#8221; background_animation=&#8221;none&#8221; padding_bottom=&#8221;45&#8243; css_animation=&#8221;&#8221;][vc_column width=&#8221;1\/2&#8243;][vc_column_text]Spektra: Graf atau carta&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-22609","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/pages\/22609","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/comments?post=22609"}],"version-history":[{"count":5,"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/pages\/22609\/revisions"}],"predecessor-version":[{"id":22877,"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/pages\/22609\/revisions\/22877"}],"wp:attachment":[{"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/media?parent=22609"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}