{"id":17874,"date":"2011-06-20T19:40:29","date_gmt":"2011-06-20T16:40:29","guid":{"rendered":"http:\/\/www.fyysika.ee\/uudised\/?p=17874"},"modified":"2011-07-08T20:13:42","modified_gmt":"2011-07-08T17:13:42","slug":"hubble-hammastav-pilt-kentaur-a-galaktikast","status":"publish","type":"post","link":"https:\/\/www.fyysika.ee\/?p=17874","title":{"rendered":"Hubble: h\u00e4mmastav pilt Kentaur A galaktikast"},"content":{"rendered":"<div id=\"attachment_17879\" style=\"width: 410px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.fyysika.ee\/uudised\/wp-content\/uploads\/2011\/06\/110616092645-large1.jpg\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-17879\" class=\"size-full wp-image-17879\" title=\"110616092645-large\" src=\"http:\/\/www.fyysika.ee\/uudised\/wp-content\/uploads\/2011\/06\/110616092645-large1.jpg\" alt=\"\" width=\"400\" height=\"414\" srcset=\"https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/06\/110616092645-large1.jpg 400w, https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/06\/110616092645-large1-289x300.jpg 289w, https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/06\/110616092645-large1-250x258.jpg 250w\" sizes=\"auto, (max-width: 400px) 100vw, 400px\" \/><\/a><p id=\"caption-attachment-17879\" class=\"wp-caption-text\">NGC 5128. Pilt: NASA, ESA ja Hubble Heritage (STScI\/AURA)-ESA\/Hubble Collaboration<\/p><\/div>\n<p>NASA\/ESA Hubble\u2019i losmoseteleskoop tegi pilti galaktikast Centauri A. Hubble\u2019i suur kaugus uuritavast objektist ning k\u00f5rgtehnoloogilised kuvamisvahendid paljastavad dramaatilise pildi voogavast d\u00fcnaamilisest galaktikast. Galaktika Centauri A, tuntud ka kui NGC 5128, on kuulus oma tugevate tumeainest koosnevate tolmutriipude poolest. Antud foto on seni tehtud piltidest k\u00f5ige detailsem. Siin pildil on kombineeritud mitmelainepikkuselisi kujutisi, kaardistades galaktika tolmuse osa ennen\u00e4gematu detailsusega. Lisaks spektri n\u00e4htavale osale on sellel komposiitpildil asendatud n\u00e4htavate v\u00e4rvidega ka ultravioletset valgust, mis tuleb noortelt t\u00e4htedelt, ning lisaks ka infrapunase kiirguse l\u00e4hedast valgust, mis lubab meil heita pilgu detailidele, mida muidu kataks tolm.<\/p>\n<p>Loe l\u00e4hemalt: &#8220;<a href=\"http:\/\/www.sciencedaily.com\/releases\/2011\/06\/110616092645.htm\">Spectacular Hubble View of Centaurus A<\/a>&#8221;<\/p>\n<p><em><br \/>\n<\/em><\/p>\n<p><em><br \/>\n<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>NASA\/ESA Hubble\u2019i losmoseteleskoop tegi pilti galaktikast Centauri A. Hubble\u2019i suur kaugus uuritavast objektist ning k\u00f5rgtehnoloogilised kuvamisvahendid paljastavad dramaatilise pildi voogavast d\u00fcnaamilisest galaktikast. Galaktika Centauri A, tuntud ka kui NGC 5128, on kuulus oma tugevate tumeainest koosnevate tolmutriipude poolest. Antud foto on seni tehtud piltidest k\u00f5ige detailsem. Siin pildil on kombineeritud mitmelainepikkuselisi kujutisi, kaardistades galaktika tolmuse [&hellip;]<\/p>\n","protected":false},"author":32,"featured_media":17879,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_genesis_hide_title":false,"_genesis_hide_breadcrumbs":false,"_genesis_hide_singular_image":false,"_genesis_hide_footer_widgets":false,"_genesis_custom_body_class":"","_genesis_custom_post_class":"","_genesis_layout":"","footnotes":""},"categories":[40],"tags":[47],"class_list":{"0":"post-17874","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-paev-pildis","8":"tag-ilmaruum","9":"entry"},"_links":{"self":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts\/17874","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/users\/32"}],"replies":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=17874"}],"version-history":[{"count":0,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts\/17874\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/media\/17879"}],"wp:attachment":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=17874"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=17874"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=17874"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}