{"id":20683,"date":"2011-09-14T17:40:57","date_gmt":"2011-09-14T14:40:57","guid":{"rendered":"http:\/\/www.fyysika.ee\/uudised\/?p=20683"},"modified":"2011-09-14T17:41:50","modified_gmt":"2011-09-14T14:41:50","slug":"suttis-supernoova-jaanuk","status":"publish","type":"post","link":"https:\/\/www.fyysika.ee\/?p=20683","title":{"rendered":"S\u00fcttis supernoova j\u00e4\u00e4nuk"},"content":{"rendered":"<div id=\"attachment_20682\" style=\"width: 509px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.fyysika.ee\/uudised\/wp-content\/uploads\/2011\/09\/586013main_image_2058_946-710.jpg\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-20682\" class=\"size-full wp-image-20682  \" src=\"http:\/\/www.fyysika.ee\/uudised\/wp-content\/uploads\/2011\/09\/586013main_image_2058_946-710.jpg\" alt=\"\" width=\"499\" height=\"375\" srcset=\"https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/09\/586013main_image_2058_946-710.jpg 946w, https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/09\/586013main_image_2058_946-710-300x225.jpg 300w, https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/09\/586013main_image_2058_946-710-250x187.jpg 250w\" sizes=\"auto, (max-width: 499px) 100vw, 499px\" \/><\/a><p id=\"caption-attachment-20682\" class=\"wp-caption-text\">Pilt: NASA, ESA ja P. Challis (Harvard-Smithsonian&#39;i Astrof\u00fc\u00fcsika Keskus )<\/p><\/div>\n<p>Hubble Kosmoseteleskoobi abil tunnistavad astronoomid ennen\u00e4gematut \u00fcleminekut supernoovast supernoova j\u00e4\u00e4nukiks. Valgus plahvatavalt t\u00e4helt naabergalaktikas the Large Magellanic Cloud (Suur Magalh\u00e3esi Pilv) j\u00f5udis Maani 1987. aasta veebruaris. Supernova 1987A-ks nimetatu oli 400 aasta jooksul l\u00e4him n\u00e4htud supernoova plahvatus. Supernoova l\u00e4hedus Maale v\u00f5imaldab astronoomidel selle arengut vaadelda. N\u00fc\u00fcd on mitme aasta jooksul tuhmunud supernoova rusud taas heledamaks muutunud. See t\u00e4hendab, et rusudes on valgust kiirgama hakanud teine energiaallikas. SN 1987A rusud hakkasid m\u00f5jutama seda \u00fcmbritsevat s\u00f5\u00f5ri, luues v\u00f5imsaid l\u00f6\u00f6klaineid, mis tekitavad NASA Chandra R\u00f6ntgenobservatooriumist vaadeldavaid r\u00f6ntgenkiiri. Need r\u00f6ntgenkiired valgustavad supernoova rususid ning l\u00f6\u00f6klainest tekkiv soojusenergia paneb selle n\u00e4htavas valguses helendama. Alates \u00f5hkut\u00f5usust 1990. aastal on Hubble teleskoop katkematult j\u00e4\u00e4dvustanud muutusi supernoovas 1987A.<\/p>\n<p><a href=\"http:\/\/www.nasa.gov\/multimedia\/imagegallery\/image_feature_2058.html\">Allikas<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Hubble Kosmoseteleskoobi abil tunnistavad astronoomid ennen\u00e4gematut \u00fcleminekut supernoovast supernoova j\u00e4\u00e4nukiks. Valgus plahvatavalt t\u00e4helt naabergalaktikas the Large Magellanic Cloud (Suur Magalh\u00e3esi Pilv) j\u00f5udis Maani 1987. aasta veebruaris. Supernova 1987A-ks nimetatu oli 400 aasta jooksul l\u00e4him n\u00e4htud supernoova plahvatus. Supernoova l\u00e4hedus Maale v\u00f5imaldab astronoomidel selle arengut vaadelda. N\u00fc\u00fcd on mitme aasta jooksul tuhmunud supernoova rusud taas heledamaks [&hellip;]<\/p>\n","protected":false},"author":448,"featured_media":20682,"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-20683","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\/20683","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\/448"}],"replies":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=20683"}],"version-history":[{"count":0,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts\/20683\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/media\/20682"}],"wp:attachment":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=20683"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=20683"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=20683"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}