{"id":19148,"date":"2011-07-31T12:06:43","date_gmt":"2011-07-31T09:06:43","guid":{"rendered":"http:\/\/www.fyysika.ee\/uudised\/?p=19148"},"modified":"2011-08-08T15:03:43","modified_gmt":"2011-08-08T12:03:43","slug":"gaas-voolamas-musta-augu-suunas","status":"publish","type":"post","link":"https:\/\/www.fyysika.ee\/?p=19148","title":{"rendered":"Gaas voolamas musta augu suunas"},"content":{"rendered":"<div id=\"attachment_19149\" style=\"width: 542px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.fyysika.ee\/uudised\/wp-content\/uploads\/2011\/07\/575047main_n3115_665.jpg\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-19149\" class=\"size-full wp-image-19149 \" src=\"http:\/\/www.fyysika.ee\/uudised\/wp-content\/uploads\/2011\/07\/575047main_n3115_665.jpg\" alt=\"\" width=\"532\" height=\"472\" srcset=\"https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/07\/575047main_n3115_665.jpg 665w, https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/07\/575047main_n3115_665-300x266.jpg 300w, https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/07\/575047main_n3115_665-250x221.jpg 250w\" sizes=\"auto, (max-width: 532px) 100vw, 532px\" \/><\/a><p id=\"caption-attachment-19149\" class=\"wp-caption-text\">Komposiitkuvand galaktikast NGC 3115. Pilt: R\u00f6ntgen: NASA\/CXC\/Alabama \u00dclikool\/K. Wong jt; Optiline: ESO\/VLT.<\/p><\/div>\n<p>Esmakordselt j\u00e4\u00e4dvustati r\u00f6ntgenkiirte abil pildile kuuma gaasi vool musta augu suunas. NASA Chandra X-ray Observatooriumi vaatlused aitavad \u00fcletada kaht p\u00f5hilisemat probleemi t\u00e4nap\u00e4eva astrof\u00fc\u00fcsikas: kujundada arusaama mustade aukude kasvamisest ja aine k\u00e4itumisest nende intensiivse gravitatsiooni m\u00f5jul.<\/p>\n<p>K\u00f5nealune must auk asub\u00a0 Maast umbes 32 miljoni valgusaasta kaugusel asuva NGC 3115-na tuntud suure galaktika keskel. Suurel hulgal eelnevaid andmeid on n\u00e4idanud aine liikumist musta augu suunas, kuid\u00a0 seni pole suudetud saada nii selget m\u00e4rki kuuma gaasi k\u00e4itumisest samas olukorras.<\/p>\n<p>Luues kujutisi kuumast gaasist erinevatel kaugustel sellest \u00fclimassiivsest mustast august, on astronoomid vaadelnud olulist k\u00fcnnist, kus gaasi liikumist hakkab esmakordselt domineerima musta augu gravitatsioon ning gaas suundub sellesse. See distants mustast august on tuntud \u00a0\u201cBondi raadiusena\u201d.<\/p>\n<p><a href=\"http:\/\/www.nasa.gov\/mission_pages\/chandra\/news\/H-11-248.html\">Allikas<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Esmakordselt j\u00e4\u00e4dvustati r\u00f6ntgenkiirte abil pildile kuuma gaasi vool musta augu suunas. NASA Chandra X-ray Observatooriumi vaatlused aitavad \u00fcletada kaht p\u00f5hilisemat probleemi t\u00e4nap\u00e4eva astrof\u00fc\u00fcsikas: kujundada arusaama mustade aukude kasvamisest ja aine k\u00e4itumisest nende intensiivse gravitatsiooni m\u00f5jul. K\u00f5nealune must auk asub\u00a0 Maast umbes 32 miljoni valgusaasta kaugusel asuva NGC 3115-na tuntud suure galaktika keskel. Suurel hulgal eelnevaid [&hellip;]<\/p>\n","protected":false},"author":448,"featured_media":19149,"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-19148","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\/19148","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=19148"}],"version-history":[{"count":0,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts\/19148\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/media\/19149"}],"wp:attachment":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=19148"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=19148"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=19148"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}