{"id":81845,"date":"2019-10-04T15:46:59","date_gmt":"2019-10-04T14:46:59","guid":{"rendered":"http:\/\/www.astb.se\/cassiopeiabloggen\/?p=81845"},"modified":"2019-10-05T14:41:23","modified_gmt":"2019-10-05T13:41:23","slug":"nr-71-2019","status":"publish","type":"post","link":"https:\/\/www.astb.se\/cassiopeiabloggen\/2019\/10\/04\/nr-71-2019\/","title":{"rendered":"Nr 71 2019"},"content":{"rendered":"<h3 class=\"text_intro pr_first\">\n\t<strong><u>ALMA (1):<\/u><\/strong><br \/>\n<\/h3>\n<h2 class=\"text_intro pr_first\">\n\t<strong>H&auml;r bildas dubbelstj&auml;rnor<\/strong><br \/>\n<\/h2>\n<p class=\"text_intro pr_first\">\n\tVi k&auml;nner alla till dem men vi vet inte mycket om hur de bildas: Dubbelstj&auml;rnorna, de fysiskt sammanh&aring;llna &nbsp;paren.\n<\/p>\n<p class=\"text_intro pr_first\">\n\tNu kommer ett mess fr&aring;n ESO som p&aring;talar att astronomer har anv&auml;nt radioteleskopet ALMA f&ouml;r att ta en extremt h&ouml;guppl&ouml;st bild p&aring; tv&aring; gas- och stoftskivor d&auml;r unga stj&auml;rnor v&auml;xer till. Dessa cirkumstell&auml;ra skivor matas med material fr&aring;n en st&ouml;rre skiva via filament i ett komplext kringelliknande m&ouml;nster. Observationerna av detta m&auml;rkliga fenomen kastar nytt ljus &ouml;ver de tidigaste stadierna i stj&auml;rnornas liv och hj&auml;lper astronomerna att f&ouml;rst&aring; hur dubbelstj&auml;rnor bildas.\n<\/p>\n<p class=\"text_intro pr_first\">\n\t<a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/eso1916a1.jpg\"><img decoding=\"async\" alt=\"eso1916a[1]\" class=\"aligncenter size-medium wp-image-81849\" height=\"122\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/eso1916a1-300x122.jpg\" width=\"300\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/eso1916a1-300x122.jpg 300w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/eso1916a1-200x81.jpg 200w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/eso1916a1.jpg 733w\" sizes=\"(max-width: 300px) 100vw, 300px\" \/><\/a>\n<\/p>\n<p style=\"text-align: center;\">\n\t<em>Bildk&auml;lla: ALMA (ESO\/NAOJ\/NRAO), Alves et al.<\/em>\n<\/p>\n<p class=\"text_intro pr_first\">\n\tDe nyf&ouml;dda stj&auml;rnorna p&aring; bilden utg&ouml;r de yngsta medlemmarna i en liten stj&auml;rnhop i den m&ouml;rka nebulosan Barnard 59, som i sin tur utg&ouml;r en del av den stora Pipnebulosan.\n<\/p>\n<p class=\"text_intro pr_first\">\n\tOm vi p&aring;pekar att bakom den&nbsp;enligt v&aring;r mening spektakul&auml;ra bilden ligger det fantastiska ALMA-maskineriet, s&aring; f&ouml;rv&aring;nas v&auml;l ingen.\n<\/p>\n<p class=\"text_intro pr_first\">\n\tHela ESO-messet <a href=\"https:\/\/www.eso.org\/public\/sweden\/news\/eso1916\/?lang\">&aring;terfinns h&auml;r.<\/a>\n<\/p>\n<p class=\"text_intro pr_first\">\n\tForskningsresultaten publicerades 3 oktober i tidskriften <em>Science.<\/em>\n<\/p>\n<h3 dir=\"ltr\" style=\"line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;\">\n\t<strong><u>ALMA (2):<\/u><\/strong><br \/>\n<\/h3>\n<h2 dir=\"ltr\" style=\"line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;\">\n\t&nbsp;<br \/>\n<\/h2>\n<h2 dir=\"ltr\" style=\"line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;\">\n\t<strong>Jupiter in p&aring; bara m&auml;ssingen<\/strong><br \/>\n<\/h2>\n<p dir=\"ltr\">\n\t\u200bALMA, som ju st&aring;r f&ouml;r Atacama Large Millimeter\/submillimeter Array,&nbsp; riktas d&aring; och d&aring; &auml;ven mot planetsystemets medlemmar. Som h&auml;r n&auml;r gasj&auml;tten Jupiter avsl&ouml;jar vad han har under det yttersta atmosf&auml;rlagret:\n<\/p>\n<p dir=\"ltr\">\n\t<img decoding=\"async\" alt=\"jupiter_ALMA_redfig2[1]\" class=\"aligncenter size-medium wp-image-81854\" height=\"200\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiter_ALMA_redfig21-300x200.jpg\" width=\"300\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiter_ALMA_redfig21-300x200.jpg 300w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiter_ALMA_redfig21-1024x682.jpg 1024w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiter_ALMA_redfig21-200x133.jpg 200w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiter_ALMA_redfig21.jpg 1800w\" sizes=\"(max-width: 300px) 100vw, 300px\" \/>\n<\/p>\n<p class=\"wp-caption-text\" style=\"text-align: center;\">\n\t<em>Bildk&auml;lla: &nbsp;ALMA (ESO\/NAOJ\/NRAO), I de Pater et al.; NRAO\/AUI NSF, S. Dagnello<\/em>\n<\/p>\n<p dir=\"ltr\">\n\tVi befinner oss femtio km under planetens synliga frysta, ammoniakdominerade &ouml;versta lager, kanske trettio km ovanf&ouml;r det flytande vattenlager som h&auml;r tros finnas. Omr&aring;det best&auml;mmer vad som h&auml;nder i Jupiters yttre lager, stormar, v&aring;ldsamma &aring;skv&auml;der etc.\n<\/p>\n<p dir=\"ltr\">\n\t<a href=\"https:\/\/alma-telescope.jp\/en\/news\/jupiter-201908\">Notabelt &auml;r att i ALMA-messet <\/a>ber&auml;ttas att det var amat&ouml;rastronomer som s&aring;g en eruption 2017 i Jupiters atmosf&auml;r. Larmet gick, varp&aring; b&aring;de radioteleskopet ALMA&nbsp;och Hubble ST riktades mot gasdominanten. Resultatet h&auml;r&nbsp;p&aring; en utplattad Jupiterbild:\n<\/p>\n<p dir=\"ltr\">\n\t<a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiterFig4_ALMA-HST-1024x9831.jpg\"><img decoding=\"async\" alt=\"jupiterFig4_ALMA-HST-1024x983[1]\" class=\"aligncenter size-medium wp-image-81858\" height=\"287\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiterFig4_ALMA-HST-1024x9831-300x287.jpg\" width=\"300\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiterFig4_ALMA-HST-1024x9831-300x287.jpg 300w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiterFig4_ALMA-HST-1024x9831-200x191.jpg 200w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiterFig4_ALMA-HST-1024x9831.jpg 1024w\" sizes=\"(max-width: 300px) 100vw, 300px\" \/><\/a>\n<\/p>\n<p dir=\"ltr\" style=\"text-align: center;\">\n\t<a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/jupiterFig4_ALMA-HST-1024x9831.jpg\">\u200b<\/a><em>Bildk&auml;lla: ALMA (ESO\/NAOJ\/NRAO), I de Pater et al.; NRAO\/AUI NSF, S. Dagnello; NASA\/Hubble<\/em>\n<\/p>\n<p dir=\"ltr\">\n\tTittips: Gl&ouml;m inte BL&Aring;SA UPP bilderna p&aring; din sk&auml;rm!\n<\/p>\n<h2 dir=\"ltr\">\n\t<strong>&quot;And the winner is&#8230;&quot;<\/strong><br \/>\n<\/h2>\n<p dir=\"ltr\">\n\tP&aring; tisdag f m f&aring;r vi veta vem som tagit hem &aring;rets nobelpris i fysik. Blir det n&aring;gon med astronomisk\/astrofysisk koppling, <strong>Shep Doeleman, <\/strong>initiativtagaren till det otroliga projektet att avbilda det svarta h&aring;let i M87, blir det <strong>Wendy Freedman,<\/strong> som &auml;gnat st&ouml;rre delen av sitt forskarliv &aring;t att best&auml;mma&nbsp; Hubble-konstanten&#8230; eller blir det n&aring;got helt annat, danskan <strong>Lene Hau<\/strong> f&ouml;r hennes och hennes teams prestation att bromsa upp ljushastigheten i diverse l&ouml;sningar och kristaller?\n<\/p>\n<p dir=\"ltr\">\n\tMed start kl 11.45 tisdag 8.10 <a href=\"https:\/\/www.kva.se\/sv\/startsida\">direkts&auml;nder Kungliga Vetenskapsakademien tillk&auml;nnagivandet p&aring; sin&nbsp; hemsida.<\/a>\n<\/p>\n<h2 dir=\"ltr\">\n\t<strong>Mira p&aring; g&aring;ng upp<\/strong><br \/>\n<\/h2>\n<p dir=\"ltr\">\n\tHelt planenligt &auml;r alla variablers variabel, Mira, omikron i Cetus, p&aring; v&auml;g att n&aring; sitt maximum om en tid &#8211; just nu ligger stj&auml;rnan runt 3:e magnituden, f&ouml;r en m&aring;nad sedan gick den knappt att sk&ouml;nja f&ouml;r blotta &ouml;gat.\n<\/p>\n<h2 dir=\"ltr\">\n\t<strong>Fullm&aring;nen st&auml;ller till det<\/strong><br \/>\n<\/h2>\n<p dir=\"ltr\">\n\tN&auml;r fullm&aring;nen f&ouml;r en tid sedan tr&auml;ngde sig emellan k&aring;karna i Pisa, fick tornet sig en t&ouml;rn och b&ouml;rjade vika ner sig.\n<\/p>\n<p dir=\"ltr\">\n\tBildbevis fr&aring;n&nbsp;<strong>Nils Gallil&eacute;:<\/strong>\n<\/p>\n<p dir=\"ltr\">\n\t<a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/762v55hrt9m31-e1570199930394.jpg\"><img decoding=\"async\" alt=\"762v55hrt9m31\" class=\"aligncenter size-medium wp-image-81866\" height=\"300\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/762v55hrt9m31-e1570199930394-223x300.jpg\" width=\"223\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/762v55hrt9m31-e1570199930394-223x300.jpg 223w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/762v55hrt9m31-e1570199930394-148x200.jpg 148w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2019\/10\/762v55hrt9m31-e1570199930394.jpg 542w\" sizes=\"(max-width: 223px) 100vw, 223px\" \/><\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>ALMA (1): H&auml;r bildas dubbelstj&auml;rnor Vi k&auml;nner alla till dem men vi vet inte mycket om hur de bildas: Dubbelstj&auml;rnorna, de fysiskt sammanh&aring;llna &nbsp;paren. Nu kommer ett mess fr&aring;n ESO som p&aring;talar att astronomer har anv&auml;nt radioteleskopet ALMA f&ouml;r att ta en extremt h&ouml;guppl&ouml;st bild p&aring; tv&aring; gas- och stoftskivor d&auml;r unga stj&auml;rnor v&auml;xer till.&hellip;&nbsp;<a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/2019\/10\/04\/nr-71-2019\/\" rel=\"bookmark\">L\u00e4s mer &raquo;<span class=\"screen-reader-text\">Nr 71 2019<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"rop_custom_images_group":[],"rop_custom_messages_group":[],"rop_publish_now":"initial","rop_publish_now_accounts":[],"rop_publish_now_history":[],"rop_publish_now_status":"pending","neve_meta_sidebar":"","neve_meta_container":"","neve_meta_enable_content_width":"","neve_meta_content_width":0,"neve_meta_title_alignment":"","neve_meta_author_avatar":"","neve_post_elements_order":"","neve_meta_disable_header":"","neve_meta_disable_footer":"","neve_meta_disable_title":"","footnotes":""},"categories":[3],"tags":[],"_links":{"self":[{"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/posts\/81845"}],"collection":[{"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/comments?post=81845"}],"version-history":[{"count":23,"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/posts\/81845\/revisions"}],"predecessor-version":[{"id":81873,"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/posts\/81845\/revisions\/81873"}],"wp:attachment":[{"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/media?parent=81845"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/categories?post=81845"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/tags?post=81845"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}