{"id":51047,"date":"2014-06-05T10:13:18","date_gmt":"2014-06-05T09:13:18","guid":{"rendered":"http:\/\/www.astb.se\/cassiopeiabloggen\/?p=51047"},"modified":"2014-06-06T21:01:42","modified_gmt":"2014-06-06T20:01:42","slug":"nr-58-2014","status":"publish","type":"post","link":"https:\/\/www.astb.se\/cassiopeiabloggen\/2014\/06\/05\/nr-58-2014\/","title":{"rendered":"Nr 58 2014"},"content":{"rendered":"<h2>R&ouml;d j&auml;tte + neutronstj&auml;rna = TZO<\/h2>\n<p>Om vi g&auml;ngar en r&ouml;d superj&auml;tte med en kompakt neutronstj&auml;rna f&aring;r vi en synnerligen m&auml;rklig hybrid i v&auml;rldsalltet :<\/p>\n<p>Ett bin&auml;rt&nbsp; <span style=\"font-weight: bold;\">&quot;<\/span>Thorne-\u017bytkow Object&quot;, uppkallat efter <strong>Kip Thorne <\/strong>och<strong> Anna \u017bytkow<\/strong>.<\/p>\n<p>Teoretiskt har dessa stj&auml;rnor diskuterats snart i fyrtio &aring;r, men nu har &#8211; sannolikt &#8211;&nbsp;<a href=\"http:\/\/arxiv-web3.library.cornell.edu\/pdf\/1406.0001 \u200e\"> ett &auml;kta TZO hittats i Lilla Magellanska molnet<\/a>, tipsar <strong>Christian Vestergaard<\/strong>.<\/p>\n<p>Dynamiken i dessa bin&auml;ra system utg&aring;r fr&aring;n att den r&ouml;da&nbsp; j&auml;tten sv&auml;ljer neutronstj&auml;rnan efter dennas supernovaexplosion, den tungtunga neutrontj&auml;rnan som sen spiralar in mot r&ouml;dj&auml;ttens k&auml;rnparti. Detta tycks bevisas av HV2112-stj&auml;rnan i Lilla Magellanska molnet.<\/p>\n<p><a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/largest-star-Betelgeuse.jpg\"><img decoding=\"async\" alt=\"\" class=\"aligncenter size-medium wp-image-51066\" height=\"235\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/largest-star-Betelgeuse-300x235.jpg\" title=\"Typisk r\u00f6d j\u00e4tte - Betelgeuse! Foto: ESA\/NASA\/HST\" width=\"300\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/largest-star-Betelgeuse-300x235.jpg 300w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/largest-star-Betelgeuse.jpg 484w\" sizes=\"(max-width: 300px) 100vw, 300px\" \/><\/a><\/p>\n<p>En av uppt&auml;ckarna, <strong>Nidia Morrell<\/strong>, har kommenterat uppt&auml;ckten med n&aring;gra ord som borde bli klassiska:<\/p>\n<p>&#8211; Jag vet inte vad det &auml;r, men jag vet att jag gillar det.<\/p>\n<p>En stj&auml;rna med en annan stj&auml;rna i sin k&auml;rna &auml;r s&aring; annorlunda i ens &quot;t&auml;nk&quot; att det ska mycket till f&ouml;r att bevisa saken. Men astronomerna har nu i stj&auml;rnans atmosf&auml;r hittat &quot;tunga&quot; grund&auml;mnen som molybden, litium och rubidium, vilket teorin f&ouml;ruts&auml;ger, och dessutom hittat dem i m&auml;ngder och proportioner som passar in i modellen.<\/p>\n<p>HV2112 har tidigare klassats som en variabel M3\/M7-j&auml;tte och varit k&auml;nd som ett av Lilla Magellanska molnets allra intressantaste objekt och legendariska astronomer som <strong>Cecilia Payne-Gaposchkin<\/strong> och <strong>Sergei Gaposchkin<\/strong> m fl har sysslat med stj&auml;rnan.<\/p>\n<p><a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/SiriusB.jpg\"><img decoding=\"async\" alt=\"\" class=\"aligncenter size-medium wp-image-51067\" height=\"296\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/SiriusB-300x296.jpg\" title=\"Typisk vit dv\u00e4rg - SiriusB. Foto: ESA\/NASA\/HST\" width=\"300\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/SiriusB-300x296.jpg 300w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/SiriusB.jpg 600w\" sizes=\"(max-width: 300px) 100vw, 300px\" \/><\/a><\/p>\n<p>Fr&aring;getecken kvarst&aring;r, erk&auml;nner forskarna, men vi har kommit g&aring;tans l&ouml;sning betydligt n&auml;rmare sen teleskopbj&auml;ssar som Magellan-reflektorn (6,5 m) tagits i bruk i Chile. Kanske hittar vi snart ett otvetydigt TZO-exempel bland massiva j&auml;ttestj&auml;rnor i Vintergatan?<\/p>\n<h2>Flyg och far<\/h2>\n<p>N&auml;r vi inom ASTB p&aring; s&ouml;ndag 8 juni &aring;ker norrut, mot v&auml;nnerna i Halland, mellanlandar vi p&aring; flygmuseet i &Auml;ngelholm. Det ger mig m&ouml;jlighet att lite grand prata om flygets roll inom astronomin. S&aring; vi &#8211; h&ouml;rs! I bussen.<\/p>\n<h2>Fj&auml;rilskrater p&aring; Mars<\/h2>\n<p>Mars Odyssey har snurrat runt Mars i flera &aring;r och ger oss fortfarande m&auml;rkliga bilder fr&aring;n v&aring;r grannplanet. Som <a href=\"http:\/\/photojournal.jpl.nasa.gov\/tiff\/PIA18267\">denna dagsf&auml;rska bild &#8211; tagen av instrumentet THEMIS <\/a>&#8211;&nbsp; p&aring; den s&aring; kallade Fj&auml;rilskratern (en av flera &quot;fj&auml;rilar&quot; p&aring; planeten):<\/p>\n<p><a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/PIA18267_modest.jpg\"><img decoding=\"async\" alt=\"\" class=\"aligncenter size-medium wp-image-51077\" height=\"300\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/PIA18267_modest-117x300.jpg\" title=\"\" width=\"117\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/PIA18267_modest-117x300.jpg 117w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/PIA18267_modest-399x1024.jpg 399w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/PIA18267_modest.jpg 624w\" sizes=\"(max-width: 117px) 100vw, 117px\" \/><\/a><\/p>\n<p>Bilden t&aring;l att BL&Aring;SAS UPP rej&auml;lt p&aring; din sk&auml;rm!<\/p>\n<p>Kratern tro ha skapats av en asteroid eller splittret fr&aring;n en Marsm&aring;ne som kommit in i en ovanligt l&aring;g vinkel.<\/p>\n<p>Fenomenet k&auml;nns igen fr&aring;n andra himlakroppar i planetsystemet. En av Apollo-bes&auml;ttningarna dokumenterade denna fj&auml;ril p&aring; m&aring;nen:<\/p>\n<p><a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/hrp119b.jpg\"><img decoding=\"async\" alt=\"\" class=\"aligncenter size-medium wp-image-51090\" height=\"300\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/hrp119b-272x300.jpg\" title=\"Bildk\u00e4lla: NASA\" width=\"272\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/hrp119b-272x300.jpg 272w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/hrp119b.jpg 660w\" sizes=\"(max-width: 272px) 100vw, 272px\" \/><\/a><\/p>\n<p>Merkurius visar motsvarande exempel:<\/p>\n<p><a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/butterfly-elliptical-crater-on-mercury-hovnatanian-craters-bright-rays-indicate-that-they-are-relat-24359.jpg\"><img decoding=\"async\" alt=\"\" class=\"aligncenter size-medium wp-image-51093\" height=\"271\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/butterfly-elliptical-crater-on-mercury-hovnatanian-craters-bright-rays-indicate-that-they-are-relat-24359-300x271.jpg\" title=\"Bildk\u00e4lla: NASA\" width=\"300\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/butterfly-elliptical-crater-on-mercury-hovnatanian-craters-bright-rays-indicate-that-they-are-relat-24359-300x271.jpg 300w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/butterfly-elliptical-crater-on-mercury-hovnatanian-craters-bright-rays-indicate-that-they-are-relat-24359.jpg 610w\" sizes=\"(max-width: 300px) 100vw, 300px\" \/><\/a><\/p>\n<p>&Auml;ven p&aring; Venus kunde genom Magellan-sondens radarsystem denna fj&auml;rilskrater observeras p&aring; 1990-talet:<\/p>\n<p><a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/PIA00474_ip.jpg\"><img decoding=\"async\" alt=\"\" class=\"aligncenter size-medium wp-image-51110\" height=\"300\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/PIA00474_ip-278x300.jpg\" title=\"Bildk\u00e4lla: NASA\/JPL\" width=\"278\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/PIA00474_ip-278x300.jpg 278w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/PIA00474_ip.jpg 600w\" sizes=\"(max-width: 278px) 100vw, 278px\" \/><\/a><\/p>\n<p>En v&auml;gledande diskussion om hur dessa kratrar kan uppst&aring; diskuteras lite varstans, <a href=\"http:\/\/www.planetary.org\/blogs\/emily-lakdawalla\/2011\/2894.html\">bland annat h&auml;r.<\/a><\/p>\n<h2>Vem var Hans Henie?<\/h2>\n<p>1914, f&ouml;r hundra &aring;r sen,&nbsp; satt norske astronomen <strong>Hans Henie<\/strong> i Lund och kollade upp den skenbara stj&auml;rnt&auml;theten p&aring; himlavalvet ner till 11:e magnituden.<\/p>\n<p><a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/554px-Hans_henie.jpg\"><img decoding=\"async\" width=\"150\" height=\"150\" alt=\"\" class=\"alignleft size-thumbnail wp-image-51075\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/554px-Hans_henie-150x150.jpg\" style=\"width: 81px; height: 81px;\" title=\"\" \/><\/a>S&auml;mst var t&auml;theten i Ursa Major\/Stora Bj&ouml;rnen.<\/p>\n<p>Henie blev fil dr p&aring; &auml;mnet.<\/p>\n<p>Denne lundafostrade astronom &auml;r v&auml;rd att syna n&auml;rmare i s&ouml;mmarna. Han var uppenbarligen en<strong> Quisling<\/strong>-anh&auml;ngare under andra v&auml;rldskriget, f&ouml;r det var nazisterna som uts&aring;g honom till rektor f&ouml;r Trondheims katedralskola och senare f&ouml;r den av Quislingarna styrda l&auml;rarh&ouml;gskolan i Hamar.<\/p>\n<p>Brev finns fr&aring;n honom till obsisprofessorn <strong>C V L Charlier<\/strong> i Charlier-samlingen, Lunds UB.<\/p>\n<p>Jag vet inget om honom i &ouml;vrigt &#8211; n&aring;gon?<\/p>\n<h2>Veckans budskap<\/h2>\n<p><a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/pleiades-with-quote-astronomical-wallpapers-galaxies-stars-and-shit-may-1900x1200-wallpaper_wallpaperswa.com_89.jpg\"><img decoding=\"async\" width=\"600\" height=\"378\" alt=\"\" class=\"aligncenter size-full wp-image-51072\" src=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/pleiades-with-quote-astronomical-wallpapers-galaxies-stars-and-shit-may-1900x1200-wallpaper_wallpaperswa.com_89.jpg\" style=\"width: 490px; height: 309px;\" title=\"\" srcset=\"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/pleiades-with-quote-astronomical-wallpapers-galaxies-stars-and-shit-may-1900x1200-wallpaper_wallpaperswa.com_89.jpg 600w, https:\/\/www.astb.se\/cassiopeiabloggen\/wp-content\/uploads\/2014\/06\/pleiades-with-quote-astronomical-wallpapers-galaxies-stars-and-shit-may-1900x1200-wallpaper_wallpaperswa.com_89-300x189.jpg 300w\" sizes=\"(max-width: 600px) 100vw, 600px\" \/><\/a><\/p>\n<p><span _fck_bookmark=\"1\" style=\"display: none;\">&nbsp;<\/span><span _fck_bookmark=\"1\" style=\"display: none;\">&nbsp;<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>R&ouml;d j&auml;tte + neutronstj&auml;rna = TZO Om vi g&auml;ngar en r&ouml;d superj&auml;tte med en kompakt neutronstj&auml;rna f&aring;r vi en synnerligen m&auml;rklig hybrid i v&auml;rldsalltet : Ett bin&auml;rt&nbsp; &quot;Thorne-\u017bytkow Object&quot;, uppkallat efter Kip Thorne och Anna \u017bytkow. Teoretiskt har dessa stj&auml;rnor diskuterats snart i fyrtio &aring;r, men nu har &#8211; sannolikt &#8211;&nbsp; ett &auml;kta TZO hittats&hellip;&nbsp;<a href=\"https:\/\/www.astb.se\/cassiopeiabloggen\/2014\/06\/05\/nr-58-2014\/\" rel=\"bookmark\">L\u00e4s mer &raquo;<span class=\"screen-reader-text\">Nr 58 2014<\/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":[],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/posts\/51047"}],"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=51047"}],"version-history":[{"count":47,"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/posts\/51047\/revisions"}],"predecessor-version":[{"id":51112,"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/posts\/51047\/revisions\/51112"}],"wp:attachment":[{"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/media?parent=51047"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/categories?post=51047"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.astb.se\/cassiopeiabloggen\/wp-json\/wp\/v2\/tags?post=51047"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}