{"id":115298,"date":"2019-11-23T20:40:31","date_gmt":"2019-11-23T19:40:31","guid":{"rendered":"https:\/\/zjarr.tv\/?p=115298"},"modified":"2019-11-23T14:59:14","modified_gmt":"2019-11-23T13:59:14","slug":"zbulohet-galaktika-e-pare-me-jo-nje-por-tre-vrima-te-zeza-ne-qender-te-saj","status":"publish","type":"post","link":"https:\/\/zjarr.tv\/sq\/zbulohet-galaktika-e-pare-me-jo-nje-por-tre-vrima-te-zeza-ne-qender-te-saj\/","title":{"rendered":"Zbulohet galaktika e par\u00eb me jo nj\u00eb, por tre vrima t\u00eb zeza n\u00eb qend\u00ebr t\u00eb saj"},"content":{"rendered":"

Zakonisht, galaktikat e m\u00ebdha, si tonat, kan\u00eb nj\u00eb vrim\u00eb t\u00eb madhe t\u00eb zez\u00eb n\u00eb qend\u00ebr t\u00eb tyre, por nj\u00eb ekip nd\u00ebrkomb\u00ebtar i astronom\u00ebve ka zbuluar galaktik\u00ebn e par\u00eb n\u00eb rajonin qendror t\u00eb s\u00eb cil\u00ebs ka tre vrima t\u00eb zeza t\u00eb m\u00ebdha, relativisht af\u00ebr nj\u00ebra-tjetr\u00ebs.Kjo \u00ebsht\u00eb galaktika NGC 6240 rreth 300 milion vite drit\u00eb nga Toka. Deri m\u00eb tani, shkenc\u00ebtar\u00ebt mendonin se ai kishte dy vrima t\u00eb zeza qendrore, por p\u00ebrfundimisht gjet\u00ebn nj\u00eb t\u00eb tret\u00eb.<\/em><\/p>\n

\u00a0<\/em>Vrimat e zeza supermasive veprojn\u00eb si motor\u00ebt q\u00eb fuqizojn\u00eb qendrat e galaktikave, p\u00ebrfshir\u00eb galaktik\u00ebn ton\u00eb t\u00eb Rrug\u00ebs s\u00eb Qum\u00ebshtit. Por, n\u00eb fillim, shkenc\u00ebtar\u00ebt kan\u00eb v\u00ebrejtur se nj\u00eb galaktik\u00eb p\u00ebrmban tre vrima t\u00eb zeza supermasive n\u00eb thelbin e saj dhe ato \u00e7udit\u00ebrisht jan\u00eb af\u00ebr.<\/p>\n

Galaktika, NGC 6240, ka nj\u00eb form\u00eb t\u00eb pazakont\u00eb, e cila m\u00eb par\u00eb i b\u00ebri shkenc\u00ebtar\u00ebt t\u00eb besojn\u00eb se ajo u krijua kur dy galaktika m\u00eb t\u00eb vogla u p\u00ebrplas\u00ebn dhe filluan t\u00eb bashkohen.<\/p>\n

NGC 6240 \u00ebsht\u00eb relativisht af\u00ebr nesh me standarde universale n\u00eb 300 milion vite drit\u00eb larg, k\u00ebshtu q\u00eb astronom\u00ebt kan\u00eb qen\u00eb n\u00eb gjendje ta studiojn\u00eb at\u00eb n\u00eb t\u00eb gjitha gjat\u00ebsit\u00eb e val\u00ebve t\u00eb drit\u00ebs.<\/p>\n

Ajo u pa si nj\u00eb standard p\u00ebr nd\u00ebrveprimin galaktik dhe shkenc\u00ebtar\u00ebt menduan se p\u00ebr shkak t\u00eb bashkimit, ka t\u00eb ngjar\u00eb t\u00eb ket\u00eb dy vrima t\u00eb zeza n\u00eb thelbin e saj.<\/p>\n

Por v\u00ebzhgimet e reja zbuluan nj\u00eb vrim\u00eb t\u00eb tret\u00eb t\u00eb zez\u00eb supermasive n\u00eb qend\u00ebr t\u00eb galaktik\u00ebs. \u00c7do vrim\u00eb e zez\u00eb ka mas\u00ebn e m\u00eb shum\u00eb se 90 milion diell secila.<\/p>\n

Gjetjet u botuan t\u00eb enjten n\u00eb revist\u00ebn\u00a0Astronomy & Astrophysics<\/a>\u00a0. V\u00ebzhgimet e reja t\u00eb galaktik\u00ebs u mor\u00ebn nga Teleskopi Shum\u00eb i Madh i Observatorit Jugor Evropian n\u00eb Kili.<\/p>\n

“P\u00ebrmes v\u00ebzhgimeve tona me rezolucion hap\u00ebsinor jasht\u00ebzakonisht t\u00eb lart\u00eb ne ishim n\u00eb gjendje t\u00eb tregonim se sistemi nd\u00ebrveprues i galaktik\u00ebs NGC 6240 pret jo dy – si\u00e7 supozohej m\u00eb par\u00eb – por tre vrima t\u00eb zeza supermasive n\u00eb qend\u00ebr t\u00eb tij,” tha \u00cbolfram Kollatschny, autor kryesor i studimit dhe profesor n\u00eb Universitetin e G\u00f6ttingen.<\/p>\n

T\u00eb tre vrimat e zeza mund t\u00eb gjenden n\u00eb t\u00eb nj\u00ebjtin rajon q\u00eb ka m\u00eb pak se 3000 vjet drit\u00eb n\u00eb t\u00eb gjith\u00eb. P\u00ebr referenc\u00eb, astronom\u00ebt than\u00eb se kjo hap\u00ebsir\u00eb \u00ebsht\u00eb m\u00eb e vog\u00ebl se nj\u00eb e pesta e madh\u00ebsis\u00eb s\u00eb t\u00eb gjith\u00eb galaktik\u00ebs.<\/p>\n

“Nj\u00eb p\u00ebrqendrim i till\u00eb i tre vrimave t\u00eb zeza supermasive nuk ishte zbuluar kurr\u00eb n\u00eb univers”, tha Peter \u00cbeilbacher, autor studimi n\u00eb Institutin Leibniz p\u00ebr Astrofizik\u00ebn Potsdam.<\/p>\n

“Rasti aktual jep prova t\u00eb nj\u00eb procesi t\u00eb bashkimit t\u00eb nj\u00ebkohsh\u00ebm t\u00eb tre galaktikave s\u00eb bashku me vrimat e tyre qendrore t\u00eb zeza”.<\/p>\n

Ky zbulim do t\u00eb lejoj\u00eb q\u00eb astronom\u00ebt t\u00eb kuptojn\u00eb m\u00eb shum\u00eb se si evoluojn\u00eb galaktikat me kalimin e koh\u00ebs, ve\u00e7an\u00ebrisht galaktikat m\u00eb t\u00eb m\u00ebdha n\u00eb univers.<\/p>\n

“N\u00ebse ndodhin proceset e shkrirjes s\u00eb nj\u00ebkohshme t\u00eb disa galaktikave, at\u00ebher\u00eb galaktikat m\u00eb t\u00eb m\u00ebdha me vrimat e tyre t\u00eb zeza supermasive qendrore jan\u00eb n\u00eb gjendje t\u00eb evoluojn\u00eb shum\u00eb m\u00eb shpejt,” tha \u00cbeilbacher.<\/p>\n

“V\u00ebzhgimet tona japin indikacionin e par\u00eb t\u00eb k\u00ebtij skenari.”<\/p>\n

Me kalimin e koh\u00ebs, me gjas\u00eb disa milion vjet, t\u00eb tre vrimat e zeza supermasive do t\u00eb bashkohen, than\u00eb studiuesit.<\/p>\n

Ky bashkim i fundit pritet t\u00eb krijoj\u00eb val\u00eb tep\u00ebr t\u00eb forta gravitacionale, ose t\u00eb zgjas\u00eb n\u00eb hap\u00ebsir\u00ebn e koh\u00ebs.<\/p>\n

<\/p>\n","protected":false},"excerpt":{"rendered":"

Zakonisht, galaktikat e m\u00ebdha, si tonat, kan\u00eb nj\u00eb vrim\u00eb t\u00eb madhe t\u00eb zez\u00eb n\u00eb qend\u00ebr t\u00eb tyre, por nj\u00eb ekip nd\u00ebrkomb\u00ebtar i astronom\u00ebve ka zbuluar galaktik\u00ebn e par\u00eb n\u00eb rajonin qendror t\u00eb s\u00eb cil\u00ebs ka tre vrima t\u00eb zeza t\u00eb m\u00ebdha, relativisht af\u00ebr nj\u00ebra-tjetr\u00ebs.Kjo \u00ebsht\u00eb galaktika NGC 6240 rreth 300 milion vite drit\u00eb nga Toka. […]<\/p>\n","protected":false},"author":2013,"featured_media":115299,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[241,206],"tags":[],"class_list":{"0":"post-115298","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-aktualitet","8":"category-shkence"},"_links":{"self":[{"href":"https:\/\/zjarr.tv\/sq\/wp-json\/wp\/v2\/posts\/115298","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/zjarr.tv\/sq\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/zjarr.tv\/sq\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/zjarr.tv\/sq\/wp-json\/wp\/v2\/users\/2013"}],"replies":[{"embeddable":true,"href":"https:\/\/zjarr.tv\/sq\/wp-json\/wp\/v2\/comments?post=115298"}],"version-history":[{"count":0,"href":"https:\/\/zjarr.tv\/sq\/wp-json\/wp\/v2\/posts\/115298\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/zjarr.tv\/sq\/wp-json\/wp\/v2\/media\/115299"}],"wp:attachment":[{"href":"https:\/\/zjarr.tv\/sq\/wp-json\/wp\/v2\/media?parent=115298"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/zjarr.tv\/sq\/wp-json\/wp\/v2\/categories?post=115298"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/zjarr.tv\/sq\/wp-json\/wp\/v2\/tags?post=115298"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}