{"id":47575,"date":"2018-09-15T08:47:50","date_gmt":"2018-09-15T06:47:50","guid":{"rendered":"https:\/\/osr.org\/?p=47575\/"},"modified":"2018-09-15T10:37:48","modified_gmt":"2018-09-15T08:37:48","slug":"kuyruklu-yildizlar-ve-turleri","status":"publish","type":"post","link":"https:\/\/osr.org\/tr\/blog\/astronomi\/kuyruklu-yildizlar-ve-turleri\/","title":{"rendered":"Kuyruklu y\u0131ld\u0131zlar ve t\u00fcrleri"},"content":{"rendered":"

Kuyruklu y\u0131ld\u0131zlar\u0131n b\u00f6l\u00fcmleri:<\/span><\/h2>\n

a.\tN\u00fcve: Nispeten kat\u0131 ve kararl\u0131 olan \u00e7ekirdek, su buzu ve di\u011fer donmu\u015f gazlar ve az miktarda kozmik toz ve di\u011fer kat\u0131 cisimlerden olu\u015fmu\u015ftur.<\/p>\n

b.\tKoma: \u00c7ekirdekten buharla\u015fan su, karbondioksit ve di\u011fer n\u00f6tr gazlar\u0131n yo\u011fun bir bulutudur. N\u00fcveyi \u00e7evreleyen \u0131\u015f\u0131k topu \u015feklinde g\u00f6r\u00fcl\u00fcr.<\/p>\n

c.\tHidrojen bulutu: \u00c7ok b\u00fcy\u00fck (milyonlarca km) ancak son derece seyrek bir n\u00f6tr hidrojen zarf\u0131d\u0131r.<\/p>\n

d.\tToz kuyru\u011fu: 10 milyon km’yi a\u015fan uzunlukta, \u00e7ekirdekten ka\u00e7an gazlarla ta\u015f\u0131nan mikroskobik toz partik\u00fcllerinden olu\u015fmu\u015f duman. Kuyruklu y\u0131ld\u0131z\u0131n \u00e7\u0131plak g\u00f6zle g\u00f6r\u00fclebilen en belirgin \u00f6zelli\u011fini olu\u015fturur.<\/p>\n

e.\t\u0130yon kuyru\u011fu: Kuyruklu y\u0131ld\u0131z\u0131n y\u00fczlerce milyon km’ye varan uzunlukta G\u00fcne\u015f r\u00fczg\u00e2r\u0131yla reaksiyon sonucu iyonize olmu\u015f gazlardan olu\u015fan plazma kuyru\u011fudur.<\/p>\n

Kuyruklu y\u0131ld\u0131zlar, G\u00fcne\u015f yak\u0131n\u0131ndan y\u00fczlerce ge\u00e7i\u015f sonunda (yakla\u015f\u0131k 500 ge\u00e7i\u015f sonunda), buz ve gazlar\u0131n\u0131n tamam\u0131na yak\u0131n\u0131n\u0131 yitirerek asteroidlere benzer bir g\u00f6r\u00fcn\u00fcm kazan\u0131rlar (muhtemelen d\u00fcnyaya yak\u0131n asteroidlerin baz\u0131lar\u0131 \u00f6l\u00fc kuyruklu y\u0131ld\u0131zlard\u0131r.) Y\u00f6r\u00fcngeleri G\u00fcne\u015f’e yakla\u015fan kuyruklu y\u0131ld\u0131zlar\u0131n, G\u00fcne\u015f ya da gezegenlerle \u00e7arp\u0131\u015fma ya da olduk\u00e7a yak\u0131n bir ge\u00e7i\u015fle (\u00f6zellikle J\u00fcpiter’e yak\u0131n ge\u00e7erlerse), G\u00fcne\u015f Sistemi d\u0131\u015f\u0131na at\u0131lmalar\u0131 olas\u0131l\u0131\u011f\u0131 vard\u0131r.<\/p>\n

Kuyruklu y\u0131ld\u0131zlar i\u00e7inde en \u00fcnl\u00fcs\u00fc Halley kuyruklu y\u0131ld\u0131z\u0131d\u0131r. Yak\u0131n ge\u00e7mi\u015fte g\u00f6r\u00fclen kuyruklu y\u0131ld\u0131zlar, 1994 yaz\u0131nda J\u00fcpiter’e \u00e7arpan SL 9 (Shoemaker-Levy) ve 1997 y\u0131l\u0131nda \u00e7\u0131plak g\u00f6zle g\u00f6zlemlenen Hale-Bopp ve 2002 y\u0131l\u0131nda g\u00f6r\u00fclen \u0130keya Seki kuyruklu y\u0131ld\u0131z\u0131d\u0131r.<\/p>\n

Kuyruklu y\u0131ld\u0131zlar G\u00fcne\u015f’e yeterince yak\u0131n olmad\u0131k\u00e7a g\u00f6r\u00fclmezler. Baz\u0131lar\u0131n\u0131n y\u00f6r\u00fcngesi G\u00fcne\u015f Sistemi’nin bir hayli d\u0131\u015f\u0131na ta\u015far, bunlar bir kez g\u00f6r\u00fcld\u00fckten sonra binlerce y\u0131l boyunca geri d\u00f6nmezler. Sadece k\u0131sa ve orta periyotlu kuyruklu y\u0131ld\u0131zlar\u0131n (Halley kuyruklu y\u0131ld\u0131z\u0131 gibi) y\u00f6r\u00fcngelerinin en az\u0131ndan \u00f6nemli bir b\u00f6l\u00fcm\u00fc G\u00fcne\u015f Sistemi i\u00e7inde kal\u0131r.<\/p>\n

Kuyruklu y\u0131ld\u0131zlar ve y\u00f6r\u00fcngeleri<\/span><\/h2>\n

Kuyruklu y\u0131ld\u0131zlar ilke olarak G\u00fcne\u015f’in \u00e7ekim alan\u0131n\u0131n etkisi alt\u0131ndad\u0131r. Y\u00f6r\u00fcngeleri elips, parabol ender olarak da hiperbol \u00e7izer. Bu y\u00f6r\u00fcngeler, izledikleri yola en yak\u0131n bi\u00e7imleri ifade eder, \u00e7\u00fcnk\u00fc kuyruklu y\u0131ld\u0131zlar ayn\u0131 zamanda G\u00fcne\u015f Sistemi’nin dokuz gezegeninin ve kendi \u00e7ekirdeklerinden a\u00e7\u0131\u011fa \u00e7\u0131kan anizotrop gazlar\u0131 \u00e7ekim g\u00fcc\u00fcyle ba\u011flant\u0131s\u0131 olmaks\u0131z\u0131n etkisi alt\u0131ndad\u0131r. Bunlar, y\u00f6r\u00fcnge periyotlar\u0131na g\u00f6re, yani G\u00fcne\u015f’in \u00e7evresinde tam bir dolan\u0131m yapmak i\u00e7in harcad\u0131klar\u0131 zamana g\u00f6re s\u0131n\u0131fland\u0131r\u0131l\u0131rlar. Listesi yap\u0131lan 710 kuyruklu y\u0131ld\u0131zdan 121’inin periyodu 200 y\u0131l\u0131n alt\u0131ndad\u0131r; Bunlara “k\u0131sa periyotlu”‘lar denir. Geriye kalan 589’u da “uzun periyotlular” grubunu olu\u015fturur.<\/p>\n

K\u0131sa periyotlular g\u00fcnberi noktalar\u0131na yakla\u015ft\u0131klar\u0131nda genel olarak birka\u00e7 kez g\u00f6zlemlenebilir, bu da y\u00f6r\u00fcngelerinin kesinlikle belirlenmesini sa\u011flar. Bunlar, G\u00fcne\u015f’in \u00e7evresinde, D\u00fcnya’n\u0131n tutulumuna (D\u00fcnya’n\u0131n G\u00fcne\u015f \u00e7evresindeki y\u00f6r\u00fcnge d\u00fczlemi) oranla biraz daha e\u011fik bir d\u00fczlem i\u00e7inde elips y\u00f6r\u00fcngeler \u00e7izer; \u00e7o\u011fu zaman D\u00fcnya ve \u00f6teki gezegenler y\u00f6n\u00fcnde d\u00f6nerler (do\u011fru y\u00f6n). <\/p>\n

Y\u0131ld\u0131zlar aras\u0131 dola\u015fan cisimler ve kuyruklu y\u0131ld\u0131zlar<\/span><\/h2>\n

Y\u0131ld\u0131zlararas\u0131 cisimler y\u0131ld\u0131zlararas\u0131 bo\u015flukta bulunan ve yer\u00e7ekimsel olarak bir y\u0131ld\u0131za ba\u011fl\u0131 olmayan bir kuyruklu y\u0131ld\u0131zlard\u0131r. Bilinen G\u00fcne\u015f Sistemi\u2019ndeki veya G\u00fcne\u015f d\u0131\u015f\u0131 kuyruklu y\u0131ld\u0131zlar , d\u0131\u015f\u0131nda, bir y\u0131ld\u0131za yer\u00e7ekimsel olarak ba\u011fl\u0131 olmayan bir y\u0131ld\u0131zlararas\u0131 kuyruklu y\u0131ld\u0131z bulunmam\u0131\u015ft\u0131r. Yine de bu kuyruklu y\u0131ld\u0131zlar\u0131n var oldu\u011fu varsay\u0131lmaktad\u0131r: gezegen ve y\u0131ld\u0131zlardan kaynaklanan yer\u00e7ekimsel da\u011f\u0131tma, pek \u00e7ok Oort Bulutu kuyruklu y\u0131ld\u0131z\u0131n\u0131 f\u0131rlatm\u0131\u015ft\u0131r ve benzeri s\u00fcre\u00e7lerin g\u00fcne\u015fd\u0131\u015f\u0131 gezegen sistemlerde de ger\u00e7ekle\u015fme olas\u0131l\u0131\u011f\u0131n\u0131n y\u00fcksekli\u011fi, b\u00fcy\u00fck miktarda ba\u011f\u0131ms\u0131z kuyruklu y\u0131ld\u0131z\u0131n varl\u0131\u011f\u0131na i\u015faret etmektedir. G\u00fcn\u00fcm\u00fczde, y\u0131ld\u0131zlaras\u0131 kuyuklu y\u0131ld\u0131zlar yaln\u0131zca G\u00fcne\u015f Sistemi\u2019nden ge\u00e7erlerse fark edilebilir ve Oort Bulutu kuyruklu y\u0131ld\u0131zlar\u0131ndan, G\u00fcne\u015f\u2019e yer\u00e7ekimsel olarak ba\u011fl\u0131 olmad\u0131klar\u0131na i\u015faret eden, sert hiperbolik y\u00f6r\u00fcngeleri sayesinde ay\u0131rt edilirler. Zay\u0131f hiperbolik y\u00f6r\u00fcngelere sahip kuyruklu y\u0131ld\u0131zlar da g\u00f6zlemlenmi\u015ftir; ancak bunlar\u0131n y\u00f6r\u00fcngelerine bak\u0131ld\u0131\u011f\u0131nda, Oort Bulutu’ndan serbest kalm\u0131\u015f gibi durduklar\u0131 ve bir y\u0131ld\u0131zlararas\u0131 bo\u015fluk k\u00f6kenine i\u015faret etmedikleri g\u00f6r\u00fclm\u00fc\u015ft\u00fcr. Bilinen en d\u0131\u015f merkezli olan(eccentric) kuyruklu y\u0131ld\u0131z, C\/1980 E1, yaln\u0131zca 1.057 d\u0131\u015f merkezlili\u011fe sahiptir,[6] ki bu da bir y\u0131ld\u0131zlararas\u0131 kuyruklu y\u0131ld\u0131zdan beklenene g\u00f6re, pek d\u0131\u015f merkezli de\u011fildir.<\/p>\n

G\u00fcncel Oort bulutu olu\u015fumu modelleri, y\u0131ld\u0131zlararas\u0131 bo\u015flu\u011fa at\u0131lan kuyruklu y\u0131ld\u0131z say\u0131s\u0131n\u0131n, bulutta kalan kuyruklu y\u0131ld\u0131zlar\u0131n say\u0131s\u0131ndan 3-100 kat fazla oldu\u011funa i\u015faret etmektedir. Ba\u015fka sim\u00fclasyonlar ise, buluttaki kuyruklu y\u0131ld\u0131zlar\u0131n 90-95%’inin d\u0131\u015far\u0131 p\u00fcsk\u00fcrt\u00fcld\u00fc\u011f\u00fcn\u00fc ileri s\u00fcrmektedir. Ba\u015fka y\u0131ld\u0131z sistemlerinde olu\u015fmu\u015f olan kuyruklu y\u0131ld\u0131zlar\u0131n da benzer bir bi\u00e7imde p\u00fcsk\u00fcrt\u00fclmemesi i\u00e7in bir sebep yoktur<\/p>\n

E\u011fer y\u0131ld\u0131zlararas\u0131 cisimler var ise, i\u00e7 G\u00fcne\u015f Sistemi’nden arada s\u0131rada ge\u00e7meleri gerekmektedir. G\u00fcne\u015f Sistemi, Hercules Tak\u0131my\u0131ld\u0131z\u0131’na do\u011fru ilerledi\u011fi i\u00e7in, daha \u00e7ok bu kuyruklu y\u0131ld\u0131zlar\u0131n rastgele h\u0131zlarla bu tak\u0131my\u0131ld\u0131z\u0131n\u0131n oldu\u011fu b\u00f6lgeden geliyor olmalar\u0131 beklenmektedir. Hen\u00fcz G\u00fcne\u015f’in kurtulma h\u0131z\u0131ndan daha h\u0131zl\u0131 bir kuyruklu y\u0131ld\u0131za rastlan\u0131lmam\u0131\u015f olmas\u0131, bu konuda \u00fcst s\u0131n\u0131r\u0131 y\u0131ld\u0131zlararas\u0131 bo\u015flu\u011fun yo\u011funlu\u011funa ba\u011f\u0131ml\u0131 k\u0131lmaktad\u0131r. Torbett taraf\u0131ndan yaz\u0131lm\u0131\u015f bir makaleye g\u00f6re, bu yo\u011funluk k\u00fcbik parsek ba\u015f\u0131na 1013 (10 trilyon) kuyruklu y\u0131ld\u0131zdan fazla de\u011fildir.<\/p>\n

\u00c7ok nadir de olsa, y\u0131ld\u0131zlararas\u0131 cisimler, G\u00fcne\u015f Sistemi’nden ge\u00e7ereken g\u00fcnmerkezli y\u00f6r\u00fcngelere girebilir. Bilgisayar sim\u00fclasyonlar\u0131, J\u00fcpiter’in b\u00f6yle bir kuyruklu y\u0131ld\u0131z\u0131 yakalayabilecek k\u00fctleye sahip tek gezegen oldu\u011funu ve bunun her altm\u0131\u015f milton y\u0131lda bir ger\u00e7ekle\u015fmesinin beklenebilece\u011fini ortaya koymaktad\u0131r.Machholz 1 ve Hyakutake C\/1996 B2 kuyruklu y\u0131ld\u0131zlar\u0131, bu t\u00fcr kuyruklu y\u0131ld\u0131zlara \u00f6rnek olma potansiyelini ta\u015f\u0131maktad\u0131r: G\u00fcne\u015f Sistemi’ndeki kuyruklu y\u0131ld\u0131zlara g\u00f6re \u00e7ok daha farkl\u0131 bir kimyasal yap\u0131lar\u0131 vard\u0131r<\/p>\n","protected":false},"excerpt":{"rendered":"

Kuyruklu y\u0131ld\u0131zlar\u0131n b\u00f6l\u00fcmleri: a. N\u00fcve: Nispeten kat\u0131 ve kararl\u0131 olan \u00e7ekirdek, su buzu ve di\u011fer donmu\u015f gazlar ve az miktarda kozmik toz ve di\u011fer kat\u0131 cisimlerden olu\u015fmu\u015ftur. b. Koma: \u00c7ekirdekten buharla\u015fan su, karbondioksit ve di\u011fer n\u00f6tr gazlar\u0131n yo\u011fun bir bulutudur. N\u00fcveyi \u00e7evreleyen \u0131\u015f\u0131k topu \u015feklinde g\u00f6r\u00fcl\u00fcr. c. Hidrojen bulutu: \u00c7ok b\u00fcy\u00fck (milyonlarca km) ancak son […]<\/p>\n","protected":false},"author":23,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":""},"categories":[506],"tags":[],"class_list":["post-47575","post","type-post","status-publish","format-standard","hentry","category-astronomi"],"acf":[],"yoast_head":"\nKuyruklu y\u0131ld\u0131zlar ve t\u00fcrleri - Online Star Register<\/title>\n<meta name=\"description\" content=\"Kuyruklu y\u0131ld\u0131zlar asl\u0131nda nedir ve nas\u0131l s\u0131n\u0131fland\u0131r\u0131l\u0131rlar...\" \/>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/osr.org\/tr\/blog\/astronomi\/kuyruklu-yildizlar-ve-turleri\/\" \/>\n<meta property=\"og:locale\" content=\"tr_TR\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Kuyruklu y\u0131ld\u0131zlar ve t\u00fcrleri - Online Star Register\" \/>\n<meta property=\"og:description\" content=\"Kuyruklu y\u0131ld\u0131zlar asl\u0131nda nedir ve nas\u0131l s\u0131n\u0131fland\u0131r\u0131l\u0131rlar...\" \/>\n<meta property=\"og:url\" content=\"https:\/\/osr.org\/tr\/blog\/astronomi\/kuyruklu-yildizlar-ve-turleri\/\" \/>\n<meta property=\"og:site_name\" content=\"Online Star Register\" \/>\n<meta property=\"article:published_time\" content=\"2018-09-15T06:47:50+00:00\" \/>\n<meta property=\"article:modified_time\" content=\"2018-09-15T08:37:48+00:00\" \/>\n<meta name=\"author\" content=\"Hatice Utkan Ozden\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Written by\" \/>\n\t<meta name=\"twitter:data1\" content=\"Hatice Utkan Ozden\" \/>\n\t<meta name=\"twitter:label2\" content=\"Est. reading time\" \/>\n\t<meta name=\"twitter:data2\" content=\"6 minutes\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\n\t \"@context\": \"https:\/\/schema.org\",\n\t \"@graph\": [\n\t {\n\t \"@type\": \"WebPage\",\n\t \"@id\": \"https:\/\/osr.org\/tr\/blog\/astronomi\/kuyruklu-yildizlar-ve-turleri\/\",\n\t \"url\": \"https:\/\/osr.org\/tr\/blog\/astronomi\/kuyruklu-yildizlar-ve-turleri\/\",\n\t \"name\": \"Kuyruklu y\u0131ld\u0131zlar ve t\u00fcrleri - Online Star Register\",\n\t \"isPartOf\": {\n\t \"@id\": \"https:\/\/osr.org\/tr\/#website\"\n\t },\n\t \"datePublished\": \"2018-09-15T06:47:50+00:00\",\n\t \"dateModified\": \"2018-09-15T08:37:48+00:00\",\n\t \"author\": {\n\t \"@id\": \"https:\/\/osr.org\/tr\/#\/schema\/person\/ef86e8c767dff5d728379a636d34a85a\"\n\t },\n\t \"description\": \"Kuyruklu y\u0131ld\u0131zlar asl\u0131nda nedir ve nas\u0131l s\u0131n\u0131fland\u0131r\u0131l\u0131rlar...\",\n\t \"breadcrumb\": {\n\t \"@id\": \"https:\/\/osr.org\/tr\/blog\/astronomi\/kuyruklu-yildizlar-ve-turleri\/#breadcrumb\"\n\t },\n\t \"inLanguage\": \"tr\",\n\t \"potentialAction\": [\n\t {\n\t \"@type\": \"ReadAction\",\n\t \"target\": [\n\t \"https:\/\/osr.org\/tr\/blog\/astronomi\/kuyruklu-yildizlar-ve-turleri\/\"\n\t ]\n\t }\n\t ]\n\t },\n\t {\n\t \"@type\": \"BreadcrumbList\",\n\t \"@id\": \"https:\/\/osr.org\/tr\/blog\/astronomi\/kuyruklu-yildizlar-ve-turleri\/#breadcrumb\",\n\t \"itemListElement\": [\n\t {\n\t \"@type\": \"ListItem\",\n\t \"position\": 1,\n\t \"name\": \"Home\",\n\t \"item\": \"https:\/\/osr.org\/tr\/\"\n\t },\n\t {\n\t \"@type\": \"ListItem\",\n\t \"position\": 2,\n\t \"name\": \"Astronomi\",\n\t \"item\": \"https:\/\/osr.org\/tr\/astronomi\/\"\n\t },\n\t {\n\t \"@type\": \"ListItem\",\n\t \"position\": 3,\n\t \"name\": \"Kuyruklu y\u0131ld\u0131zlar ve t\u00fcrleri\"\n\t }\n\t ]\n\t },\n\t {\n\t \"@type\": \"WebSite\",\n\t \"@id\": \"https:\/\/osr.org\/tr\/#website\",\n\t \"url\": \"https:\/\/osr.org\/tr\/\",\n\t \"name\": \"Online Star Register\",\n\t \"description\": \"\",\n\t \"potentialAction\": [\n\t {\n\t \"@type\": \"SearchAction\",\n\t \"target\": {\n\t \"@type\": \"EntryPoint\",\n\t \"urlTemplate\": \"https:\/\/osr.org\/tr\/?s={search_term_string}\"\n\t },\n\t \"query-input\": {\n\t \"@type\": \"PropertyValueSpecification\",\n\t \"valueRequired\": true,\n\t \"valueName\": \"search_term_string\"\n\t }\n\t }\n\t ],\n\t \"inLanguage\": \"tr\"\n\t },\n\t {\n\t \"@type\": \"Person\",\n\t \"@id\": \"https:\/\/osr.org\/tr\/#\/schema\/person\/ef86e8c767dff5d728379a636d34a85a\",\n\t \"name\": \"Hatice Utkan Ozden\",\n\t \"description\": \"Hatice Utkan \u00d6zden is a writer and a journalist. 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