{"id":42,"date":"2013-03-29T00:30:47","date_gmt":"2013-03-28T22:30:47","guid":{"rendered":"http:\/\/blog.metu.edu.tr\/esenturk\/?p=42"},"modified":"2017-05-22T21:15:05","modified_gmt":"2017-05-22T18:15:05","slug":"gezegenler","status":"publish","type":"post","link":"https:\/\/blog.metu.edu.tr\/esenturk\/gezegenler\/","title":{"rendered":"Gezegenler hakk\u0131nda baz\u0131 ger\u00e7ekler…"},"content":{"rendered":"

Views: 399<\/p>

\"hgv\"<\/a><\/p>\n

Ven\u00fcs ad\u0131n\u0131 Romal\u0131lar\u0131n A\u015fk ve G\u00fczellik Tanr\u0131\u00e7as\u0131 Ven\u00fcs\u2019ten alm\u0131\u015ft\u0131r. \u00a0(Ven\u00fcs, Yunan Tanr\u0131\u00e7as\u0131 Afrodit\u2019in kar\u015f\u0131l\u0131\u011f\u0131d\u0131r). \u00a0Ven\u00fcs\u2019\u00fcn g\u00fczellik tanr\u0131\u00e7as\u0131ndan ismini almas\u0131n\u0131n antik \u00e7a\u011fdaki\u00a0g\u00f6k bilimcilerin\u00a0g\u00f6ky\u00fcz\u00fcnde bildi\u011fi\u00a05 gezegenden en parlak olan\u0131 olmas\u0131ndan kaynakland\u0131\u011f\u0131na inan\u0131l\u0131yor.<\/span><\/p>\n

Bilinen uydusu olmayan Ven\u00fcs, y\u00fczey s\u0131cakl\u0131\u011f\u0131 yakla\u015f\u0131k 462 santigrat derece olan g\u00fcne\u015f sistemindeki en s\u0131cak gezegendir. G\u00fcne\u015f Sistemindeki di\u011fer t\u00fcm gezegenlere k\u0131yasla kendi ekseni etraf\u0131nda aksi y\u00f6nde d\u00f6nen tek gezegen Ven\u00fcs’t\u00fcr. \u00a0<\/span><\/p>\n

Sat\u00fcrn, \u00e7evresinde halkalar\u0131 olan tek gezegen de\u011fil; J\u00fcpiter, Uran\u00fcs, Nept\u00fcn gibi di\u011fer gaz devleri de halkalara sahip, sadece halkalar\u0131 \u00e7ok belirgin de\u011fil.\u00a0<\/span><\/p>\n

60’\u0131n \u00fczerinde uydusu bulunan J\u00fcpiter’in kendi i\u00e7lerinde gezegen say\u0131labilecek 4 b\u00fcy\u00fck uydusu vard\u0131r. Bu uydular: Europa (Yuropa), Ganymede (Ganimed), Callisto (Kalisto) ve Io(Ayo)’dur.<\/p>\n

Kutbu g\u00fcne\u015fe bakacak \u015fekilde, y\u00f6r\u00fcngesi \u00fcst\u00fcne yatm\u0131\u015f \u00a0bir f\u0131\u00e7\u0131 gibi d\u00f6nen tek gezegen Uran\u00fcs’t\u00fcr.<\/p>\n

2006\u2019da Uluslararas\u0131 Astronomi Birli\u011fi, gezegen tan\u0131m\u0131n\u0131 de\u011fi\u015ftirdi. Yeni tan\u0131ma g\u00f6re art\u0131k Pl\u00fcton bir c\u00fcce gezegen.<\/p>\n

Ceres (Seres) Mars ve J\u00fcpiter aras\u0131ndaki asteroit ku\u015fa\u011f\u0131nda yer almaktad\u0131r.\u00a0Nept\u00fcn’den 45 y\u0131l \u00f6nce, Pl\u00fcton’dan da \u00f6nce iyi bilinen Ceres (Seres), 1801 y\u0131l\u0131nda ke\u015ffedilmi\u015ftir. \u00a0Yakla\u015f\u0131k 50 y\u0131l boyunca bir gezegen olarak d\u00fc\u015f\u00fcn\u00fclen Ceres (Seres), sonralar\u0131 Asteroit ve 2006 y\u0131l\u0131nda c\u00fcce gezegen olarak s\u0131n\u0131fland\u0131r\u0131lm\u0131\u015ft\u0131r.<\/p>\n

2005 y\u0131l\u0131nda ke\u015ffedilen Eris, 2006 y\u0131l\u0131nda c\u00fcce gezegen olarak yeniden s\u0131n\u0131fland\u0131r\u0131l\u0131ncaya kadar 10. gezegen olarak\u00a0kabul\u00a0g\u00f6rm\u00fc\u015ft\u00fc. G\u00fcne\u015f sisteminde bilinen en b\u00fcy\u00fck c\u00fcce gezegendir.<\/p>\n

<\/em>Kaynak\u00e7a<\/em><\/p>\n[1] http:\/\/solarsystem.nasa.gov\/planets\/profile.cfm?Object=Venus&Display=OverviewLong<\/p>\n[2] http:\/\/solarsystem.nasa.gov\/planets\/profile.cfm?Display=Facts&Object=Venus<\/p>\n[3]\u00a0http:\/\/www.sciencekids.co.nz\/sciencefacts\/space.html<\/p>\n[4]\u00a0http:\/\/www.sciencekids.co.nz\/sciencefacts\/space\/dwarfplanets.html<\/p>\n[5]\u00a0http:\/\/apod.nasa.gov\/apod\/image\/0608\/planets_iau_big.jpg<\/p>\n","protected":false},"excerpt":{"rendered":"

Views: 399 Ven\u00fcs ad\u0131n\u0131 Romal\u0131lar\u0131n A\u015fk ve G\u00fczellik Tanr\u0131\u00e7as\u0131 Ven\u00fcs\u2019ten alm\u0131\u015ft\u0131r. \u00a0(Ven\u00fcs, Yunan Tanr\u0131\u00e7as\u0131 Afrodit\u2019in kar\u015f\u0131l\u0131\u011f\u0131d\u0131r). \u00a0Ven\u00fcs\u2019\u00fcn g\u00fczellik tanr\u0131\u00e7as\u0131ndan ismini almas\u0131n\u0131n antik \u00e7a\u011fdaki\u00a0g\u00f6k bilimcilerin\u00a0g\u00f6ky\u00fcz\u00fcnde bildi\u011fi\u00a05 gezegenden en parlak olan\u0131 olmas\u0131ndan kaynakland\u0131\u011f\u0131na inan\u0131l\u0131yor. Bilinen uydusu olmayan Ven\u00fcs, y\u00fczey s\u0131cakl\u0131\u011f\u0131 yakla\u015f\u0131k 462 santigrat derece olan g\u00fcne\u015f sistemindeki en s\u0131cak gezegendir. G\u00fcne\u015f Sistemindeki di\u011fer t\u00fcm gezegenlere k\u0131yasla kendi […]<\/p>\n","protected":false},"author":1394,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":"","_links_to":"","_links_to_target":""},"categories":[21],"tags":[],"class_list":["post-42","post","type-post","status-publish","format-standard","hentry","category-biliyor-muydunuz"],"_links":{"self":[{"href":"https:\/\/blog.metu.edu.tr\/esenturk\/wp-json\/wp\/v2\/posts\/42","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/blog.metu.edu.tr\/esenturk\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/blog.metu.edu.tr\/esenturk\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/blog.metu.edu.tr\/esenturk\/wp-json\/wp\/v2\/users\/1394"}],"replies":[{"embeddable":true,"href":"https:\/\/blog.metu.edu.tr\/esenturk\/wp-json\/wp\/v2\/comments?post=42"}],"version-history":[{"count":0,"href":"https:\/\/blog.metu.edu.tr\/esenturk\/wp-json\/wp\/v2\/posts\/42\/revisions"}],"wp:attachment":[{"href":"https:\/\/blog.metu.edu.tr\/esenturk\/wp-json\/wp\/v2\/media?parent=42"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/blog.metu.edu.tr\/esenturk\/wp-json\/wp\/v2\/categories?post=42"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/blog.metu.edu.tr\/esenturk\/wp-json\/wp\/v2\/tags?post=42"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}