{"id":4879,"date":"2023-08-04T18:32:23","date_gmt":"2023-08-04T15:32:23","guid":{"rendered":"https:\/\/www.blog.extremeoutdoor.com.tr\/?p=4879"},"modified":"2023-08-04T18:32:24","modified_gmt":"2023-08-04T15:32:24","slug":"gunes-sistemindeki-gezegenler-ve-ozellikleri","status":"publish","type":"post","link":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/2023\/08\/04\/gunes-sistemindeki-gezegenler-ve-ozellikleri\/","title":{"rendered":"G\u00fcne\u015f Sistemindeki Gezegenler ve \u00d6zellikleri"},"content":{"rendered":"

S\u00fcrekli geni\u015fleyen evrenin h\u0131z\u0131na eri\u015fmek m\u00fcmk\u00fcn de\u011fil. Uzay ke\u015fifleri heyecan verici seyahatlerle devam etse de evrenin s\u0131rr\u0131na vak\u0131f olmak suya yaz\u0131 yazmaya benziyor. Neyse ki g\u00fcne\u015f sistemi daha hesaplanabilir ve g\u00f6zlemlenebilir ger\u00e7ekler sunuyor. G\u00fcne\u015f sistemindeki gezegenler<\/strong> hakk\u0131nda baz\u0131lar\u0131n\u0131 bildi\u011finiz fakat bir\u00e7o\u011funu ilk kez duyaca\u011f\u0131n\u0131z \u015fa\u015f\u0131rt\u0131c\u0131 bilgiler i\u00e7in bu rehberi okuyabilirsiniz.<\/p>

\"\"<\/figure>

G\u00fcne\u015f sisteminde D\u00fcnya da dahil olmak \u00fczere toplamda 8 gezegen bulunuyor. Bunlardan ilk d\u00f6rd\u00fc i\u00e7 gezegenler<\/strong>, son d\u00f6rd\u00fc ise d\u0131\u015f gezegenler olarak s\u0131n\u0131fland\u0131r\u0131l\u0131yor. G\u00fcne\u015f sistemindeki gezegenler ve \u00f6zelliklerini yaz\u0131m\u0131z\u0131n devam\u0131nda bulabilirsin. Teorik bilgilerinizi prati\u011fe d\u00f6kmek i\u00e7in b\u00fct\u00e7enize uygun teleskop<\/strong> modellerine de g\u00f6z atmay\u0131 unutmay\u0131n!<\/p>

\"\"<\/figure>

Merk\u00fcr<\/strong><\/h2>

Gezegenler g\u00fcne\u015fe yak\u0131nl\u0131klar\u0131na g\u00f6re s\u0131raland\u0131\u011f\u0131nda, Merk\u00fcr ilk s\u0131rada yer al\u0131yor. G\u00fcne\u015f sistemindeki sekiz gezegen aras\u0131nda en k\u00fc\u00e7\u00fc\u011f\u00fc olan Merk\u00fcr hakk\u0131nda olduk\u00e7a ilgin\u00e7 bilgiler var. <\/p>

  • Ekvator \u00c7ap\u0131:<\/strong> 4.879 km<\/li>\n\n
  • Kutup \u00c7ap\u0131:<\/strong> 4.879 km<\/li>\n\n
  • Ekvator \u00c7evresi:<\/strong> 15.329 km<\/li>\n\n
  • Y\u00f6r\u00fcnge Periyodu:<\/strong> 87.97 D\u00fcnya g\u00fcn\u00fc<\/li>\n\n
  • Y\u00fczey S\u0131cakl\u0131\u011f\u0131:<\/strong> -173 ila 427 \u00b0C<\/li>\n\n
  • Uydu:<\/strong> Yok<\/li><\/ul>

    Merk\u00fcr hakk\u0131nda ilgin\u00e7 bilgiler:<\/strong><\/h3>
    • Merk\u00fcr\u2019\u00fcn ke\u015ffedilme tarihi bilinmemekle birlikte ilk olarak M.\u00d6. 3000 civar\u0131nda S\u00fcmerliler taraf\u0131ndan s\u00f6z edildi\u011fine inan\u0131l\u0131yor.<\/li>\n\n
    • Merk\u00fcr\u2019de bir y\u0131l yakla\u015f\u0131k 88 g\u00fcn s\u00fcrmesine ra\u011fmen bir Merk\u00fcr g\u00fcn\u00fc 176 g\u00fcn\u00fcne tekab\u00fcl ediyor.<\/li>\n\n
    • Merk\u00fcr g\u00fcne\u015f sistemindeki en k\u00fc\u00e7\u00fck gezegen olmas\u0131na ra\u011fmen \u00e7\u0131plak g\u00f6zle g\u00f6r\u00fclebilen be\u015f gezegenden biri.<\/li>\n\n
    • G\u00fcne\u015f sisteminde metal ve kayalar\u0131n olu\u015fturdu\u011fu d\u00f6rt i\u00e7 gezegen aras\u0131nda yer al\u0131yor. <\/li>\n\n
    • G\u00fcne\u015f etraf\u0131ndaki h\u0131zl\u0131 hareketi nedeniyle ad\u0131n\u0131 Yunan mitolojisinde Hermes olarak da bilinen Roma tanr\u0131lar\u0131n\u0131n el\u00e7isi olan Merk\u00fcr\u2019den al\u0131yor. <\/li>\n\n
    • G\u00fcne\u015fe en yak\u0131n gezegen olmas\u0131na ra\u011fmen en s\u0131cak ikinci gezegen olarak biliniyor.<\/li>\n\n
    • Merk\u00fcr, D\u00fcnya\u2019daki yer\u00e7ekiminin yaln\u0131zca %38\u2019ine sahip; bu nedenle hem uydular\u0131 hem de halkalar\u0131 yok. Ayr\u0131ca d\u00fc\u015f\u00fck yer\u00e7ekiminden dolay\u0131 \u00e7ok ince bir atmosfer tabakas\u0131 var.<\/li>\n\n
    • Merk\u00fcr\u2019\u00fcn y\u00fczeyi t\u0131pk\u0131 Ay gibi kraterlerle dolu. \u00c7o\u011fu gezegenin aksine jeolojik olarak aktif olmad\u0131\u011f\u0131ndan asteroit ve kuyruklu y\u0131ld\u0131zlar\u0131n olu\u015fturdu\u011fu kraterler oldu\u011fu gibi kal\u0131yor.<\/li>\n\n
    • Merk\u00fcr\u2019\u00fc ziyaret eden uzay arac\u0131 say\u0131s\u0131 sadece iki; bunlardan ilki 1973\u2019te f\u0131rlat\u0131lan Mariner 10, ikincisi ise 2004\u2019te g\u00f6nderilen MESSENGER uzay sondas\u0131. <\/li><\/ul>
      \"\"<\/figure>

      Ven\u00fcs<\/strong><\/h2>

      Boyutlar\u0131 ve k\u00fctleleri benzedi\u011fi i\u00e7in D\u00fcnya\u2019n\u0131n karde\u015f gezegeni olarak adland\u0131r\u0131lan Ven\u00fcs ayn\u0131 zamanda D\u00fcnya\u2019ya en yak\u0131n gezegen. \u0130smini Roma mitolojisinde a\u015fk ve g\u00fczellik tanr\u0131\u00e7as\u0131 Ven\u00fcs\u2019ten alan bu i\u00e7 gezegenin \u00f6zellikleri \u015fu \u015fekilde:<\/p>

      • Ekvator \u00c7ap\u0131:<\/strong> 12.104 km<\/li>\n\n
      • Kutup \u00c7ap\u0131:<\/strong> 12.104 km<\/li>\n\n
      • Ekvator \u00c7evresi:<\/strong> 38.025 km<\/li>\n\n
      • Y\u00f6r\u00fcnge Periyodu:<\/strong> 224.70 D\u00fcnya g\u00fcn\u00fc<\/li>\n\n
      • Y\u00fczey S\u0131cakl\u0131\u011f\u0131: <\/strong>462 \u00b0C<\/li>\n\n
      • Uydu:<\/strong> Yok<\/li><\/ul>

        Ven\u00fcs hakk\u0131nda ilgin\u00e7 bilgiler:<\/strong><\/h3>
        • Uydusu olmayan gezegenler<\/strong> aras\u0131nda bulunan Ven\u00fcs, g\u00fcne\u015f sisteminde G\u00fcne\u015f ve Ay\u2019dan sonraki en parlak ikinci nesne olarak biliniyor.<\/li>\n\n
        • Ven\u00fcs\u2019te bir g\u00fcn ge\u00e7irmek bir y\u0131l ge\u00e7irmekten daha uzun s\u00fcr\u00fcyor. Kendi ekseni etraf\u0131ndaki d\u00f6n\u00fc\u015f\u00fcn\u00fc 243 g\u00fcnde tamamlayan bu gezegen y\u00f6r\u00fcne turunu ise 225 g\u00fcnde tamaml\u0131yor.<\/li>\n\n
        • Ven\u00fcs\u2019\u00fcn de t\u0131pk\u0131 D\u00fcnya gibi merkezi bir \u00e7ekirde\u011fi, erimi\u015f bir mantosu ve kabu\u011fu var. <\/li>\n\n
        • Bilim insanlar\u0131 Ven\u00fcs\u2019\u00fcn bir zamanlar b\u00fcy\u00fck miktarda su kayna\u011f\u0131 oldu\u011funa inan\u0131yor fakat a\u015f\u0131r\u0131 sera etkisinden kaynaklanan y\u00fcksek s\u0131cakl\u0131klar bu sular\u0131 buharla\u015ft\u0131rd\u0131\u011f\u0131 i\u00e7in gezegenin y\u00fczeyi ya\u015famak i\u00e7in \u00e7ok s\u0131cak, hatta g\u00fcne\u015f sisteminin en s\u0131ca\u011f\u0131.<\/li>\n\n
        • Ven\u00fcs y\u00fczeyinin tahmini ya\u015f\u0131 300 ila 400 milyon y\u0131l civar\u0131nda. D\u00fcnya y\u00fczeyinin yakla\u015f\u0131k 100 milyon ya\u015f\u0131nda oldu\u011fu d\u00fc\u015f\u00fcn\u00fcl\u00fcrse olduk\u00e7a ya\u015fl\u0131 bir gezegen.<\/li>\n\n
        • Ven\u00fcs\u2019\u00fcn atmosferin bas\u0131nc\u0131 D\u00fcnya\u2019dakinden 92 kat daha g\u00fc\u00e7l\u00fc. Bu da atmosfere giren herhangi bir cismin muazzam bas\u0131n\u00e7 alt\u0131nda eriyip gitti\u011fi anlam\u0131na geliyor. Haliyle Ven\u00fcs\u2019\u00fcn y\u00fczeyinde kraterlere rastlamak pek m\u00fcmk\u00fcn de\u011fil.<\/li>\n\n
        • Ven\u00fcs, g\u00fcne\u015f sisteminde ad\u0131n\u0131 bir kad\u0131n fig\u00fcr\u00fcnden alan tek gezegen. <\/li>\n\n
        • Di\u011fer gezegenlerin \u00e7o\u011fu kendi eksenindeki d\u00f6n\u00fc\u015flerini saat y\u00f6n\u00fcn\u00fcn tersine do\u011fru ger\u00e7ekle\u015ftirirken, Ven\u00fcs biraz farkl\u0131 davran\u0131yor. T\u0131pk\u0131 Uran\u00fcs gibi saat y\u00f6n\u00fcnde d\u00f6nen Ven\u00fcs\u2019\u00fcn ge\u00e7mi\u015f zamanda sert bir \u00e7arp\u0131\u015fma ya\u015fad\u0131\u011f\u0131na inan\u0131l\u0131yor.  <\/li>\n\n
        • Ven\u00fcs\u2019\u00fcn etraf\u0131n\u0131 kaplayan toz bulutlar\u0131 devasa kal\u0131nl\u0131kta oldu\u011fu i\u00e7in y\u00fczeyini g\u00f6zlemlemek pek de kolay olmuyor. Neyse ki 1978\u2019de Pioneer Ven\u00fcs uzay arac\u0131n\u0131n giri\u015fimlerinden beri radar haritalama y\u00f6ntemiyle Ven\u00fcs y\u00fczeyi hakk\u0131nda daha \u00e7ok bilgi ediniliyor.<\/li><\/ul>
          \"\"<\/figure>

          D\u00fcnya<\/strong><\/h2>

          G\u00fcne\u015f sisteminde ad\u0131n\u0131 mitolojik bir varl\u0131ktan almayan ve \u00fczerinde ya\u015fam varl\u0131\u011f\u0131 olan tek gezegen: D\u00fcnya. Bir\u00e7ok a\u00e7\u0131dan benzersiz \u00f6zellikler ta\u015f\u0131yan D\u00fcnyam\u0131z milyarlarca y\u0131l \u00f6nce ya\u015fam kavram\u0131n\u0131n ortaya \u00e7\u0131kt\u0131\u011f\u0131 tek yer.<\/p>

          • Ekvator \u00c7ap\u0131:<\/strong> 12.756 km<\/li>\n\n
          • Kutup \u00c7ap\u0131:<\/strong> 12.714 km<\/li>\n\n
          • Ekvator \u00c7evresi:<\/strong> 40.030 km<\/li>\n\n
          • Y\u00f6r\u00fcnge Periyodu:<\/strong> 365.26 D\u00fcnya g\u00fcn\u00fc<\/li>\n\n
          • Y\u00fczey S\u0131cakl\u0131\u011f\u0131:<\/strong> -88 ila 58 \u00b0C<\/li>\n\n
          • Uydu:<\/strong> Ay<\/li><\/ul>

            D\u00fcnya hakk\u0131nda ilgin\u00e7 bilgiler:<\/strong><\/h3>
            • Etimolojik k\u00f6kenine g\u00f6re D\u00fcnya gezegenin ad\u0131 Arap\u00e7a\u2019da yery\u00fcz\u00fc anlam\u0131na geliyor. \u0130ngilizcedeki \u201cearth\u201d ad\u0131n\u0131 ise eski \u0130ngilizcede toprak anlam\u0131na gelen \u201certha\u201ddan al\u0131yor.<\/li>\n\n
            • B\u00fcy\u00fckl\u00fck ve k\u00fctle bak\u0131m\u0131ndan g\u00fcne\u015f sistemindeki en b\u00fcy\u00fck be\u015finci gezegen olmas\u0131na ra\u011fmen, D\u00fcnya en yo\u011fun gezegen olarak biliniyor. <\/li>\n\n
            • D\u00fcnya\u2019n\u0131n en al\u00e7ak noktas\u0131 kabul edilen Challenger Deep, deniz seviyesinden yakla\u015f\u0131k 10.9 kilometre daha derinde bulunuyor.<\/li>\n\n
            • 1543\u2019te Kopernik, g\u00fcne\u015f sistemi modelini \u00f6nerene dek D\u00fcnya\u2019n\u0131n evrenin merkezi oldu\u011funa inan\u0131l\u0131yordu. <\/li>\n\n
            • D\u00fcnya\u2019n\u0131n d\u00f6n\u00fc\u015f\u00fc insano\u011flu fark etmese de giderek yava\u015fl\u0131yor. Bu yava\u015flama de\u011feri 100 y\u0131lda yaln\u0131zca 17 milisaniye, yani yakla\u015f\u0131k 140 milyon y\u0131l sonra bir g\u00fcn 24 saatten 25 saate \u00e7\u0131kabilir.<\/li>\n\n
            • K\u00fcresel \u0131s\u0131nma<\/strong>\u00a0nedeniyle D\u00fcnya\u2019daki ortalama s\u0131cakl\u0131\u011f\u0131n 2100 y\u0131l\u0131nda 7 derece artaca\u011f\u0131 \u00f6ng\u00f6r\u00fcl\u00fcyor.\u00a0<\/li>\n\n
            • D\u00fcnya\u2019n\u0131n ola\u011fan\u00fcst\u00fc g\u00fc\u00e7l\u00fc manyetik alan\u0131 gezegeni g\u00fcne\u015f r\u00fczgarlar\u0131n\u0131n etkisinden koruyor. <\/li>\n\n
            • D\u00fcnya\u2019daki ilk ya\u015famsal belirtilerin abiyogenez ve biyopoez ad\u0131 verilen biyolojik s\u00fcre\u00e7lerle okyanuslarda geli\u015fti\u011fine inan\u0131l\u0131yor. Bu, ya\u015fam\u0131n basit organik bile\u015fikler gibi cans\u0131z maddelerden geli\u015fti\u011fi do\u011fal bir s\u00fcreci temsil ediyor.<\/li>\n\n
            • G\u00fcne\u015f sistemindeki di\u011fer i\u00e7 gezegenlerle k\u0131yasland\u0131\u011f\u0131nda, D\u00fcnya\u2019da az say\u0131da krater bulunuyor. Bu durum D\u00fcnya\u2019n\u0131n jeolojik olarak aktif olmas\u0131ndan ve y\u00fczeyi yeniden \u015fekillendiren tektonik ve erozyon s\u00fcre\u00e7lerine sahip olmas\u0131ndan kaynaklan\u0131yor.<\/li>\n\n
            • D\u00fcnya\u2019daki suyun ba\u015flang\u0131\u00e7ta gezegenin i\u00e7inde hapsoldu\u011fu ve volkanik aktiviteler nedeniyle zaman i\u00e7inde y\u00fczeye \u00e7\u0131kt\u0131\u011f\u0131 biliniyor.<\/li><\/ul>
              \"\"<\/figure>

              Mars<\/strong><\/h2>

              G\u00fcne\u015fe yak\u0131n gezegenler<\/strong> aras\u0131nda d\u00f6rd\u00fcnc\u00fc s\u0131rada yer alan ve i\u00e7 gezegenlerin sonuncusu olan Mars, kahverengi-k\u0131rm\u0131z\u0131 y\u00fczeyi nedeniyle K\u0131z\u0131l Gezgen olarak da biliniyor. 21. y\u00fczy\u0131l uzay yolculuklar\u0131n\u0131n tutkusu haline gelen bu gezegen heyecan verici \u00f6zellikler ta\u015f\u0131yor.<\/p>

              • Ekvator \u00c7ap\u0131:<\/strong> 6.805 km<\/li>\n\n
              • Kutup \u00c7ap\u0131:<\/strong> 6.755 km<\/li>\n\n
              • Ekvator \u00c7evresi:<\/strong> 21.297 km<\/li>\n\n
              • Y\u00f6r\u00fcnge Periyodu:<\/strong> 686,98 D\u00fcnya g\u00fcn\u00fc<\/li>\n\n
              • Y\u00fczey S\u0131cakl\u0131\u011f\u0131:<\/strong> -87 ila 5 \u00b0C<\/li>\n\n
              • Uydu:<\/strong> Phobos ve Deimos<\/li><\/ul>

                Mars hakk\u0131nda ilgin\u00e7 bilgiler:<\/strong><\/h3>
                • Gezegen, ad\u0131n\u0131 Roma sava\u015f tanr\u0131s\u0131 Mars\u2019tan al\u0131yor. \u00c7inli g\u00f6kbilimciler Mars\u2019\u0131 \u201cate\u015f y\u0131ld\u0131z\u0131\u201d olarak adland\u0131r\u0131rken, eski M\u0131s\u0131rl\u0131 rahipler ise Mars\u2019a \u201ck\u0131rm\u0131z\u0131 olan\u201d anlam\u0131na gelen \u2018her desher\u2019 ad\u0131n\u0131 verdiler.<\/li>\n\n
                • Mars\u2019\u0131n Phobos ve Deimos ad\u0131nda iki uydusu bulunuyor. Mars\u2019\u0131n uydular\u0131yla ilgili \u015fa\u015f\u0131rt\u0131c\u0131 bir ger\u00e7ek daha var. K\u0131z\u0131l gezegenin iki adet uyduya sahip oldu\u011fu hen\u00fcz ke\u015ffedilmemi\u015fken Jonathan Swift\u2019in G\u00fcliver\u2019in Seyahatleri kitab\u0131nda ge\u00e7iyor. <\/li>\n\n
                • Mars\u2019ta da t\u0131pk\u0131 D\u00fcnya gibi farkl\u0131 mevsimler ya\u015fan\u0131yor fakat tek bir farkla, Mars\u2019takiler iki kat daha uzun s\u00fcr\u00fcyor. Bu durum Mars\u2019\u0131n kendi ekseni \u00fczerindeki e\u011fikli\u011finin D\u00fcnya\u2019dan daha fazla olmas\u0131ndan kaynaklan\u0131yor.<\/li>\n\n
                • D\u00fcnya d\u0131\u015f\u0131nda kutup buzullar\u0131na sahip tek gezegen olmas\u0131 Mars\u2019ta ya\u015fam olabilece\u011fi inanc\u0131n\u0131 kuvvetlendiriyor.<\/li>\n\n
                • Bilimkurgu filmlerinde s\u0131k\u00e7a i\u015flenen Marsl\u0131lar ger\u00e7ekte yok, ancak gelecekte burada ya\u015fam kolonisi kurulma ihtimali ke\u015fif projelerine h\u0131z kazand\u0131r\u0131yor. <\/li>\n\n
                • Mars y\u00fczeyine ilk ba\u015far\u0131l\u0131 ini\u015fler 1971 y\u0131l\u0131nda ger\u00e7ekle\u015firken ilk foto\u011fraf g\u00f6nderme g\u00f6revi ise 1988\u2019de Sovyetlerin f\u0131rlatt\u0131\u011f\u0131 uzay ara\u00e7lar\u0131yla sa\u011fland\u0131. 18 \u015eubat 2021 y\u0131l\u0131nda Mars\u2019a ini\u015f yapan Perseverance ke\u015fif arac\u0131 ise g\u00f6revini hala s\u00fcrd\u00fcr\u00fcyor.<\/li>\n\n
                • Mars, D\u00fcnya\u2019n\u0131n yaln\u0131zca %37\u2019si kadar yer\u00e7ekimine sahip. Bu da D\u00fcnya ile k\u0131yasland\u0131\u011f\u0131nda yakla\u015f\u0131k 3 kat daha y\u00fckse\u011fe z\u0131planabilece\u011fi anlam\u0131na geliyor.<\/li>\n\n
                • Mars\u2019ta yakla\u015f\u0131k 21 km y\u00fcksekli\u011fiyle g\u00fcne\u015f sisteminin en y\u00fcksek da\u011f\u0131 olan Oympus Mons yanarda\u011f\u0131 bulunuyor. <\/li>\n\n
                • \u0130nce atmosferin neden oldu\u011fu d\u00fc\u015f\u00fck bas\u0131nca ra\u011fmen, Mars\u2019ta kuvvetli toz f\u0131rt\u0131nalar\u0131, don, sis ve r\u00fczg\u00e2r gibi bir dizi hava olay\u0131 ger\u00e7ekle\u015fiyor.<\/li><\/ul>
                  \"\"<\/figure>

                  J\u00fcpiter<\/strong><\/h2>

                  G\u00fcne\u015f sistemindeki en b\u00fcy\u00fck gezegen olmas\u0131yla bilinen J\u00fcpiter ad\u0131n\u0131 Roma mitolojisindeki g\u00f6ky\u00fcz\u00fc tanr\u0131s\u0131ndan al\u0131yor. Devasa boyutlar\u0131 ilgi \u00e7ekici kar\u015f\u0131la\u015ft\u0131rmalara sebep olan bu J\u00fcpiter\u2019in \u00f6zellikleri \u015fu \u015fekilde:<\/p>

                  • Ekvator \u00c7ap\u0131:<\/strong> 142.984 km<\/li>\n\n
                  • Kutup \u00c7ap\u0131:<\/strong> 133.709 km<\/li>\n\n
                  • Ekvator \u00c7evresi:<\/strong> 439.264 km<\/li>\n\n
                  • Y\u00f6r\u00fcnge Periyodu:<\/strong> 4.333 D\u00fcnya g\u00fcn\u00fc<\/li>\n\n
                  • Y\u00fczey S\u0131cakl\u0131\u011f\u0131:<\/strong> -108 \u00b0C<\/li>\n\n
                  • Uydu:<\/strong> En az 67 adet, en \u00f6nemlileri Io, Europa, Ganymede ve Callisto<\/li><\/ul>

                    J\u00fcpiter hakk\u0131nda ilgin\u00e7 bilgiler:<\/strong><\/h3>
                    • Devasa b\u00fcy\u00fckl\u00fc\u011f\u00fcyle fark yaratan J\u00fcpiter, di\u011fer t\u00fcm gezegenlerin toplam\u0131ndan iki kat daha b\u00fcy\u00fck. Ayr\u0131ca k\u00fctlesi itibariyle D\u00fcnya\u2019dan 317 kat daha a\u011f\u0131r. <\/li>\n\n
                    • J\u00fcpiter\u2019in dev hacmi i\u00e7ine 1300\u2019ten fazla D\u00fcnya\u2019y\u0131 s\u0131\u011fd\u0131rabilir. Bu, bir basketbol topuyla \u00fcz\u00fcm tanesi b\u00fcy\u00fckl\u00fc\u011f\u00fcn\u00fcn kar\u015f\u0131la\u015ft\u0131r\u0131lmas\u0131na benziyor.<\/li>\n\n
                    • J\u00fcpiter\u2019in y\u00fczeyinde bulunan b\u00fcy\u00fck k\u0131rm\u0131z\u0131 nokta y\u00fczy\u0131llard\u0131r devam eden dev bir kas\u0131rgay\u0131 temsil ediyor. Bu kas\u0131rgan\u0131n b\u00fcy\u00fckl\u00fc\u011f\u00fc ise D\u00fcnya\u2019n\u0131n iki kat\u0131 kadar.<\/li>\n\n
                    • Kendi ekseni etraf\u0131nda \u00e7ok h\u0131zl\u0131 d\u00f6nd\u00fc\u011f\u00fc i\u00e7in g\u00fcne\u015f sistemindeki en k\u0131sa g\u00fcn J\u00fcpiter\u2019de ya\u015fan\u0131yor. Bu h\u0131z\u0131 nedeniyle yass\u0131 bir g\u00f6r\u00fcn\u00fcm kazanan J\u00fcpiter\u2019in kendi ekseni etraf\u0131ndaki d\u00f6n\u00fc\u015f\u00fc 9 saat 55 dakikada tamamlan\u0131yor.<\/li>\n\n
                    • Halkas\u0131 olan gezegenlerden biri olan J\u00fcpiter\u2019in etraf\u0131nda asteroit \u00e7arpmalar\u0131 sonucu uydular\u0131ndan kopan par\u00e7alar yer al\u0131yor.<\/li>\n\n
                    • D\u00fcnya\u2019dan bak\u0131ld\u0131\u011f\u0131nda \u00e7\u0131plak g\u00f6zle g\u00f6r\u00fclebilen be\u015f gezegenden biri olan J\u00fcpiter ayn\u0131 zamanda g\u00fcne\u015f sistemindeki en parlak d\u00f6rd\u00fcnc\u00fc nesne.<\/li>\n\n
                    • G\u00fcne\u015f sistemindeki en g\u00fc\u00e7l\u00fc manyetik alana sahip oldu\u011fu i\u00e7in J\u00fcpiter\u2019in bilinen 67 adet uydusu var. J\u00fcpiter uydular\u0131n\u0131n ilk ke\u015ffi ise 1610 y\u0131l\u0131nda Galileo Galilei taraf\u0131ndan ke\u015ffediliyor. En \u00f6nemlileri kabul edilen bu d\u00f6rt uydunun isimleri ise Io, Europa, Ganymede ve Callisto.<\/li><\/ul>
                      \"\"<\/figure>

                      Sat\u00fcrn<\/strong><\/h2>

                      G\u00fcne\u015f sisteminin \u00e7ap ve k\u00fctle bak\u0131m\u0131ndan en b\u00fcy\u00fck ikinci gezegeni olan Sat\u00fcrn, J\u00fcpiter\u2019le olduk\u00e7a benzer \u00f6zellikler ta\u015f\u0131yor. Bu akrabal\u0131k mitolojiye de yans\u0131m\u0131\u015f olacak ki ismini Roma mitolojisindeki J\u00fcpiter\u2019in babas\u0131ndan al\u0131yor. Halkal\u0131 gezegen olarak da bilinen Sat\u00fcrn\u2019\u00fcn \u00f6zellikleri \u015fu \u015fekilde:<\/p>

                      • Ekvator \u00c7ap\u0131:<\/strong> 120.536 km<\/li>\n\n
                      • Kutup \u00c7ap\u0131:<\/strong> 108.728 km<\/li>\n\n
                      • Ekvator \u00c7evresi:<\/strong> 365.882 km<\/li>\n\n
                      • Y\u00f6r\u00fcnge Periyodu:<\/strong> 10.755 D\u00fcnya g\u00fcn\u00fc<\/li>\n\n
                      • Y\u00fczey S\u0131cakl\u0131\u011f\u0131:<\/strong> -139 \u00b0C<\/li>\n\n
                      • Uydu:<\/strong> En az 62 adet, en \u00f6nemlileri Titan, Rhea ve Enceladus.<\/li><\/ul>

                        Sat\u00fcrn hakk\u0131nda ilgin\u00e7 bilgiler:<\/strong><\/h3>
                        • Halkas\u0131 olan gezegenler aras\u0131nda en me\u015fhuru olan Sat\u00fcrn, eski uygarl\u0131klar\u0131n ke\u015ffetti\u011fi son gezegen. Babillerin ve Uzakdo\u011fulu astronomlar\u0131n Sat\u00fcrn\u2019\u00fc bildi\u011fine inan\u0131l\u0131yor.<\/li>\n\n
                        • Sat\u00fcrn\u2019\u00fcn etraf\u0131nda bulunan ve yakla\u015f\u0131k 20 metre kal\u0131nd\u0131\u011f\u0131na sahip halkalar\u0131n b\u00fcy\u00fck b\u00f6l\u00fcm\u00fc buz par\u00e7alar\u0131 ve karbonlu tozlardan olu\u015fuyor.<\/li>\n\n
                        • G\u00fcne\u015f sistemindeki di\u011fer gezegenlere k\u0131yasla Sat\u00fcrn\u2019deki r\u00fczgarlar ola\u011fan\u00fcst\u00fc h\u0131zlara ula\u015f\u0131yor. Saatte yakla\u015f\u0131k 1800 km h\u0131zla seyreden r\u00fczgarlara rastlamak m\u00fcmk\u00fcn.<\/li>\n\n
                        • Yo\u011funlu\u011fu en d\u00fc\u015f\u00fck gezegen olarak bilinen Sat\u00fcrn\u2019\u00fcn b\u00fcy\u00fck b\u00f6l\u00fcm\u00fcn\u00fc hidrojen gazlar\u0131 olu\u015fturuyor. Bu gezegenin helyum ve hidrojen gazlar\u0131ndan olu\u015fan par\u00e7alar\u0131 derinlerde yo\u011funla\u015farak metalik bir i\u00e7 \u00e7ekirdek meydana getiriyor.<\/li>\n\n
                        • Ekvator ve kutup \u00e7aplar\u0131 aras\u0131nda en fazla mesafeye sahip gezegen olan Sat\u00fcrn, d\u00fc\u015f\u00fck yo\u011funlu\u011fu ve y\u00fcksek h\u0131z\u0131 nedeniyle g\u00fcne\u015f sistemindeki en d\u00fcz gezegen olarak biliniyor.<\/li>\n\n
                        • Sat\u00fcrn kendi etraf\u0131ndaki d\u00f6n\u00fc\u015f\u00fcn\u00fc yakla\u015f\u0131k 10,5 saatte tamaml\u0131yor.<\/li>\n\n
                        • Hubble Uzay Teleskobu verilerine g\u00f6re Sat\u00fcrn\u2019\u00fcn atmosferindeki beyaz lekeler t\u0131pk\u0131 J\u00fcpiter\u2019deki k\u0131rm\u0131z\u0131 nokta gibi devasa f\u0131rt\u0131nalardan olu\u015fuyor. <\/li>\n\n
                        • Sat\u00fcrn\u2019e ula\u015fan ilk uzay arac\u0131 1979 y\u0131l\u0131nda gezegene yaln\u0131zca 22.000 kilometre yakla\u015fabilen Pioneer 11. <\/li><\/ul>
                          \"\"<\/figure>

                          Uran\u00fcs<\/strong><\/h2>

                          G\u00fcne\u015f\u2019ten uzakla\u015ft\u0131k\u00e7a i\u015fler daha da bilinmez hale geliyor. Buz devlerinden biri olan Uran\u00fcs, yedinci gezegen olarak ad\u0131n\u0131 Roma tanr\u0131s\u0131 Sat\u00fcrn\u2019\u00fcn babas\u0131ndan al\u0131yor. Peki hen\u00fcz 1781 y\u0131l\u0131nda ke\u015ffedilen Uran\u00fcs\u2019\u00fc ilgi \u00e7ekici k\u0131lan \u00f6zellikler neler?<\/p>

                          • Ekvator \u00c7ap\u0131:<\/strong> 51.118 km<\/li>\n\n
                          • Kutup \u00c7ap\u0131:<\/strong> 49.946 km<\/li>\n\n
                          • Ekvator \u00c7evresi:<\/strong> 159.354 km<\/li>\n\n
                          • Y\u00f6r\u00fcnge Periyodu:<\/strong> 30.687 D\u00fcnya g\u00fcn\u00fc<\/li>\n\n
                          • Y\u00fczey S\u0131cakl\u0131\u011f\u0131:<\/strong> -197 \u00b0C<\/li>\n\n
                          • Uydu:<\/strong> En az 27 adet, en \u00f6nemlileri Oberon, Titania, Miranda, Ariel ve Umbriel.<\/li><\/ul>

                            Uran\u00fcs hakk\u0131nda ilgin\u00e7 bilgiler:<\/strong><\/h3>
                            • Modern bilimin ke\u015ffetti\u011fi ilk gezegen olma ayr\u0131cal\u0131\u011f\u0131n\u0131 ta\u015f\u0131yan Uran\u00fcs, 1781 y\u0131l\u0131nda Alman astronom William Herschel taraf\u0131ndan ke\u015ffediliyor.<\/li>\n\n
                            • Ven\u00fcs gibi Uran\u00fcs de di\u011fer gezegenlerin tersi y\u00f6n\u00fcnde d\u00f6n\u00fcyor. Uran\u00fcs\u2019\u00fcn kendi ekseni etraf\u0131ndaki d\u00f6n\u00fc\u015f\u00fc ise 17 saat 14 dakikada tamamlan\u0131yor.<\/li>\n\n
                            • G\u00fcne\u015fin etraf\u0131ndaki yolculu\u011fu \u00e7ok uzun ge\u00e7en Uran\u00fcs, D\u00fcnya\u2019ya g\u00f6re 42 y\u0131l \u0131\u015f\u0131k al\u0131rken 42 y\u0131l karanl\u0131kta kal\u0131yor.<\/li>\n\n
                            • G\u00fcne\u015f sistemindeki d\u00f6rt d\u0131\u015f gezegenden en hafifi olan Uran\u00fcs, D\u00fcnya\u2019n\u0131n 14.5 kat\u0131 k\u00fctleye sahip.<\/li>\n\n
                            • Buzul gezegen olarak da bilinen Uran\u00fcs\u2019\u00fcn kendine has soluk mavi rengi onu di\u011ferlerinden ay\u0131r\u0131yor. Gezegenin minimum y\u00fczey s\u0131cakl\u0131\u011f\u0131 ise -224 \u00b0C.<\/li>\n\n
                            • Uran\u00fcs\u2019e d\u00fczenlenmi\u015f yaln\u0131zca tek bir uzay gezisi bulunuyor. 1986 y\u0131l\u0131nda g\u00f6nderilen Voyager 2 uzay arac\u0131 gezegene yaln\u0131zca 81.500 km yakla\u015fabildi. <\/li>\n\n
                            • Halkas\u0131 olan gezegenlerden biri olan Uran\u00fcs\u2019\u00fcn bilinen 13 adet halkas\u0131 var. <\/li>\n\n
                            • Uranyum elementi ad\u0131n\u0131 bu gezegenden al\u0131yor.<\/li><\/ul>
                              \"\"<\/figure>

                              Nept\u00fcn<\/strong><\/h2>

                              G\u00fcne\u015f sistemindeki gezegenler s\u0131ralamas\u0131<\/strong> Nept\u00fcn\u2019le son buluyor. Pl\u00fcton\u2019un 2006 y\u0131l\u0131nda c\u00fcce gezegenler<\/strong> s\u0131n\u0131f\u0131na dahil edilmesiyle son gezegen unvan\u0131na kavu\u015fan Nept\u00fcn kendine \u00f6zg\u00fc mavi rengiyle biliniyor. Bu sebeple ad\u0131 Roma mitolojisindeki deniz tanr\u0131s\u0131ndan geliyor. <\/p>

                              • Ekvator \u00c7ap\u0131:<\/strong> 49.528 km<\/li>\n\n
                              • Kutup \u00c7ap\u0131:<\/strong> 48.682 km<\/li>\n\n
                              • Ekvator \u00c7evresi:<\/strong> 155.600 km<\/li>\n\n
                              • Y\u00f6r\u00fcnge Periyodu:<\/strong> 60.190 D\u00fcnya g\u00fcn\u00fc<\/li>\n\n
                              • Y\u00fczey S\u0131cakl\u0131\u011f\u0131:<\/strong> -201 \u00b0C<\/li>\n\n
                              • Uydu:<\/strong> En az 14 adet, en \u00f6nemlisi Triton<\/li><\/ul>

                                Nept\u00fcn hakk\u0131nda ilgin\u00e7 bilgiler:<\/strong><\/h3>
                                • \u00c7\u0131plak g\u00f6zle g\u00f6r\u00fclmesi m\u00fcmk\u00fcn olmayan Nept\u00fcn, d\u0131\u015f gezegenler olarak bilinen d\u00f6rt gezegenden sonuncusunu temsil ediyor.<\/li>\n\n
                                • J\u00fcpiter\u2019in ard\u0131ndan en b\u00fcy\u00fck ikinci yer \u00e7ekimine sahip gezegenin ke\u015ffi ise 1846 y\u0131l\u0131nda ger\u00e7ekle\u015fiyor. Nept\u00fcn\u2019\u00fcn en b\u00fcy\u00fck uydusu olan Triton ise bundan yaln\u0131zca 17 g\u00fcn sonra ke\u015ffedildi.<\/li>\n\n
                                • Gazlardan olu\u015ftu\u011fu i\u00e7in kendi etraf\u0131nda inan\u0131lmaz h\u0131zl\u0131 bir \u015fekilde d\u00f6nen Nept\u00fcn bir tam turu 18 saatte tamaml\u0131yor.<\/li>\n\n
                                • \u00dcst katmanlar\u0131nda devasa hava hareketleri meydana gelen Nept\u00fcn\u2019de J\u00fcpiter\u2019dekine benzer bir kas\u0131rga bulunuyor ve bu yakla\u015f\u0131k olarak D\u00fcnya b\u00fcy\u00fckl\u00fc\u011f\u00fcnde.<\/li>\n\n
                                • D\u00fcnya\u2019dan yakla\u015f\u0131k 17 kat daha b\u00fcy\u00fck olan gezegenin \u00e7ekirde\u011fi ise kayalardan olu\u015fuyor.<\/li>\n\n
                                • Halkas\u0131 olan gezegenlerden biri olmas\u0131na ra\u011fmen Nept\u00fcn\u2019\u00fcn halkalar\u0131 fark edilemeyecek kadar soluk buz par\u00e7alar\u0131 ve toz tanelerinden olu\u015fuyor.<\/li><\/ul>
                                  \"\"<\/figure>

                                  Bir Zamanlar\u0131n Gezegeni Art\u0131k C\u00fcce: Pl\u00fcton<\/strong><\/h2>

                                  Ke\u015ffedildi\u011fi 1930 y\u0131l\u0131ndan 2006 y\u0131l\u0131ndaki tart\u0131\u015fmal\u0131 Prag Uluslararas\u0131 Astronomi Birli\u011fi toplant\u0131s\u0131na kadar gezegen kabul edilen Pl\u00fcton, art\u0131k bir c\u00fcce gezegen. D\u00fcnya\u2019n\u0131n uydusu Ay\u2019dan daha k\u00fc\u00e7\u00fck olan bu c\u00fcce gezegen kaotik bir y\u00f6r\u00fcngede ilerliyor. Bir\u00e7ok y\u00f6nden gizemini koruyan Pl\u00fcton\u2019un buzul mantolar\u0131 ve donmu\u015f nitrojenle \u00e7evrelenmi\u015f kat\u0131 bir kayal\u0131k \u00e7ekirde\u011fe sahip oldu\u011fu d\u00fc\u015f\u00fcn\u00fcl\u00fcyor.<\/p>

                                  • \u00c7ap\u0131:<\/strong> 2.368 km<\/li>\n\n
                                  • Y\u00f6r\u00fcnge Periyodu:<\/strong> 248 D\u00fcnya y\u0131l\u0131 <\/li>\n\n
                                  • Y\u00fczey S\u0131cakl\u0131\u011f\u0131:<\/strong> -229 \u00b0C<\/li>\n\n
                                  • Uydu:<\/strong> En az 5 adet<\/li><\/ul>

                                    G\u00fcne\u015f sistemindeki c\u00fcce gezegenler<\/strong> \u015fu \u015fekilde:<\/p>

                                    • Ceres<\/li>\n\n
                                    • Pl\u00fcton<\/li>\n\n
                                    • Haumea<\/li>\n\n
                                    • Makemake<\/li>\n\n
                                    • Eris<\/li><\/ul>

                                      Uzay ara\u015ft\u0131rmalar\u0131, gezegen yolculuklar\u0131 ve Mars kolonileri derken astronomi d\u00fcnyas\u0131nda ke\u015fiflerin ard\u0131 arkas\u0131 gelmiyor. Ba\u015fka bir gezegende ya\u015fama fikri kula\u011fa olduk\u00e7a heyecan verici gelse de g\u00fcne\u015f sisteminin ya\u015fanabilir tek gezegeni D\u00fcnya\u2019n\u0131n gelece\u011fine s\u0131k\u0131 s\u0131k\u0131ya sar\u0131lmak gerekiyor.<\/p>\n\n

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                                      \n Oylama Yap<\/span>\n <\/div>\n <\/div>\n","protected":false},"excerpt":{"rendered":"

                                      S\u00fcrekli geni\u015fleyen evrenin h\u0131z\u0131na eri\u015fmek m\u00fcmk\u00fcn de\u011fil. Uzay ke\u015fifleri heyecan verici seyahatlerle devam etse de evrenin s\u0131rr\u0131na vak\u0131f olmak suya…<\/p>\n","protected":false},"author":990005,"featured_media":4890,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1108],"tags":[1117,1115,461,127,1114,1119,1116,1118],"class_list":["post-4879","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-ilginc-bilgiler","tag-dunya","tag-ekvator","tag-extreme-outdoor","tag-extreme-outdoor-blog","tag-gunes-sistemindeki-gezegenler","tag-kuresel-isinma","tag-merkur","tag-uydu"],"_links":{"self":[{"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/posts\/4879","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/users\/990005"}],"replies":[{"embeddable":true,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/comments?post=4879"}],"version-history":[{"count":2,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/posts\/4879\/revisions"}],"predecessor-version":[{"id":4892,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/posts\/4879\/revisions\/4892"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/media\/4890"}],"wp:attachment":[{"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/media?parent=4879"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/categories?post=4879"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/tags?post=4879"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}