[vc_row][vc_column][vc_column_text]<\/p>\n
G\u00fcne\u015f sisteminin en b\u00fcy\u00fck gezegeni olan J\u00fcpiter\u2019in bilinen 79 uydusu bulunuyor. En b\u00fcy\u00fck uydusu Ganymede sadece J\u00fcpiter\u2019in de\u011fil, ayn\u0131 zamanda G\u00fcne\u015f sisteminin de bilinen en b\u00fcy\u00fck uydusu. Bu uydu e\u011fer J\u00fcpiter\u2019in de\u011fil de G\u00fcne\u015f\u2019in etraf\u0131nda d\u00f6nseydi, boyutlar\u0131ndan dolay\u0131 rahatl\u0131kla bir gezegen olarak kabul edilebilirdi. 1610\u2019da \u0130talyan g\u00f6k bilimci Galileo Galilei taraf\u0131ndan J\u00fcpiter\u2019in di\u011fer \u00fc\u00e7 b\u00fcy\u00fck uydusuyla birlikte ke\u015ffedilen bu dev uydu hakk\u0131nda ilgin\u00e7 bilgileri yaz\u0131m\u0131zda listeledik.<\/p>\n
[\/vc_column_text][\/vc_column][\/vc_row][vc_row el_class=”innerItemContainer”][vc_column][eltd_section_title alignment=”left” title=”1#” title_font_size=”13″][vc_single_image image=”28307″ img_size=”full” el_class=”innerImageContainer”][vc_column_text el_class=”innerText”]<\/p>\n
Ganymede d\u00e2hil olmak \u00fczere Io, Europa ve Callisto, J\u00fcpiter’in en b\u00fcy\u00fck d\u00f6rt uydusudur ve bu uydular \u201cGalileo Uydular\u0131\u201d olarak adland\u0131r\u0131l\u0131r.<\/p>\n
[\/vc_column_text][\/vc_column][\/vc_row][vc_row el_class=”innerItemContainer”][vc_column][eltd_section_title alignment=”left” title=”2#” title_font_size=”13″][vc_single_image image=”28308″ img_size=”full” el_class=”innerImageContainer”][vc_column_text el_class=”innerText”]<\/p>\n
5.262 km\u2019lik \u00e7apa sahip Ganymede\u2019nin y\u00fczey alan\u0131 4.879 km \u00e7apa sahip Merk\u00fcr gezegeninden daha b\u00fcy\u00fckt\u00fcr ve bu do\u011fal uydu k\u00fc\u00e7\u00fck bir teleskop ya da d\u00fcrb\u00fcnle bile \u00e7ok rahat g\u00f6zlemlenebilir. Ganymede y\u00fczey \u00f6l\u00e7\u00fcs\u00fc bak\u0131m\u0131ndan Merk\u00fcr\u2019den b\u00fcy\u00fck olsa da iki g\u00f6k cismi k\u00fctlesel olarak k\u0131yasland\u0131\u011f\u0131nda Ganymede daha hafiftir. Bunun sebebi ise Ganymede\u2019nin b\u00fcy\u00fck oranda buzdan olu\u015fmas\u0131d\u0131r.<\/p>\n
[\/vc_column_text][\/vc_column][\/vc_row][vc_row el_class=”innerItemContainer”][vc_column][eltd_section_title alignment=”left” title=”3#” title_font_size=”13″][vc_single_image image=”28309″ img_size=”full” el_class=”innerImageContainer”][vc_column_text el_class=”innerText”]<\/p>\n
Ganymede\u2019nin y\u00fczeyi kal\u0131n bir buz tabakas\u0131ndan olu\u015fur ve jeolojik olarak pek de aktif bir yap\u0131ya sahip de\u011fildir. G\u00f6k bilimciler bu bilgiye ya\u015f\u0131 yakla\u015f\u0131k 4 milyar\u0131 a\u015fan kraterler sayesinde ula\u015fm\u0131\u015ft\u0131r. Ganymede\u2019nin y\u00fczeyinde \u00e7arpma izleri, kraterler ve oluklar bulunur. Kraterler y\u00fczeyin ya\u015f\u0131n\u0131 belirlemek ve G\u00fcne\u015f sistemindeki \u00e7e\u015fitli d\u00f6nemleri anlamak i\u00e7in kullan\u0131lan \u00f6nemli g\u00f6stergelerdir.<\/p>\n
[\/vc_column_text][\/vc_column][\/vc_row][vc_row el_class=”innerItemContainer”][vc_column][eltd_section_title alignment=”left” title=”4#” title_font_size=”13″][vc_single_image image=”28310″ img_size=”full” el_class=”innerImageContainer”][vc_column_text el_class=”innerText”]Ganymede, kendine ait manyetosfere sahip olan tek uydudur. Manyetosfer, G\u00fcne\u015f r\u00fczg\u00e2rlar\u0131yla olu\u015fan plazma ak\u0131m\u0131n\u0131n engellenmesini sa\u011flar ve y\u00fckl\u00fc par\u00e7ac\u0131klar\u0131n gezegenin veya g\u00f6k cisminin atmosferine \u00e7arpmas\u0131n\u0131 engelleyen bariyer g\u00f6revi g\u00f6r\u00fcr. Ganymede\u2019nin manyetosferi hem G\u00fcne\u015f\u2019ten hem de J\u00fcpiter\u2019den gelen y\u00fcksek enerjili par\u00e7ac\u0131k ak\u0131\u015f\u0131ndan kendini korur.[\/vc_column_text][\/vc_column][\/vc_row][vc_row el_class=”innerItemContainer”][vc_column][eltd_section_title alignment=”left” title=”5#” title_font_size=”13″][vc_single_image image=”28311″ img_size=”full” el_class=”innerImageContainer”][vc_column_text el_class=”innerText”]<\/p>\n
J\u00fcpiter\u2019e yak\u0131nl\u0131k a\u00e7\u0131s\u0131ndan ele al\u0131nd\u0131\u011f\u0131nda Ganymede; Io ve Europa\u2019dan sonra \u00fc\u00e7\u00fcnc\u00fc s\u0131rada yer al\u0131r. Yak\u0131n zamanda yer alt\u0131nda tuzlu su okyanuslar\u0131n\u0131n bulundu\u011funu \u00f6\u011frendi\u011fimiz Ganymede\u2019de y\u00fczey s\u0131cakl\u0131\u011f\u0131 olduk\u00e7a d\u00fc\u015f\u00fckt\u00fcr ve genellikle -150 \u00b0C civar\u0131ndad\u0131r. Ganymede, D\u00fcnya d\u0131\u015f\u0131nda ya\u015fam ihtimalinin ara\u015ft\u0131r\u0131ld\u0131\u011f\u0131 \u00f6nemli bir uydudur. 2024’te \u201cEuropa Clipper\u201d uzay arac\u0131, \u201cGalileo Uydular\u0131\u201dnda ya\u015fam\u0131n izlerini aramak i\u00e7in uzaya f\u0131rlat\u0131lacak ve bir aksilik \u00e7\u0131kmazsa bu uydular\u0131n en net foto\u011fraflar\u0131 \u00e7ekilecektir.<\/p>\n
[\/vc_column_text][\/vc_column][\/vc_row]<\/p>\n","protected":false},"excerpt":{"rendered":"
[vc_row][vc_column][vc_column_text] G\u00fcne\u015f sisteminin en b\u00fcy\u00fck gezegeni olan J\u00fcpiter\u2019in bilinen 79 uydusu bulunuyor. En b\u00fcy\u00fck uydusu Ganymede sadece J\u00fcpiter\u2019in de\u011fil, ayn\u0131 zamanda G\u00fcne\u015f sisteminin de bilinen en b\u00fcy\u00fck uydusu. Bu uydu e\u011fer J\u00fcpiter\u2019in de\u011fil de G\u00fcne\u015f\u2019in etraf\u0131nda d\u00f6nseydi, boyutlar\u0131ndan dolay\u0131 rahatl\u0131kla bir gezegen olarak kabul edilebilirdi. 1610\u2019da \u0130talyan g\u00f6k bilimci Galileo Galilei taraf\u0131ndan J\u00fcpiter\u2019in di\u011fer \u00fc\u00e7 […]<\/p>\n","protected":false},"author":1,"featured_media":28306,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[10],"tags":[2242,2243,2244,2245],"class_list":["post-28303","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-yasam","tag-galileo-galilei","tag-ganymede","tag-jupiter","tag-uydu"],"_links":{"self":[{"href":"https:\/\/soms.invekor.net\/index.php?rest_route=\/wp\/v2\/posts\/28303","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/soms.invekor.net\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/soms.invekor.net\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/soms.invekor.net\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/soms.invekor.net\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=28303"}],"version-history":[{"count":0,"href":"https:\/\/soms.invekor.net\/index.php?rest_route=\/wp\/v2\/posts\/28303\/revisions"}],"wp:attachment":[{"href":"https:\/\/soms.invekor.net\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=28303"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/soms.invekor.net\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=28303"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/soms.invekor.net\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=28303"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}