Herhangi bir maddenin yans\u0131yan g\u00f6r\u00fcnt\u00fcs\u00fcne Anti madde denir. Ancak ili\u015fki halinde kar\u015f\u0131l\u0131kl\u0131 tahribat s\u00f6zkonusudur. Bir antihidrojen atomu \u00e7ekirdek olarak bir anti-proton ve etraf\u0131nda d\u00f6nen bir positrona (pozitif elektron) sahiptir. Daha b\u00fcy\u00fck anti madde atomlar\u0131n\u0131n olu\u015fmas\u0131 anti-n\u00f6tronlar\u0131n olu\u015fmas\u0131n\u0131 gerektirir. Bu anti maddeler y\u00fcksek enerji madde h\u0131zland\u0131r\u0131c\u0131lar\u0131nda olu\u015fturulmu\u015ftur. Ancak antimaddenin evrende do\u011fal olarak olu\u015fmad\u0131\u011f\u0131 ortaya \u00e7\u0131km\u0131\u015ft\u0131r. Y\u00f6r\u00fcngedeki g\u00f6zlemevleri ile ilgili planlar t\u00fcm elektromanyetik spektrumla ilgili seyahat bro\u015f\u00fcrleri gibidir. Sovyet uzay bilginleri, bir uzay radyo telek -topunu uzun s\u00fcredir incelemi\u015f ve ayr\u0131nt\u0131l\u0131 \u015femalar\u0131n\u0131 \u00e7\u0131karm\u0131\u015flard\u0131r. \u00c7ap\u0131nda 1 km ve 10 km. aras\u0131 bir d\u00fczenleme ve milimetre ve desimetrelere uzanan ay\u0131nc\u0131 g\u00fcce sahip olan bu Sovyet arac\u0131 100.000 \u0131\u015f\u0131k y\u0131l\u0131 uzakl\u0131ktaki g\u00fcne\u015fe benzer y\u0131ld\u0131zlar\u0131n radyo dalgalar\u0131n\u0131 saptayabilmektedir. \u00c7al\u0131\u015fma \u00f6l\u00e7e\u011fi (interferometry) teknikleri * ile b\u00f6yle iki ayr\u0131 uzay \u00fcss\u00fcnden t\u00fcm evreni taramak m\u00fcmk\u00fcn olabilmektedir. Bu giri\u015fim ayn\u0131 zamanda Sovyet SET\u0130 (D\u00fcnya D\u0131\u015f\u0131 Bilgi Ara\u015ft\u0131rmalar\u0131) projesinde de i\u015fe yarayacakt\u0131r.<\/p>\n
Spektrumun k\u0131z\u0131l\u00f6tesi b\u00f6l\u00fcm\u00fc, 1981\u2019de k\u0131z\u0131l\u00f6tesi Astronomi Uydu-su\u2019nun (IRAS) f\u0131rlat\u0131lmas\u0131 ile ele al\u0131nacakt\u0131r. NASA-Ingiltere-Hollanda\u2019-n\u0131n birlikte y\u00fcr\u00fctece\u011fi bir ara\u015ft\u0131rmada kutup y\u00f6r\u00fcngeli 3 kelvine (-270C) kadar so\u011futulmu\u015f 700 kg\u2019l\u0131k bir teleskopla evrenin b\u00fcy\u00fck patlamas\u0131ndan geriye kalan k\u0131z\u0131l\u00f6tesi ve kozmik (-243 C) radyasyon t\u00fcm g\u00f6ky\u00fcz\u00fcnde ara\u015ft\u0131r\u0131lacak. NASA taraf\u0131ndan ayr\u0131ca bir de ek olarak kozmik Saha Ara\u015ft\u0131r\u0131c\u0131s\u0131 (COBE) \u00f6nerilmi\u015ftir.<\/p>\n
Gelecek on y\u0131lda yap\u0131lacak ara\u015ft\u0131rmalardan en \u00f6nemlisi NESA-ESA uzay teleskopunun 1983\u2019te y\u00f6r\u00fcngeye sokulmas\u0131d\u0131r. Bu merkezin can damar\u0131 2.4 m. \u00e7ap\u0131nda 27. kademe y\u0131ld\u0131zlar\u0131n\u0131 bile g\u00f6zleyebilecek yetenekte bir ayna olacakt\u0131r. Bu teleskop 508 cm.\u2019lik Mount Palomer teleskopunun g\u00f6rd\u00fc\u011f\u00fc y\u0131ld\u0131zlardan 50 kez daha silik y\u0131ld\u0131zlar\u0131 g\u00f6rebilme yetene\u011finde-dir. Amerikan Uzay Shuttle\u2019i taraf\u0131ndan f\u0131rlat\u0131lacak olan d\u00fczenek, 1-2 y\u0131l da bir y\u00f6r\u00fcngede bak\u0131m gerektirecek d\u00f6rt ila yedi y\u0131lda bir de d\u00fcnyada aynan\u0131n tekrar s\u0131rlanmas\u0131 gerekecektir. Ana aynaya ek olarak pek \u00e7ok ba\u015fka ara\u00e7 telesktopun \u00e7evresinde y\u00f6r\u00fcngeye sokulacakt\u0131r. Bunlar\u0131n aras\u0131nda bir geni\u015f a\u00e7\u0131 foto\u011fraf makinesi bir uzak nesneler i\u00e7in foto\u011fraf makinesi gezegenlerle ilgili bir makine, bir uzak nesneler i\u00e7in y\u00fcksek ay\u0131r\u0131c\u0131 g\u00fc\u00e7l\u00fc sepk-trograf ve bir IR fotometre bulunmaktad\u0131r.<\/p>\n
ESA\u2019n\u0131n yapt\u0131\u011f\u0131 EXOSAT uydusunun 1981\/1982 y\u0131llar\u0131nda f\u0131rlat\u0131lmas\u0131 porgramlanm\u0131\u015ft\u0131r. Bu uydunun 1979\u2019da f\u0131rlat\u0131lan HEOA 3 ile ba\u011flant\u0131l\u0131 olarak ay taraf\u0131ndan perdelenen X-\u0131\u015f\u0131m kaynaklar\u0131n\u0131 ara\u015ft\u0131rmas\u0131 planlanmaktad\u0131r. Bu uydular\u0131n ana hedefleri, muhtemel n\u00f6tron y\u0131ld\u0131zlar\u0131, pul-sarlar, kara deliklerdir. 1980\u2019lerin ortalar\u0131 i\u00e7in \u00f6nerilmi\u015f bulunan bir geli\u015ftirilmi\u015f X-\u0131\u015f\u0131n\u0131 Astrofizik Arac\u0131 (AXAF) da bu ara\u015ft\u0131rmalar\u0131 geni\u015fleterek, y\u0131ld\u0131z ve galaksi yap\u0131s\u0131n\u0131 ve evrimini ve de\u011fi\u015fik kozmolojik teorileri inceleyecektir. 1984\u2019te Shuttle ile f\u0131rlat\u0131lmas\u0131 i\u00e7in \u00f6nerilen Gama I\u015f\u0131n\u0131 G\u00f6zlemcisi (GRO) ise galaksi ile ilgili ve galaksi d\u0131\u015f\u0131 kaynaklardan gelen gama \u0131\u015f\u0131n\u0131 yay\u0131lmalar\u0131n\u0131 ara\u015ft\u0131racakt\u0131r. Radyo galaksilerini, pulsar\u00edan, quasarlan, anti madde kaynaklar\u0131n\u0131 ilgilendiren bilginin yan\u0131 s\u0131ra daha \u00f6nce kaydedilmi\u015f bulunan gama-\u0131\u015f\u0131n\u0131 patlamalar\u0131 ve di\u011fer ge\u00e7ici olaylar ara\u015ft\u0131r\u0131lacakt\u0131r.<\/p>\n
Uzay u\u00e7u\u015flar\u0131n\u0131n son yirmi bir y\u0131l\u0131, insanl\u0131\u011fa daha \u00f6nce bilinmeyen bir evrenin kap\u0131s\u0131n\u0131 a\u00e7t\u0131. Batlamyus\u2019un teorileri Kopemik i\u00e7in ne kadar eskiyse Sputnik \u0130\u2019den \u00f6nceki teoriler de bilim adamlar\u0131na o kadar eski gelmektedir. Gelecekteki ara\u015ft\u0131rmalar bizi arad\u0131\u011f\u0131m\u0131z ger\u00e7eklerin daha yak\u0131n\u0131na getirecektir.<\/p>\n","protected":false},"excerpt":{"rendered":"
Herhangi bir maddenin yans\u0131yan g\u00f6r\u00fcnt\u00fcs\u00fcne Anti madde denir. Ancak ili\u015fki halinde kar\u015f\u0131l\u0131kl\u0131 tahribat s\u00f6zkonusudur. Bir antihidrojen atomu \u00e7ekirdek olarak bir anti-proton ve etraf\u0131nda d\u00f6nen bir positrona (pozitif elektron) sahiptir. Daha…<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[92],"tags":[],"class_list":["post-8111","post","type-post","status-publish","format-standard","hentry","category-bilim"],"_links":{"self":[{"href":"https:\/\/www.ilkkimbuldu.com\/index.php?rest_route=\/wp\/v2\/posts\/8111"}],"collection":[{"href":"https:\/\/www.ilkkimbuldu.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.ilkkimbuldu.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.ilkkimbuldu.com\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.ilkkimbuldu.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=8111"}],"version-history":[{"count":1,"href":"https:\/\/www.ilkkimbuldu.com\/index.php?rest_route=\/wp\/v2\/posts\/8111\/revisions"}],"predecessor-version":[{"id":8112,"href":"https:\/\/www.ilkkimbuldu.com\/index.php?rest_route=\/wp\/v2\/posts\/8111\/revisions\/8112"}],"wp:attachment":[{"href":"https:\/\/www.ilkkimbuldu.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=8111"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.ilkkimbuldu.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=8111"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.ilkkimbuldu.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=8111"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}