\n
\n\t\u0130talya Ulusal Astrofizik Enstit\u00fcs\u00fc\u2019nden Eloisa Poggio liderli\u011findeki ekip, Samanyolu\u2019nun d\u0131\u015f diskinde yer alan yakla\u015f\u0131k 17 bin gen\u00e7 dev y\u0131ld\u0131z ve 3 bin 400 de\u011fi\u015fken (Cepheid) y\u0131ld\u0131z\u0131n hareketlerini inceledi. Bulgular, y\u0131ld\u0131zlar\u0131n yukar\u0131-a\u015fa\u011f\u0131 y\u00f6nl\u00fc h\u0131zlar\u0131nda d\u00fczenli bir \u201cdalga hareketi\u201d oldu\u011funu g\u00f6sterdi.<\/p>\n
\n\tAra\u015ft\u0131rmac\u0131lara g\u00f6re bu dalgalar, g\u00f6lde at\u0131lan bir ta\u015f\u0131n ard\u0131ndan su y\u00fczeyinde olu\u015fan halkalara benziyor. Dalgan\u0131n genli\u011fi, yani yukar\u0131 ve a\u015fa\u011f\u0131 y\u00f6nl\u00fc sal\u0131n\u0131m miktar\u0131, galaksi merkezinden uzakla\u015ft\u0131k\u00e7a art\u0131yor.<\/p>\n
\n\tSebebi ba\u015fka bir galaksiyle \u00e7arp\u0131\u015fma olabilir<\/h2>\n
\n\tBilim insanlar\u0131, bu kozmik dalgay\u0131 tetikleyen olay\u0131n kayna\u011f\u0131n\u0131 kesin olarak bilmiyor. Ancak en g\u00fc\u00e7l\u00fc ihtimallerden biri, Samanyolu\u2019nun h\u00e2len etkile\u015fimde oldu\u011fu Sagittarius c\u00fcce galaksisi.<\/p>\n
\n\tUzmanlara g\u00f6re bu k\u00fc\u00e7\u00fck galaksi, Samanyolu diskinin i\u00e7inden ge\u00e7mi\u015f olabilir; t\u0131pk\u0131 bir g\u00f6lete at\u0131lan ta\u015f gibi galaksi boyunca dalgalar olu\u015fturmu\u015f olabilir.<\/p>\n
\n\tGalaksi san\u0131landan \u00e7ok daha dinamik<\/h2>\n
\n\tGaia verileri, Samanyolu\u2019nun d\u00fcz ve sakin bir yap\u0131da olmad\u0131\u011f\u0131n\u0131, aksine e\u011frilmi\u015f ve dalgal\u0131 bir disk yap\u0131s\u0131na sahip oldu\u011funu bir kez daha do\u011frulad\u0131. Ara\u015ft\u0131rmac\u0131lar, \u201cElde edilen bulgular, galaksi merkezinden d\u0131\u015fa do\u011fru yay\u0131lan dikey bir dalga oldu\u011funu g\u00f6steriyor,\u201d ifadesini kulland\u0131.<\/p>\n
\n\tBu dalgan\u0131n, galaksinin gaz tabakas\u0131nda ba\u015flay\u0131p gen\u00e7 y\u0131ld\u0131zlara da aktar\u0131lm\u0131\u015f olabilece\u011fi d\u00fc\u015f\u00fcn\u00fcl\u00fcyor.<\/p>\n
\n\tYeni verilerle s\u0131r perdesi aralanabilir<\/h2>\n
\n\tBilim insanlar\u0131, 2026\u2019da yay\u0131mlanmas\u0131 planlanan Gaia\u2019n\u0131n d\u00f6rd\u00fcnc\u00fc veri setiyle (DR4) bu dalgan\u0131n kayna\u011f\u0131n\u0131 daha net incelemeyi hedefliyor.<\/p>\n
\n\tPoggio, \u201cBu dalgan\u0131n Sagittarius galaksisiyle mi, yoksa daha k\u00fc\u00e7\u00fck yap\u0131larla m\u0131 ba\u011flant\u0131l\u0131 oldu\u011funu anlamak i\u00e7in \u00e7ok daha geni\u015f veriye ihtiyac\u0131m\u0131z var,\u201d dedi.<\/p>\n
\n\tYeni bulgular, Astronomy & Astrophysics dergisinde yay\u0131mland\u0131 ve Samanyolu\u2019nun h\u00e2l\u00e2 dinamik, ya\u015fayan bir galaksi oldu\u011funu bir kez daha kan\u0131tlad\u0131.<\/p>\n<\/p><\/div>\n","protected":false},"excerpt":{"rendered":"
\u0130talya Ulusal Astrofizik Enstit\u00fcs\u00fc\u2019nden Eloisa Poggio liderli\u011findeki ekip, Samanyolu\u2019nun d\u0131\u015f diskinde yer alan yakla\u015f\u0131k 17 bin gen\u00e7 dev y\u0131ld\u0131z ve 3 bin 400 de\u011fi\u015fken (Cepheid) y\u0131ld\u0131z\u0131n hareketlerini inceledi. Bulgular, y\u0131ld\u0131zlar\u0131n yukar\u0131-a\u015fa\u011f\u0131 y\u00f6nl\u00fc h\u0131zlar\u0131nda d\u00fczenli bir \u201cdalga hareketi\u201d oldu\u011funu g\u00f6sterdi.
Ara\u015ft\u0131rmac\u0131lara g\u00f6re bu dalgalar, g\u00f6lde at\u0131lan bir ta\u015f\u0131n ard\u0131ndan su y\u00fczeyinde olu\u015fan halkalara benziyor. […]<\/p>\n","protected":false},"author":1,"featured_media":31354,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"jnews-multi-image_gallery":[],"jnews_single_post":[],"jnews_primary_category":[],"footnotes":""},"categories":[2],"tags":[],"class_list":["post-31353","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-dunya"],"yoast_head":"\n
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\u0130talya Ulusal Astrofizik Enstit\u00fcs\u00fc\u2019nden Eloisa Poggio liderli\u011findeki ekip, Samanyolu\u2019nun d\u0131\u015f diskinde yer alan yakla\u015f\u0131k 17 bin gen\u00e7 dev y\u0131ld\u0131z ve 3 bin 400 de\u011fi\u015fken (Cepheid) y\u0131ld\u0131z\u0131n hareketlerini inceledi. Bulgular, y\u0131ld\u0131zlar\u0131n yukar\u0131-a\u015fa\u011f\u0131 y\u00f6nl\u00fc h\u0131zlar\u0131nda d\u00fczenli bir \u201cdalga hareketi\u201d oldu\u011funu g\u00f6sterdi.
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\u0130talya Ulusal Astrofizik Enstit\u00fcs\u00fc\u2019nden Eloisa Poggio liderli\u011findeki ekip, Samanyolu\u2019nun d\u0131\u015f diskinde yer alan yakla\u015f\u0131k 17 bin gen\u00e7 dev y\u0131ld\u0131z ve 3 bin 400 de\u011fi\u015fken (Cepheid) y\u0131ld\u0131z\u0131n hareketlerini inceledi. Bulgular, y\u0131ld\u0131zlar\u0131n yukar\u0131-a\u015fa\u011f\u0131 y\u00f6nl\u00fc h\u0131zlar\u0131nda d\u00fczenli bir \u201cdalga hareketi\u201d oldu\u011funu g\u00f6sterdi.
Ara\u015ft\u0131rmac\u0131lara g\u00f6re bu dalgalar, g\u00f6lde at\u0131lan bir ta\u015f\u0131n ard\u0131ndan su y\u00fczeyinde olu\u015fan halkalara benziyor. 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