Ven\u00fcs D\u00fcnya’dan bak\u0131ld\u0131\u011f\u0131nda beyaz bir gezegen gibi g\u00f6r\u00fcn\u00fcr. Bunun nedeni gezegenin yo\u011fun atmosferidir ve bu atmosfer D\u00fcnya’daki atmosferden \u00e7ok daha kal\u0131nd\u0131r. Ger\u00e7ekten o kadar yo\u011fundur ki, insanlar taraf\u0131ndan solunursa zehirlidir. Ancak kal\u0131n, beyaz bulutlar\u0131n alt\u0131ndaki Ven\u00fcs asl\u0131nda k\u0131rm\u0131z\u0131d\u0131r! Bu k\u0131rm\u0131z\u0131 renge Ven\u00fcs’te akan lavlar\u0131n dolamba\u00e7l\u0131 yollar\u0131 neden olur.<\/p>\n
![\"Ven\u00fcs](\"https:\/\/osr.org\/wp-content\/uploads\/2021\/02\/TR-Venus.jpg\" "\\"TR-Ven\u00fcs\\"")
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Samanyolumuzda Ven\u00fcs<\/span><\/h2>\nG\u00fcne\u015f’ten bak\u0131ld\u0131\u011f\u0131nda, Ven\u00fcs gezegeni g\u00fcne\u015f sistemimizdeki ikinci gezegendir. D\u00fcnya’dan bak\u0131ld\u0131\u011f\u0131nda, Ven\u00fcs, G\u00fcne\u015f ve Ay’dan sonra g\u00f6ky\u00fcz\u00fcndeki en parlak nesnedir. Ven\u00fcs’e “Ay’\u0131n k\u0131z karde\u015fi” de denir, \u00e7\u00fcnk\u00fc Ay gibi o da G\u00fcne\u015f’ten bir miktar \u0131\u015f\u0131k ve \u0131s\u0131 al\u0131r. Ayr\u0131ca, gece g\u00f6ky\u00fcz\u00fcnde g\u00f6r\u00fclebilen en parlak gezegendir. Buna ek olarak, Ven\u00fcs g\u00fcne\u015f sistemimizdeki en s\u0131cak gezegendir. Ven\u00fcs’te g\u00fcnd\u00fcz ve gece s\u0131cakl\u0131k neredeyse 500 \u00b0C’dir!<\/p>\n
Ven\u00fcs’\u00fcn di\u011fer astronomik cisimlerle kar\u015f\u0131la\u015ft\u0131r\u0131lmas\u0131<\/span><\/h2>\nVen\u00fcs gezegeninin b\u00fcy\u00fckl\u00fc\u011f\u00fc, k\u00fctlesi ve ortalama yo\u011funlu\u011fu yakla\u015f\u0131k olarak D\u00fcnya’yla ayn\u0131d\u0131r. Ven\u00fcs ve D\u00fcnya yakla\u015f\u0131k olarak ayn\u0131 zamanda; 4,6 milyar y\u0131l \u00f6nce ayn\u0131 gaz ve toz bulutunun i\u00e7inde olu\u015ftu. Ayr\u0131ca her iki gezegen de da\u011flar, volkanlar ve \u00e7arpma kraterlerinden olu\u015fan \u00e7e\u015fitli y\u00fczey alanlar\u0131na sahiptir. Ven\u00fcs’e, “D\u00fcnya’n\u0131n ikiz karde\u015fi” bile denilmi\u015ftir.<\/p>\n
Di\u011fer bir\u00e7ok gezegenden farkl\u0131 olarak, Ven\u00fcs’\u00fcn uydusu yoktur. \u0130lk g\u00f6zlemciler gezegeni \u00e7evreleyen muhtemel bir uydu fark etmi\u015fti. Bu uyduya Neith ad\u0131 verilmi\u015fti. Bu g\u00f6zlemlerin daha sonra yanl\u0131\u015f oldu\u011fu tespit edildi. G\u00fcn\u00fcm\u00fczde Ven\u00fcs’\u00fcn bu s\u00f6zde uydusundan “Neith: Ven\u00fcs’\u00fcn kay\u0131p uydusu” olarak bahsedilmektedir.<\/p>\n
Ven\u00fcs gezegeninde ya\u015fam var m\u0131?<\/span><\/h2>\nVen\u00fcs, D\u00fcnya’m\u0131zla kar\u015f\u0131la\u015ft\u0131r\u0131ld\u0131\u011f\u0131nda bir\u00e7ok benzerli\u011fe sahiptir, bu nedenle 19. y\u00fczy\u0131lda Ven\u00fcs’teki ya\u015fam hakk\u0131nda bir\u00e7ok spek\u00fclasyon yap\u0131lm\u0131\u015ft\u0131r. 1870 ‘te \u0130ngiliz astronom Richard Proctor Ven\u00fcs’teki ya\u015fam olabilece\u011fini ileri s\u00fcrd\u00fc. \u0130sve\u00e7li fizik\u00e7i ve kimyager Svante Arrhenius ise 1918’de Ven\u00fcs’\u00fc nemli ve ye\u015fil bir gezegen olarak tan\u0131mlad\u0131. Ancak, 20. y\u00fczy\u0131ldan bu yana Ven\u00fcs’\u00fcn a\u015f\u0131r\u0131 bir iklime sahip oldu\u011fu a\u00e7\u0131k\u00e7a g\u00f6r\u00fclm\u00fc\u015ft\u00fcr. Ola\u011fan\u00fcst\u00fc y\u00fcksek s\u0131cakl\u0131\u011fa ve 90 barl\u0131k hava bas\u0131nc\u0131na sahip Ven\u00fcs’te ya\u015fam imk\u00e2ns\u0131z g\u00f6r\u00fcn\u00fcyor.<\/p>\n
Ven\u00fcs gezegeninin g\u00f6r\u00fcnt\u00fclenmesi<\/span><\/h2>\nVen\u00fcs, D\u00fcnya ve Merk\u00fcr aras\u0131ndaki y\u00f6r\u00fcngede yer almaktad\u0131r. Ven\u00fcs’\u00fcn Merk\u00fcr’e g\u00f6re G\u00fcne\u015f’ten \u00e7ok daha uzak oldu\u011funu g\u00f6z \u00f6n\u00fcnde bulundurursak, Ven\u00fcs’\u00fc genellikle D\u00fcnya’dan g\u00f6rebiliriz. G\u00fcne\u015f’e bu kadar yak\u0131n olmas\u0131 nedeniyle, Ven\u00fcs sadece g\u00fcn bat\u0131m\u0131ndan sonraki d\u00f6rt saatte veya g\u00fcn do\u011fumundan \u00f6nceki d\u00f6rt saatte g\u00f6r\u00fclebilir. Bu nedenle Ven\u00fcs’e “Sabah Y\u0131ld\u0131z\u0131” veya “Ak\u015fam Y\u0131ld\u0131z\u0131” ad\u0131 da verilmi\u015ftir! Bu ayn\u0131 zamanda Ven\u00fcs’\u00fcn g\u00fcnd\u00fcz ve gece g\u00f6r\u00fclemedi\u011fi anlam\u0131na gelir.<\/p>\n
Ven\u00fcs’\u00fc genellikle G\u00fcne\u015f’ten 48 dereceye kadar g\u00f6rebilirsiniz. Ven\u00fcs’\u00fcn g\u00f6r\u00fcn\u00fcr parlakl\u0131\u011f\u0131 -3,7 ile -4,6 aras\u0131nda de\u011fi\u015fir. \u015eans\u0131n\u0131z varsa ve do\u011fru yerde ve zamanda Ven\u00fcs’\u00fc \u00e7\u0131plak g\u00f6zle g\u00f6rebilirsiniz. Yine de, bir d\u00fcrb\u00fcn veya teleskop kullanman\u0131z\u0131 \u00f6neririz. B\u00f6ylece gezegenin t\u00fcm harika ayr\u0131nt\u0131lar\u0131n\u0131 g\u00f6rebilirsiniz. Bir y\u0131ld\u0131z g\u00f6zlemcisi olarak gece yapaca\u011f\u0131n\u0131z g\u00f6zlemlerie ilgili ipu\u00e7lar\u0131m\u0131za g\u00f6z at\u0131n.<\/a><\/p>\nVen\u00fcs s\u00fcrprizlerle dolu!<\/span><\/h2>\nBu blogda size a\u015fk\u0131n gezegeni olan Ven\u00fcs’\u00fc tan\u0131tt\u0131k. Ven\u00fcs’e neden “Sabah Y\u0131ld\u0131z\u0131” veya “Ak\u015fam Y\u0131ld\u0131z\u0131” ad\u0131 verildi\u011fini ve nas\u0131l g\u00f6r\u00fcnd\u00fc\u011f\u00fcn\u00fc art\u0131k biliyorsunuz. Buna ek olarak, Ven\u00fcs’\u00fcn G\u00fcne\u015f sisteminde nerede bulundu\u011funu ve bu beyaz gezegendeki ya\u015fam\u0131n neden imk\u00e2ns\u0131z oldu\u011funu \u00f6\u011frendiniz. Bu Sevgililer G\u00fcn\u00fc’ne Ven\u00fcs’e birlikte bak\u0131n, birbirinize ba\u011fland\u0131\u011f\u0131n\u0131z\u0131 hissedin ve sevdi\u011finiz ki\u015finin hayat\u0131n\u0131 ayd\u0131nlat\u0131n! OSR Star Finder uygulamas\u0131 ile G\u00fcne\u015f sistemimizde seyahat edin ve y\u0131ld\u0131zlar\u0131m\u0131z\u0131 ve gezegenlerimizi g\u00f6r\u00fcn!<\/p>\n
Ven\u00fcs gezegeninin b\u00fcy\u00fckl\u00fc\u011f\u00fc, k\u00fctlesi ve ortalama yo\u011funlu\u011fu yakla\u015f\u0131k olarak D\u00fcnya’yla ayn\u0131d\u0131r. Ven\u00fcs ve D\u00fcnya yakla\u015f\u0131k olarak ayn\u0131 zamanda; 4,6 milyar y\u0131l \u00f6nce ayn\u0131 gaz ve toz bulutunun i\u00e7inde olu\u015ftu. Ayr\u0131ca her iki gezegen de da\u011flar, volkanlar ve \u00e7arpma kraterlerinden olu\u015fan \u00e7e\u015fitli y\u00fczey alanlar\u0131na sahiptir. Ven\u00fcs’e, “D\u00fcnya’n\u0131n ikiz karde\u015fi” bile denilmi\u015ftir.<\/p>\n
Di\u011fer bir\u00e7ok gezegenden farkl\u0131 olarak, Ven\u00fcs’\u00fcn uydusu yoktur. \u0130lk g\u00f6zlemciler gezegeni \u00e7evreleyen muhtemel bir uydu fark etmi\u015fti. Bu uyduya Neith ad\u0131 verilmi\u015fti. Bu g\u00f6zlemlerin daha sonra yanl\u0131\u015f oldu\u011fu tespit edildi. G\u00fcn\u00fcm\u00fczde Ven\u00fcs’\u00fcn bu s\u00f6zde uydusundan “Neith: Ven\u00fcs’\u00fcn kay\u0131p uydusu” olarak bahsedilmektedir.<\/p>\n
Ven\u00fcs gezegeninde ya\u015fam var m\u0131?<\/span><\/h2>\nVen\u00fcs, D\u00fcnya’m\u0131zla kar\u015f\u0131la\u015ft\u0131r\u0131ld\u0131\u011f\u0131nda bir\u00e7ok benzerli\u011fe sahiptir, bu nedenle 19. y\u00fczy\u0131lda Ven\u00fcs’teki ya\u015fam hakk\u0131nda bir\u00e7ok spek\u00fclasyon yap\u0131lm\u0131\u015ft\u0131r. 1870 ‘te \u0130ngiliz astronom Richard Proctor Ven\u00fcs’teki ya\u015fam olabilece\u011fini ileri s\u00fcrd\u00fc. \u0130sve\u00e7li fizik\u00e7i ve kimyager Svante Arrhenius ise 1918’de Ven\u00fcs’\u00fc nemli ve ye\u015fil bir gezegen olarak tan\u0131mlad\u0131. Ancak, 20. y\u00fczy\u0131ldan bu yana Ven\u00fcs’\u00fcn a\u015f\u0131r\u0131 bir iklime sahip oldu\u011fu a\u00e7\u0131k\u00e7a g\u00f6r\u00fclm\u00fc\u015ft\u00fcr. Ola\u011fan\u00fcst\u00fc y\u00fcksek s\u0131cakl\u0131\u011fa ve 90 barl\u0131k hava bas\u0131nc\u0131na sahip Ven\u00fcs’te ya\u015fam imk\u00e2ns\u0131z g\u00f6r\u00fcn\u00fcyor.<\/p>\n
Ven\u00fcs gezegeninin g\u00f6r\u00fcnt\u00fclenmesi<\/span><\/h2>\nVen\u00fcs, D\u00fcnya ve Merk\u00fcr aras\u0131ndaki y\u00f6r\u00fcngede yer almaktad\u0131r. Ven\u00fcs’\u00fcn Merk\u00fcr’e g\u00f6re G\u00fcne\u015f’ten \u00e7ok daha uzak oldu\u011funu g\u00f6z \u00f6n\u00fcnde bulundurursak, Ven\u00fcs’\u00fc genellikle D\u00fcnya’dan g\u00f6rebiliriz. G\u00fcne\u015f’e bu kadar yak\u0131n olmas\u0131 nedeniyle, Ven\u00fcs sadece g\u00fcn bat\u0131m\u0131ndan sonraki d\u00f6rt saatte veya g\u00fcn do\u011fumundan \u00f6nceki d\u00f6rt saatte g\u00f6r\u00fclebilir. Bu nedenle Ven\u00fcs’e “Sabah Y\u0131ld\u0131z\u0131” veya “Ak\u015fam Y\u0131ld\u0131z\u0131” ad\u0131 da verilmi\u015ftir! Bu ayn\u0131 zamanda Ven\u00fcs’\u00fcn g\u00fcnd\u00fcz ve gece g\u00f6r\u00fclemedi\u011fi anlam\u0131na gelir.<\/p>\n
Ven\u00fcs’\u00fc genellikle G\u00fcne\u015f’ten 48 dereceye kadar g\u00f6rebilirsiniz. Ven\u00fcs’\u00fcn g\u00f6r\u00fcn\u00fcr parlakl\u0131\u011f\u0131 -3,7 ile -4,6 aras\u0131nda de\u011fi\u015fir. \u015eans\u0131n\u0131z varsa ve do\u011fru yerde ve zamanda Ven\u00fcs’\u00fc \u00e7\u0131plak g\u00f6zle g\u00f6rebilirsiniz. Yine de, bir d\u00fcrb\u00fcn veya teleskop kullanman\u0131z\u0131 \u00f6neririz. B\u00f6ylece gezegenin t\u00fcm harika ayr\u0131nt\u0131lar\u0131n\u0131 g\u00f6rebilirsiniz. Bir y\u0131ld\u0131z g\u00f6zlemcisi olarak gece yapaca\u011f\u0131n\u0131z g\u00f6zlemlerie ilgili ipu\u00e7lar\u0131m\u0131za g\u00f6z at\u0131n.<\/a><\/p>\nVen\u00fcs s\u00fcrprizlerle dolu!<\/span><\/h2>\nBu blogda size a\u015fk\u0131n gezegeni olan Ven\u00fcs’\u00fc tan\u0131tt\u0131k. Ven\u00fcs’e neden “Sabah Y\u0131ld\u0131z\u0131” veya “Ak\u015fam Y\u0131ld\u0131z\u0131” ad\u0131 verildi\u011fini ve nas\u0131l g\u00f6r\u00fcnd\u00fc\u011f\u00fcn\u00fc art\u0131k biliyorsunuz. Buna ek olarak, Ven\u00fcs’\u00fcn G\u00fcne\u015f sisteminde nerede bulundu\u011funu ve bu beyaz gezegendeki ya\u015fam\u0131n neden imk\u00e2ns\u0131z oldu\u011funu \u00f6\u011frendiniz. Bu Sevgililer G\u00fcn\u00fc’ne Ven\u00fcs’e birlikte bak\u0131n, birbirinize ba\u011fland\u0131\u011f\u0131n\u0131z\u0131 hissedin ve sevdi\u011finiz ki\u015finin hayat\u0131n\u0131 ayd\u0131nlat\u0131n! OSR Star Finder uygulamas\u0131 ile G\u00fcne\u015f sistemimizde seyahat edin ve y\u0131ld\u0131zlar\u0131m\u0131z\u0131 ve gezegenlerimizi g\u00f6r\u00fcn!<\/p>\n
Ven\u00fcs, D\u00fcnya ve Merk\u00fcr aras\u0131ndaki y\u00f6r\u00fcngede yer almaktad\u0131r. Ven\u00fcs’\u00fcn Merk\u00fcr’e g\u00f6re G\u00fcne\u015f’ten \u00e7ok daha uzak oldu\u011funu g\u00f6z \u00f6n\u00fcnde bulundurursak, Ven\u00fcs’\u00fc genellikle D\u00fcnya’dan g\u00f6rebiliriz. G\u00fcne\u015f’e bu kadar yak\u0131n olmas\u0131 nedeniyle, Ven\u00fcs sadece g\u00fcn bat\u0131m\u0131ndan sonraki d\u00f6rt saatte veya g\u00fcn do\u011fumundan \u00f6nceki d\u00f6rt saatte g\u00f6r\u00fclebilir. Bu nedenle Ven\u00fcs’e “Sabah Y\u0131ld\u0131z\u0131” veya “Ak\u015fam Y\u0131ld\u0131z\u0131” ad\u0131 da verilmi\u015ftir! Bu ayn\u0131 zamanda Ven\u00fcs’\u00fcn g\u00fcnd\u00fcz ve gece g\u00f6r\u00fclemedi\u011fi anlam\u0131na gelir.<\/p>\n
Ven\u00fcs’\u00fc genellikle G\u00fcne\u015f’ten 48 dereceye kadar g\u00f6rebilirsiniz. Ven\u00fcs’\u00fcn g\u00f6r\u00fcn\u00fcr parlakl\u0131\u011f\u0131 -3,7 ile -4,6 aras\u0131nda de\u011fi\u015fir. \u015eans\u0131n\u0131z varsa ve do\u011fru yerde ve zamanda Ven\u00fcs’\u00fc \u00e7\u0131plak g\u00f6zle g\u00f6rebilirsiniz. Yine de, bir d\u00fcrb\u00fcn veya teleskop kullanman\u0131z\u0131 \u00f6neririz. B\u00f6ylece gezegenin t\u00fcm harika ayr\u0131nt\u0131lar\u0131n\u0131 g\u00f6rebilirsiniz. Bir y\u0131ld\u0131z g\u00f6zlemcisi olarak gece yapaca\u011f\u0131n\u0131z g\u00f6zlemlerie ilgili ipu\u00e7lar\u0131m\u0131za g\u00f6z at\u0131n.<\/a><\/p>\n Bu blogda size a\u015fk\u0131n gezegeni olan Ven\u00fcs’\u00fc tan\u0131tt\u0131k. Ven\u00fcs’e neden “Sabah Y\u0131ld\u0131z\u0131” veya “Ak\u015fam Y\u0131ld\u0131z\u0131” ad\u0131 verildi\u011fini ve nas\u0131l g\u00f6r\u00fcnd\u00fc\u011f\u00fcn\u00fc art\u0131k biliyorsunuz. Buna ek olarak, Ven\u00fcs’\u00fcn G\u00fcne\u015f sisteminde nerede bulundu\u011funu ve bu beyaz gezegendeki ya\u015fam\u0131n neden imk\u00e2ns\u0131z oldu\u011funu \u00f6\u011frendiniz. Bu Sevgililer G\u00fcn\u00fc’ne Ven\u00fcs’e birlikte bak\u0131n, birbirinize ba\u011fland\u0131\u011f\u0131n\u0131z\u0131 hissedin ve sevdi\u011finiz ki\u015finin hayat\u0131n\u0131 ayd\u0131nlat\u0131n! OSR Star Finder uygulamas\u0131 ile G\u00fcne\u015f sistemimizde seyahat edin ve y\u0131ld\u0131zlar\u0131m\u0131z\u0131 ve gezegenlerimizi g\u00f6r\u00fcn!<\/p>\nVen\u00fcs s\u00fcrprizlerle dolu!<\/span><\/h2>\n