یہ فائل ویکی ذخائر کی ہے اور دیگر منصوبوں کے زیر استعمال ہوسکتی ہے۔
فائل کے صفحہ تعارف پر موجود تعارف ذیل میں موجود ہے۔
خلاصہ
تفصیلAerial view of the ESO Very Large Telescope (VLT).jpg
English: Aerial view of the ESO Very Large Telescope (VLT), atop Cerro Paranal, in the Chilean Atacama Desert. On the low-left side of the platform, the buildings of the four giant 8.2-metre Unit Telescopes (UTs) are clearly distinguishable. The UTs can observe either individually or combined by two or three, using a technique called interferometry. Their position in the platform is the one which allows the maximum number of possible configurations. Aligned on the right of the UTs are the four 1.8-metre Auxiliary Telescopes (ATs), entirely dedicated to interferometric observations. The ATs can be relocated in 30 different observing positions, allowing a huge number of different configurations. On the left corner of the platform is the 2.6-metre VLT Survey Telescope (VST). With a 256 megapixels camera, the VST will have a field of view four times the area of the full Moon, enabling the VST to cover large areas of the sky. On the lower side of the platform is the Control Building, where astronomers operate the telescopes during the night.
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شیئر کرنے – کام کو نقل، تقسیم یا منتقل کرنے کے لیے
ریمکس کے لیے – کام منبطق کرنے کے لیے
مندرجہ ذیل شرائط کے تحت:
انتساب – آپ کو اس کام کا انتساب مصنف یا اجازت دہندہ کے بتائے گئے طریقہ کے مطابق دینا ہوگا (تاہم یہ انتساب اس طرح نہیں ہونا چاہیے کہ اسے دیکھ کر ایسا محسوس ہو کہ اصل مصنف یا اجازت دہندہ آپ کے یا آپ کے ذریعہ اس کام کے استعمال کرنے کے حامی ہیں)۔
https://creativecommons.org/licenses/by/4.0CC BY 4.0 Creative Commons Attribution 4.0 truetrue
Captions
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اِس فائل میں اِضافی معلومات شامل ہیں، جو شاید اُس ڈیجیٹل کیمرے یا اِسکینر سے آئی ہیں جس کے ذریعے یہ فائل بنائی گئی تھی۔
اگر فائل اپنی اصل حالت میں نہ ہو تو کچھ معلومات ترمیم شدہ فائل کی مکمل طور پر عکاسی نہیں کر پائیں گی۔
تصویر کا عنوان
Aerial view of the ESO Very Large Telescope (VLT), atop Cerro Paranal, in the Chilean Atacama Desert. On the low-left side of the platform, the buildings of the four giant 8.2-metre Unit Telescopes (UTs) are clearly distinguishable. The UTs can observe either individually or combined by two or three, using a technique called interferometry. Their position in the platform is the one which allows the maximum number of possible configurations. Aligned on the right of the UTs are the four 1.8-metre Auxiliary Telescopes (ATs), entirely dedicated to interferometric observations. The ATs can be relocated in 30 different observing positions, allowing a huge number of different configurations. On the left corner of the platform is the 2.6-metre VLT Survey Telescope (VST). With a 256 megapixels camera, the VST will have a field of view four times the area of the full Moon, enabling the VST to cover large areas of the sky. On the lower side of the platform is the Control Building, where astronomers operate the telescopes during the night.
مصنف
J.L. DAUVERGNE/Ciel et Espace
ڈیٹا تیار کرنے کی تاریخ اور وقت
13:41، 28 جولائی 2010ء
ماخذ
European Southern Observatory
کریڈٹ/مہیا کار
J.L. Dauvergne & G. Hüdepohl (atacamaphoto.com)/ESO
استعمال کے شرائط
Creative Commons Attribution 4.0 International License