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- Die Totalitätszone der totalen Sonnenfinsternis vom 21. August 1914 erstreckte sich über Nordamerika, Europa und Asien. (de)
- A total solar eclipse occurred on August 21, 1914. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.The totality of this eclipse was visible from northern Canada, Greenland, Norway, Sweden, Russian Empire (the parts now belonging to Åland, Finland, Estonia, Latvia, Lithuania, Belarus, Ukraine and Russia, including cities of Riga, Minsk, Kiev and northeastern part of Vilnius), Ottoman Empire (the parts now belonging to Turkey, northeastern tip of Syria and northern Iraq), Persia and British Raj (the parts now belonging to Pakistan and western tip of India).It was the first of four total solar eclipses that would be seen from Sweden during the next 40 years. This total solar eclipse occurred in the same calendar date as 2017, but at the opposite node. The moon was just 2.7 days before perigee, making it fairly large. A number of observatories sent expeditions to Russia to observe the eclipse including those from Argentina, the United Kingdom, Germany, Russia, and the United States. The expeditions led by Charles Dillon Perrine of the Argentine National Observatory, Erwin Finlay-Freundlich of the Berlin-Babelsberg Observatory, Germany, and William W. Campbell of the Lick Observatory, California, included in their programs the second attempt to verify the general relativity theory of Albert Einstein. (Perrine had made the first attempt at the 1912 solar eclipse in Brazil.) However, World War I broke out and Freundlich and his equipment were interned in Russia, unable to carry out the necessary measurements. C. D. Perrine and W. W. Campbell, from neutral countries, Argentina and the United States, were permitted to continue with their plans, but clouds obscured the eclipse. Perrine was able to obtain one photograph of the eclipse but the thin cloud cover was enough to obscure star locations necessary to test Einstein's theory. (en)
- L'eclissi solare del 21 agosto 1914 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 12.34 UTC.L'eclissi, di tipo totale, è stata visibile in alcune parti dell'Africa, dell'Europa (Norvegia, Russia e Svezia), dell'Asia (India, Iran, Iraq, Pakistan e Turchia), del Nord America (Canada) e della Groenlandia. La durata della fase massima dell'eclissi è stata di 2 minuti e 14 secondi; Il punto di massima totalità è avvenuto in Bielorussia tra e Vyazin e l'ombra lunare sulla superficie terrestre raggiunse una larghezza di 170 km. L'eclissi del 21 agosto 1914 divenne la seconda eclissi solare nel 1914 e la 32ª nel XX secolo. La precedente eclissi solare si è verificata il 25 febbraio 1914, la seguente il 14 febbraio 1915. (it)
- 1914년 8월 21일 일식은 달이 지구와 태양 사이를 지나면서 태양을 완전히 가리는 개기일식이다. 개기일식은 달의 시직경이 태양의 시직경보다 커서 태양을 다 가릴 수 있을 때 일어난다. 개기일식은 매우 좁은 지역에서만 관측 가능하며, 대부분의 다른 지역에서는 부분일식으로 관측된다. (ko)
- 1914年8月21日の日食は、1914年8月21日に観測された日食である。カナダ、グリーンランド、ノルウェー、スウェーデン、ロシア帝国、オスマン帝国、ペルシャ、イギリス領インドで皆既日食が観測され、北アメリカ東北部、ヨーロッパ全部、アジア中西部、アフリカ北東部の約半分で部分日食が観測された。 (ja)
- De totale zonsverduistering van 21 augustus 1914 trok veel over land en was achtereenvolgens te zien in deze 17 landen : Canada, Groenland, Noorwegen, Zweden, Finland, Estland, Letland, Litouwen, Wit-Rusland, Oekraïne, Rusland, Turkije, Syrië, Irak, Iran, Pakistan en India. (nl)
- Солнечное затмение 21 августа 1914 года — полное солнечное затмение, которое наблюдались в Канаде и Гренландии, в различных странах Европы и Азии. Частные фазы затмения наблюдались также в Африке. Астрономы из разных стран предприняли попытки наблюдения этого затмения; в частности, планировалось с его помощью проверить общую теорию относительности. Однако Первая мировая война и облачность в местах наблюдения помешала осуществиться большинству экспериментов. (ru)
- 1914年8月21日日食是一次日全食，發生於1914年8月21日。新月當天（即朔日），地球上觀測到月球和太阳的角距離極小，此時月球如果恰好在月球交點附近，穿過太阳和地球之間，與地球、太阳接近一直線，則會出現日食。月球本影接觸地表而使該區域完全得不到陽光，就會形成日全食，同時在本影兩側數千公里的半影範圍內遮擋部分陽光，形成日偏食。此次日全食經過了加拿大、格陵兰、挪威、瑞典、俄國、鄂圖曼帝國、波斯、英屬印度，日偏食則覆蓋了北美洲東北部、整個欧洲、亚洲中西部、非洲東北半部。 (zh)
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- Die Totalitätszone der totalen Sonnenfinsternis vom 21. August 1914 erstreckte sich über Nordamerika, Europa und Asien. (de)
- 1914년 8월 21일 일식은 달이 지구와 태양 사이를 지나면서 태양을 완전히 가리는 개기일식이다. 개기일식은 달의 시직경이 태양의 시직경보다 커서 태양을 다 가릴 수 있을 때 일어난다. 개기일식은 매우 좁은 지역에서만 관측 가능하며, 대부분의 다른 지역에서는 부분일식으로 관측된다. (ko)
- 1914年8月21日の日食は、1914年8月21日に観測された日食である。カナダ、グリーンランド、ノルウェー、スウェーデン、ロシア帝国、オスマン帝国、ペルシャ、イギリス領インドで皆既日食が観測され、北アメリカ東北部、ヨーロッパ全部、アジア中西部、アフリカ北東部の約半分で部分日食が観測された。 (ja)
- De totale zonsverduistering van 21 augustus 1914 trok veel over land en was achtereenvolgens te zien in deze 17 landen : Canada, Groenland, Noorwegen, Zweden, Finland, Estland, Letland, Litouwen, Wit-Rusland, Oekraïne, Rusland, Turkije, Syrië, Irak, Iran, Pakistan en India. (nl)
- Солнечное затмение 21 августа 1914 года — полное солнечное затмение, которое наблюдались в Канаде и Гренландии, в различных странах Европы и Азии. Частные фазы затмения наблюдались также в Африке. Астрономы из разных стран предприняли попытки наблюдения этого затмения; в частности, планировалось с его помощью проверить общую теорию относительности. Однако Первая мировая война и облачность в местах наблюдения помешала осуществиться большинству экспериментов. (ru)
- 1914年8月21日日食是一次日全食，發生於1914年8月21日。新月當天（即朔日），地球上觀測到月球和太阳的角距離極小，此時月球如果恰好在月球交點附近，穿過太阳和地球之間，與地球、太阳接近一直線，則會出現日食。月球本影接觸地表而使該區域完全得不到陽光，就會形成日全食，同時在本影兩側數千公里的半影範圍內遮擋部分陽光，形成日偏食。此次日全食經過了加拿大、格陵兰、挪威、瑞典、俄國、鄂圖曼帝國、波斯、英屬印度，日偏食則覆蓋了北美洲東北部、整個欧洲、亚洲中西部、非洲東北半部。 (zh)
- A total solar eclipse occurred on August 21, 1914. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.The totality of this eclipse was visible from northern Canada, Greenland, Norway, Sweden, Russian Empire (the parts now belonging to Åland, Finland, Estonia, Latvia, Lithuania, Belarus, Ukraine and Russia, including cities of Riga, Minsk, Kiev and northeastern part of Vilnius), Ottoman Empire (the pa (en)
- L'eclissi solare del 21 agosto 1914 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 12.34 UTC.L'eclissi, di tipo totale, è stata visibile in alcune parti dell'Africa, dell'Europa (Norvegia, Russia e Svezia), dell'Asia (India, Iran, Iraq, Pakistan e Turchia), del Nord America (Canada) e della Groenlandia. La durata della fase massima dell'eclissi è stata di 2 minuti e 14 secondi; Il punto di massima totalità è avvenuto in Bielorussia tra e Vyazin e l'ombra lunare sulla superficie terrestre raggiunse una larghezza di 170 km. (it)
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