| dbo:abstract |
An annular solar eclipse occurred on February 25, 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. (en) 1914년 2월 25일 일식은 달이 지구와 태양 사이를 지나면서 태양을 다 가리지 못하고 태양의 가장자리가 고리 모양으로 보이는 금환일식이다. 금환일식은 달의 시직경이 태양의 시직경보다 작아 태양을 다 가리지 못할 때 일어난다. 금환일식은 매우 좁은 지역에서만 관측 가능하며, 대부분의 다른 지역에서는 부분일식으로 관측된다 (ko) L'eclissi solare del 25 febbraio 1914 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 0.13 UTC. L'eclissi anulare si verifica quando il diametro visivo della luna è più piccolo di quello del sole, quindi questo non può essere completamente coperto.. L'eclissi anulare può essere osservata solo in aree molto piccole, e nella maggior parte delle altre aree può essere osservata come un'eclissi parziale. L'eclissi del 25 febbraio 1914, di tipo anulare, è stata visibile in alcune parti dell'Antartide e della Nuova Zelanda. L'evento è durato 5 minuti e 35 secondi e l'ombra lunare proiettata sulla superficie terrestre raggiunse una larghezza di 839 km. L'eclissi aveva una magnitudine di 0,9248 e raggiunse il massimo alle 00:13:01 UTC alle coordinate di 62° S.w. - 113° O. L'eclissi del 25 febbraio 1914 divenne la prima eclissi solare nel 1914 e la 31° nel XX secolo. L'eclissi solare precedente avvenne il 30 settembre 1913 e la seguente avvenne il 21 agosto 1914. (it) 1914年2月25日日食是一次日環食，發生於1914年2月25日（包括整個環食帶在內的西半球大多爲2月24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。月球穿過太阳和地球之間，但距地球較遠，本影未能接觸地表，而使偽本影覆蓋的區域內看到月球的角直徑小於太陽，就形成日環食，同時在偽本影兩側數千公里的半影範圍內形成日偏食。此次日環食經過了南极洲毛德皇后地和玛丽·伯德地，日偏食則覆蓋了南极洲大部、太平洋中南部及周邊部分地區。 (zh) |
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An annular solar eclipse occurred on February 25, 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. (en) 1914년 2월 25일 일식은 달이 지구와 태양 사이를 지나면서 태양을 다 가리지 못하고 태양의 가장자리가 고리 모양으로 보이는 금환일식이다. 금환일식은 달의 시직경이 태양의 시직경보다 작아 태양을 다 가리지 못할 때 일어난다. 금환일식은 매우 좁은 지역에서만 관측 가능하며, 대부분의 다른 지역에서는 부분일식으로 관측된다 (ko) 1914年2月25日日食是一次日環食，發生於1914年2月25日（包括整個環食帶在內的西半球大多爲2月24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。月球穿過太阳和地球之間，但距地球較遠，本影未能接觸地表，而使偽本影覆蓋的區域內看到月球的角直徑小於太陽，就形成日環食，同時在偽本影兩側數千公里的半影範圍內形成日偏食。此次日環食經過了南极洲毛德皇后地和玛丽·伯德地，日偏食則覆蓋了南极洲大部、太平洋中南部及周邊部分地區。 (zh) L'eclissi solare del 25 febbraio 1914 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 0.13 UTC. L'eclissi anulare si verifica quando il diametro visivo della luna è più piccolo di quello del sole, quindi questo non può essere completamente coperto.. L'eclissi anulare può essere osservata solo in aree molto piccole, e nella maggior parte delle altre aree può essere osservata come un'eclissi parziale. L'eclissi del 25 febbraio 1914, di tipo anulare, è stata visibile in alcune parti dell'Antartide e della Nuova Zelanda. (it) |
| rdfs:label |
Eclissi solare del 25 febbraio 1914 (it) 1914년 2월 25일 일식 (ko) Solar eclipse of February 25, 1914 (en) 1914年2月25日日食 (zh) |
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