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A total solar eclipse occurred on February 25, 1952. 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 path of totality crossed Africa, the Middle East, and Asia.

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  • Eclissi solare del 25 febbraio 1952 (it)
  • 1952년 2월 25일 일식 (ko)
  • 1952年2月25日の日食 (ja)
  • Zonsverduistering van 25 februari 1952 (nl)
  • Solar eclipse of February 25, 1952 (en)
  • Солнечное затмение 25 февраля 1952 года (ru)
  • 1952年2月25日日食 (zh)
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  • A total solar eclipse occurred on February 25, 1952. 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 path of totality crossed Africa, the Middle East, and Asia. (en)
  • 1952年2月25日の日食は、1952年2月25日に観測された日食である。ポルトガル領サントメ・プリンシペ、フランス領赤道アフリカ、スペイン領ギニア、フランス領カメルーン、ベルギー領コンゴ、英埃領スーダン、サウジアラビア、サウジアラビアとイラクの中立地帯、イラク、イギリス領クウェート、イラン、ソ連で皆既日食が観測され、ヨーロッパのほとんど、アフリカのほとんど、アジア中西部で部分日食が観測された。 (ja)
  • 1952년 2월 25일 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)
  • De totale zonsverduistering van 25 februari 1952 trok veel over zee, maar was achtereenvolgens te zien in deze 17 landen : (nl)
  • Солнечное затмение 25 февраля 1952 года — полное солнечное затмение 139 сароса. Максимальная фаза затмения составила 1,0366 и достигла своего максимума в 09:11:35 UTC. Максимальная длительность полной фазы — 3 минуты и 9 секунд, а лунная тень на земной поверхности достигла ширины 138 км. Следующее затмение данного сароса произошло 7 марта 1970 года. Данное затмение стало вторым солнечным затмением в 1970-х годах и 160-м затмением XX века. Предыдущее солнечное затмение произошло , а следующее — . (ru)
  • 1952年2月25日日食是一次日全食,發生於1952年2月25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。此次日全食經過了葡屬聖多美和普林西比、法屬赤道非洲、西屬幾內亞、法屬喀麥隆、比屬剛果、英埃蘇丹、沙特阿拉伯、沙特阿拉伯-伊拉克中立区、伊拉克、英屬科威特、伊朗、苏联,日偏食則覆蓋了歐洲、非洲的幾乎全部和亚洲中西部的廣大地區。 (zh)
  • L'eclissi solare del 25 febbraio 1952 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 9.11 UTC. L'eclissi, di tipo totale, è stata visibile in alcune parti dell'Europa, dell'Africa (Gabon, Repubblica Centrafricana e Sudan), dell'Asia (Arabia Saudita, Kazakistan, Iran, Iraq, Turkmenistan e Uzbekistan) e della Russia; Il punto di massima totalità è stato nel Nord Sudan nella capitale Khartoum. La durata della fase massima dell'eclissi è stata di 3 minuti e 9 secondi e l'ombra lunare sulla superficie terrestre raggiunse una larghezza di 138 km. (it)
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