| dbo:abstract |
An annular solar eclipse occurred on September 1, 1951. 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. Annularity was visible from the United States, Spanish Sahara (today's West Sahara), French West Africa (the parts now belonging to Mauritania, Mali, Burkina Faso and Ivory Coast), British Gold Coast (today's Ghana), southern tip of French Equatorial Africa (the part now belonging to R. Congo), Belgian Congo (today's DR Congo), Northern Rhodesia (today's Zambia), Portuguese Mozambique (today's Mozambique), Nyasaland (today's Malawi), and French Madagascar (today's Madagascar). (en) L'eclissi solare del 1º settembre 1951 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 12.51 UTC. L'eclissi, di tipo anulare, è stata visibile in alcune parti dell'Africa (Angola, Botswana, Congo, Costa d'Avorio, Ghana, Madagascar, Mauritania, Mozambico, Sahara Occidentale e Zimbabwe), del Sud America, del Nord America (Caraibi e Stati Uniti d'America) e dell'Europa. L'eclissi è durata 2 minuti e 36 secondi. (it) 1951년 9월 1일 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) 1951年9月1日日食是一次日環食，發生於1951年9月1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。此次日環食經過了美国、西屬撒哈拉、法屬西非、英屬黃金海岸、法屬赤道非洲、葡屬西非、比屬剛果、北羅德西亞、葡屬東非、尼亞薩蘭、法屬馬達加斯加，日偏食則覆蓋了北美洲東部、非洲絕大部分、欧洲西部及周邊部分地區。 (zh) |
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L'eclissi solare del 1º settembre 1951 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 12.51 UTC. L'eclissi, di tipo anulare, è stata visibile in alcune parti dell'Africa (Angola, Botswana, Congo, Costa d'Avorio, Ghana, Madagascar, Mauritania, Mozambico, Sahara Occidentale e Zimbabwe), del Sud America, del Nord America (Caraibi e Stati Uniti d'America) e dell'Europa. L'eclissi è durata 2 minuti e 36 secondi. (it) 1951년 9월 1일 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) 1951年9月1日日食是一次日環食，發生於1951年9月1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。此次日環食經過了美国、西屬撒哈拉、法屬西非、英屬黃金海岸、法屬赤道非洲、葡屬西非、比屬剛果、北羅德西亞、葡屬東非、尼亞薩蘭、法屬馬達加斯加，日偏食則覆蓋了北美洲東部、非洲絕大部分、欧洲西部及周邊部分地區。 (zh) An annular solar eclipse occurred on September 1, 1951. 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. Annularity was visible from the United States, Spanish Sahara (today's West Sahara), French West Africa (the parts now belonging to Mauritania, Mali, Burkina Faso and Ivory Coast), British Gold Coast (today's Ghana), southern tip of French Equatorial Africa (the part now belonging to R. Congo), Belgian Congo (en) |
| rdfs:label |
Eclissi solare del 1º settembre 1951 (it) 1951년 9월 1일 일식 (ko) Solar eclipse of September 1, 1951 (en) 1951年9月1日日食 (zh) |
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