Solar eclipse of March 29, 1903 (original) (raw)

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An annular solar eclipse occurred on March 29, 1903. 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 China (now northwestern China, Mongolia and northeastern China), Russia on March 29th (Sunday), and Northern Canada on March 28th (Saturday).

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dbo:abstract An annular solar eclipse occurred on March 29, 1903. 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 China (now northwestern China, Mongolia and northeastern China), Russia on March 29th (Sunday), and Northern Canada on March 28th (Saturday). (en) L'eclissi solare del 29 marzo 1903 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 01.35 UTC. L'eclissi, di tipo anulare, è stata visibile dalla Cina (ora Cina nordoccidentale, Mongolia e Cina nord-orientale), dalla Russia il 29 marzo (domenica) e dal Canada settentrionale il 28 marzo (sabato). L'eclissi è durata 1 minuto e 53 secondi. (it) 1903년 3월 29일 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) 1903年3月29日の日食は、1903年3月29日に観測された日食である。中国、ロシア、カナダで金環日食が観測され、アジア中東部、北アメリカ北西部及び以上の地域の周辺の一部で部分日食が観測された。 (ja) 1903年3月29日日食是一次日環食，發生於1903年3月29日（西半球爲3月28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。此次日環食經過了中國、俄國、加拿大，日偏食則覆蓋了亚洲中東部、北美洲西北部及周邊部分地區。 (zh)
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rdfs:comment An annular solar eclipse occurred on March 29, 1903. 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 China (now northwestern China, Mongolia and northeastern China), Russia on March 29th (Sunday), and Northern Canada on March 28th (Saturday). (en) L'eclissi solare del 29 marzo 1903 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 01.35 UTC. L'eclissi, di tipo anulare, è stata visibile dalla Cina (ora Cina nordoccidentale, Mongolia e Cina nord-orientale), dalla Russia il 29 marzo (domenica) e dal Canada settentrionale il 28 marzo (sabato). L'eclissi è durata 1 minuto e 53 secondi. (it) 1903년 3월 29일 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) 1903年3月29日の日食は、1903年3月29日に観測された日食である。中国、ロシア、カナダで金環日食が観測され、アジア中東部、北アメリカ北西部及び以上の地域の周辺の一部で部分日食が観測された。 (ja) 1903年3月29日日食是一次日環食，發生於1903年3月29日（西半球爲3月28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。此次日環食經過了中國、俄國、加拿大，日偏食則覆蓋了亚洲中東部、北美洲西北部及周邊部分地區。 (zh)
rdfs:label Eclissi solare del 29 marzo 1903 (it) 1903年3月29日の日食 (ja) 1903년 3월 29일 일식 (ko) Solar eclipse of March 29, 1903 (en) 1903年3月29日日食 (zh)
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