Solar eclipse of April 29, 1995 (original) (raw)
An annular solar eclipse occurred on April 29, 1995. 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 in Peru, southeastern Ecuador, southeastern Colombia and Brazil.
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| dbo:abstract | Bei der ringförmige Sonnenfinsternis vom 29. April 1995 verlief die 195,5 Kilometer breite Zentralzone über das dünnbesiedelte Amazonasbecken. Die Dauer der ringförmigen Phase lag etwa 6½ Minuten im Mittelfeld. Ihre Saros-Nachfolgerin ist die Sonnenfinsternis vom 10. Mai 2013, dessen ringförmige Zone über das ebenso dünnbesiedelte Nordwestaustralien verlaufen wird. Der Saros 138 begann am 6. Juni 1472 mit nur 7 partiellen Finsternissen in der Antarktis. Danach erfolgen 50 ringförmige, gefolgt von einer hybriden und 3 totalen Sonnenfinsternissen. Nach 9 weiteren partiellen Finsternissen in der Arktis endet Saros 138 am 11. Juli 2716. (de) An annular solar eclipse occurred on April 29, 1995. 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 in Peru, southeastern Ecuador, southeastern Colombia and Brazil. (en) 1995년 4월 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) L'eclissi solare del 29 aprile 1995 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 17.33 UTC. L'eclissi, di tipo anulare, è stata visibile in Perù, nell'Ecuador sud-orientale, nella Colombia sud-orientale e in Brasile. L'eclissi è durata 6 minuti e 37 secondi e l'ombra lunare sulla superficie terrestre ha raggiunto una larghezza di 196 km. L'eclissi del 29 aprile 1995 è stata la prima eclissi solare nel 1995 e la 215ª nel XX secolo. La precedente eclissi solare si è verificata il 3 novembre 1994, la seguente è avvenuta il 24 ottobre 1995. (it) 1995年4月29日の日食は、1995年4月29日に観測された日食である。ペリー、エクアドル、コロンビア、ブラジルで金環日食が観測され、ラテンアメリカのほとんどと以上の地域の周辺の一部で部分日食が観測された。 (ja) 1995年4月29日日食是一次日環食，發生於1995年4月29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。此次日環食經過了秘鲁、厄瓜多尔、哥伦比亚、巴西，日偏食則覆蓋了拉丁美洲的大部分和周邊部分地區。 (zh) |
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| rdfs:comment | An annular solar eclipse occurred on April 29, 1995. 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 in Peru, southeastern Ecuador, southeastern Colombia and Brazil. (en) 1995년 4월 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) L'eclissi solare del 29 aprile 1995 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 17.33 UTC. L'eclissi, di tipo anulare, è stata visibile in Perù, nell'Ecuador sud-orientale, nella Colombia sud-orientale e in Brasile. L'eclissi è durata 6 minuti e 37 secondi e l'ombra lunare sulla superficie terrestre ha raggiunto una larghezza di 196 km. L'eclissi del 29 aprile 1995 è stata la prima eclissi solare nel 1995 e la 215ª nel XX secolo. La precedente eclissi solare si è verificata il 3 novembre 1994, la seguente è avvenuta il 24 ottobre 1995. (it) 1995年4月29日の日食は、1995年4月29日に観測された日食である。ペリー、エクアドル、コロンビア、ブラジルで金環日食が観測され、ラテンアメリカのほとんどと以上の地域の周辺の一部で部分日食が観測された。 (ja) 1995年4月29日日食是一次日環食，發生於1995年4月29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。此次日環食經過了秘鲁、厄瓜多尔、哥伦比亚、巴西，日偏食則覆蓋了拉丁美洲的大部分和周邊部分地區。 (zh) Bei der ringförmige Sonnenfinsternis vom 29. April 1995 verlief die 195,5 Kilometer breite Zentralzone über das dünnbesiedelte Amazonasbecken. Die Dauer der ringförmigen Phase lag etwa 6½ Minuten im Mittelfeld. Ihre Saros-Nachfolgerin ist die Sonnenfinsternis vom 10. Mai 2013, dessen ringförmige Zone über das ebenso dünnbesiedelte Nordwestaustralien verlaufen wird. (de) |
| rdfs:label | Sonnenfinsternis vom 29. April 1995 (de) Eclissi solare del 29 aprile 1995 (it) 1995년 4월 29일 일식 (ko) 1995年4月29日の日食 (ja) Solar eclipse of April 29, 1995 (en) 1995年4月29日日食 (zh) |
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