Avtory i prava: Loren Laveder
(PixHeaven.net
/ Nochnoi mir)
Perevod: D.Yu.Cvetkov
Poyasnenie:
Diametr Luny —
3476 kilometrov.
Odnako vidimyi
uglovoi razmer,
to est' ugol, v kotorom pomeshaetsya ob'ekt, takzhe ves'ma vazhen dlya
lyubitelei nablyudat' Lunu.
Uglovoi razmer zavisit ot rasstoyaniya, i chem dal'she nahoditsya ob'ekt, tem men'she
ego uglovoi razmer.
Tak kak rasstoyanie do Luny — okolo 400 tysyach kilometrov, ee uglovoi razmer —
vsego 1/2 gradusa, to est' ee mozhno legko zakryt' konchikom pal'ca na vytyanutoi ruke,
a mozhno popytat'sya izmerit' ee ruletkoi, kotoruyu derzhit stoyashii nedaleko ot vas drug.
Konechno,
Solnce
namnogo bol'she Luny, a imenno v 400 raz bol'she.
Odnako segodnya molodaya Luna zakroet Solnce.
Polnoe solnechnoe zatmenie
mozhno budet nablyudat' v polose, prohodyashei cherez sever Kanady, Arktiku, Sibir' i sever Kitaya.
(Chastnoe zatmenie vidno iz bol'shei oblasti).
Solnechnye zatmeniya
naglyadno pokazyvayut udachnoe sovpadenie: hotya Solnce v 400 raz bol'she Luny,
ono i v 400 raz dal'she ee, i poetomu
uglovye razmery
Solnca i Luny pochti odinakovy.
Polnoe solnechnoe zatmenie:
Internet-translyaciya iz Kitaya
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Publikacii s klyuchevymi slovami:
solar eclipse - Solnechnoe zatmenie
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