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The night sky Including a sky tour for double andvariable star observers

机译:夜空包括双星和变星观测者的天空之旅

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Capella itself will not transit until after 3am andDecember, not October, is its best month, but from the UKit is actually visible all year round because, at +46 degrees,it never drops below seven degrees altitude from London.By midnight it is already 55 degrees above the easternhorizon. Capella shines at magnitude +0.1 making it thethird brightest star in the northern celestial sphere. It is nota 60,000 solar luminosity cosmic lighthouse like Deneb,but simply a very bright nearby system just 42 light yearsdistant. Capella's light comes mainly from two giant stars,roughly ten times the diameter of our own Sun and a 'mere'80 times its luminosity. Their separation of only 100 millionkilometres means the two stars are only a twentieth of anarcsecond apart as seen from Earth and so not resolvablein amateur telescopes. The stars do not eclipse from ourviewing point, but simply orbit each other every 104 days.Capella will be a prominent marker in the skies for manymonths to come.
机译:卡佩拉(Capella)本身要到凌晨3点和12月(不是10月)才是最好的月份,但是从UKit全年都可以看到,因为在+46度时,它从未降落到距伦敦7度以下的高度。到午夜时分东纬55度以上。卡佩拉(Capella)的辐射强度为+0.1,成为北天球上第三颗最亮的恒星。它不是像Deneb那样的60,000个太阳光度宇宙灯塔,而仅仅是距离我们仅42光年的非常明亮的附近系统。卡佩拉的光主要来自两颗巨星,大约是我们自己太阳直径的十倍,是其光度的“仅” 80倍。它们的间隔只有1亿公里,这意味着从地球上看,两颗星仅相隔了二十秒的弧度,因此在业余望远镜中无法分辨。从我们的角度来看,恒星并不会黯然失色,而是每104天绕轨道运行一次。Capella将在未来数月成为天空中的杰出标志。

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