A.stars
B.Moon
C.Sun
D.Planets
您可能感興趣的試卷
你可能感興趣的試題
A.error of perpendicularity
B.side error
C.prismatic error
D.centering error
A.cluster
B.shower
C.constellation
D.galaxy
A.cluster
B.shower
C.constellation
D.galaxy
A.2.5 times as bright as a second magnitude star
B.3 times as bright as a second magnitude star
C.5 times as bright as a second magnitude star
D.10 times as bright as a second magnitude star
A.has a declination equal to twice that of the Sun
B.comprises two stars that appear close together
C.is twice as bright as a single star
D.suddenly becomes much brighter and then fades
![](https://static.ppkao.com/ppmg/img/appqrcode.png)
最新試題
英版海圖上回轉(zhuǎn)流表列潮流在某個(gè)方向上有兩個(gè)速度,表示()
英版《航海天文歷》高度修正表中太陽高度總改正表的查表引數(shù)是()
將觀測高度修正為真高度時(shí),需要進(jìn)行半徑差改正的天體是()
一般觀測天體定位應(yīng)避免觀測高度較低的天體,其主要原因是()
《航海天文歷》中列出的太陽出沒時(shí)刻是()
航海上測定指標(biāo)差時(shí),可以利用()①星體②太陽③水天線
使用英版《航海天文歷》高度修正表求取行星真高度時(shí),總改正的查表引數(shù)是()
縮小六分儀邊差的方法是()
影響蒙氣差的因素有()①氣溫②氣壓③天體高度
英版《潮汐表》中,潮高差是()