A.cluster
B.shower
C.constellation
D.galaxy
您可能感興趣的試卷
你可能感興趣的試題
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
A.the Sun
B.the Moon
C.Venus
D.None of the above
A.the declination is the opposite name to the latitude
B.the algebraic sum of the colatitude and declination exceeds 90
C.the observer is in high latitudes above either polar circle
D.the body is circumpolar
![](https://static.ppkao.com/ppmg/img/appqrcode.png)
最新試題
測定羅經(jīng)差精度較高的方法是()
英版《潮汐表》中,潮高差是()
太陽方位正南,觀測太陽上中天高度求緯度,則()
在中版《航海天文歷》的“恒星視位置表”中可查取恒星的()①地方時角②格林時角③共軛赤經(jīng)④赤緯
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()
測者可自行校正的六分儀誤差有:①定鏡差;②指標(biāo)差;③動鏡差。三者正確的校正順序是()
將觀測高度修正為真高度時,需要進行半徑差改正的天體是()
將觀測高度修正為真高度時,不必進行視差改正的天體是()
天體高度與視差的關(guān)系,下列說法正確的是()
在六分儀上直接讀取太陽的下邊緣觀測高度,并利用英版《航海天文歷》求太陽的真高度,則需要修正哪些誤差?()①器差②指標(biāo)差③眼高差④綜合改正⑤附加改正