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Pyxis Constellation Map
图像
图注: The constellation Pyxis with its bright stars and surrounding constellations. Pyxis is surrounded by (going clockwise from the top): Hydra, Puppis, Vela and Antilia.
Pyxis is a southern constellation and thus the whole constellation is visible at some point in the year throughout the southern hemisphere. The whole constellation is also visible in equatorial and some temperate regions of the northern hemisphere with parts of the constellation visible to the remaining temperate regions of the northern hemisphere.
The y-axis of this diagram is in degrees of declination with north as up and the x-axis is in hours of right ascension with east to the left. The sizes of the stars marked here relate to the star's apparent magnitude, a measure of its apparent brightness. The larger dots represent brighter stars. The Greek letters mark the brightest stars in the constellation. These are ranked by brightness with the brightest star being labeled alpha, the second brightest beta, etc., although this ordering is not always followed exactly. The dotted boundary lines mark the IAU's boundaries of the constellations and the solid green lines mark one of the common forms used to represent the figures of the constellations. Neither the constellation boundaries, nor the lines joining the stars appear on the sky.
来源: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope
来源链接
词汇表:
视星等 , 天球坐标 , 星座 , 赤纬 , 赤经(RA)
分类:
肉眼天文学
授权许可: 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 图标
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( 图像
73.93 kB)
PDF 文件
(PDF file
152.64 kB)
Columba Constellation Map
图像
图注: The constellation Columba with its bright stars and surrounding constellations. Columba is surrounded by (going clockwise from the top): Lepus, Caelum, Pictor, Puppis and Canis Major.
Columba is a southern constellation and thus is visible to the whole southern hemisphere at some point in the year. The whole constellation is also visible from equatorial and some temperate regions of the northern hemisphere.
The globular cluster NGC 1851 lies in Columba and is marked here with a yellow circle with a plus sign superimposed on it.
The y-axis of this diagram is in degrees of declination with north as up and the x-axis is in hours of right ascension with east to the left. The sizes of the stars marked here relate to the star's apparent magnitude, a measure of its apparent brightness. The larger dots represent brighter stars. The Greek letters mark the brightest stars in the constellation. These are ranked by brightness with the brightest star being labeled alpha, the second brightest beta, etc., although this ordering is not always followed exactly. The dotted boundary lines mark the IAU's boundaries of the constellations and the solid green lines mark one of the common forms used to represent the figures of the constellations. Neither the constellation boundaries, nor the lines joining the stars appear on the sky.
来源: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope
来源链接
词汇表:
视星等 , 天球坐标 , 星座 , 赤纬 , 赤经(RA)
分类:
肉眼天文学
授权许可: 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 图标
文件
( 图像
85.80 kB)
PDF 文件
(PDF file
158.40 kB)
Corona Borealis Constellation Map
图像
图注: The constellation Corona Borealis with its bright stars and surrounding constellations. Corona Borealis is surrounded by (going clockwise from the top): Boötes, Serpens Caput and Hercules.
Corona Borealis is a northern constellation and thus the constellation is visible from the whole northern hemisphere at some point in the year. It whole constellation is also visible from equatorial and most temperate regions of the southern hemisphere. The constellation is best viewed in the evening in the northern hemisphere summer and southern hemisphere winter.
The y-axis of this diagram is in degrees of declination with north as up and the x-axis is in hours of right ascension with east to the left. The sizes of the stars marked here relate to the star's apparent magnitude, a measure of its apparent brightness. The larger dots represent brighter stars. The Greek letters mark the brightest stars in the constellation. These are ranked by brightness with the brightest star being labeled alpha, the second brightest beta, etc., although this ordering is not always followed exactly. The dotted boundary lines mark the IAU's boundaries of the constellations and the solid green lines mark one of the common forms used to represent the figures of the constellations. Neither the constellation boundaries, nor the lines joining the stars appear on the sky.
来源: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope
来源链接
词汇表:
视星等 , 天球坐标 , 星座 , 赤纬 , 赤经(RA)
分类:
肉眼天文学
授权许可: 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 图标
文件
( 图像
80.08 kB)
PDF 文件
(PDF file
154.15 kB)
Equuleus Constellation Map
图像
图注: The constellation Equuleus with its brighter stars and surrounding constellations. Equuleus is surrounded by (going clockwise from the top): Delphinus, Aquarius and Pegasus. It is a relatively small constellation with few bright stars.
Equuleus lies just north of the celestial equator and thus the whole constellation is visible at some point in the year to all but the most antarctic regions. Equuleus is best viewed in the evening in the early northern hemisphere autumn and early southern hemisphere spring.
The y-axis of this diagram is in degrees of declination with north as up and the x-axis is in hours of right ascension with east to the left. The sizes of the stars marked here relate to the star's apparent magnitude, a measure of its apparent brightness. The larger dots represent brighter stars. The Greek letters mark the brightest stars in the constellation. These are ranked by brightness with the brightest star being labeled alpha, the second brightest beta, etc., although this ordering is not always followed exactly. The dotted boundary lines mark the IAU's boundaries of the constellations and the solid green lines mark one of the common forms used to represent the figures of the constellations. Neither the constellation boundaries, nor the lines joining the stars appear on the sky.
来源: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope
来源链接
词汇表:
视星等 , 天球坐标 , 星座 , 赤纬 , 赤经(RA) , 宝瓶座
分类:
肉眼天文学
授权许可: 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 图标
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( 图像
61.60 kB)
PDF 文件
(PDF file
143.63 kB)
Grus Constellation Map
图像
图注: The constellation Grus with its bright stars and surrounding constellations. Grus is surrounded by (going clockwise from the top): Piscis Austrinus, Microscopium, Indus, Tucana, Phoenix and Sculptor.
Grus is a southern constellation and thus the whole constellation is visible at some point in the year from the whole southern hemisphere at some point in the year. The whole constellation is also visible from equatorial and some temperate regions of the northern hemisphere. Grus is best viewed in the evening in the northern hemisphere autumn and southern hemisphere spring.
The y-axis of this diagram is in degrees of declination with north as up and the x-axis is in hours of right ascension with east to the left. The sizes of the stars marked here relate to the star's apparent magnitude, a measure of its apparent brightness. The larger dots represent brighter stars. The Greek letters mark the brightest stars in the constellation. These are ranked by brightness with the brightest star being labeled alpha, the second brightest beta, etc., although this ordering is not always followed exactly. The dotted boundary lines mark the IAU's boundaries of the constellations and the solid green lines mark one of the common forms used to represent the figures of the constellations. Neither the constellation boundaries, nor the lines joining the stars appear on the sky.
来源: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope
来源链接
词汇表:
视星等 , 天球坐标 , 星座 , 赤纬 , 赤经(RA)
分类:
肉眼天文学
授权许可: 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 图标
文件
( 图像
105.07 kB)
PDF 文件
(PDF file
179.81 kB)
