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Pavo Constellation Map
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Legenda: The constellation Pavo with its bright stars and surrounding constellations. Pavo is surrounded by (going clockwise from the top): Telescopium, Ara, Apus, Octans and Indus.
Pavo 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 some equatorial regions of the northern hemisphere with parts of the constellation visible in the remaining northern equatorial regions. Pavo is circumpolar in antarctic 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 globular cluster NGC 6752 lies in Pavo 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.
Crédito: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope
Link do crédito
Termos do Glossário:
Magnitude aparente , Coordenadas celestes , Estrelas circumpolares , Constelação , Declinação , Aglomerado Globular , Ascensão Reta (AR)
Categorias
Astronomia a Olho Nu
Licença: Creative Commons Attribution 4.0 International (CC BY 4.0) Creative Commons Attribution 4.0 International (CC BY 4.0) ícones
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128.18 kB)
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188.85 kB)
Delphinus Constellation Map
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Legenda: The constellation Delphinus with its brighter stars and surrounding constellations. Delphinus is surrounded by (going clockwise from the top): Vulpecula, Sagitta, Aquila, Aquarius, Equuleus and Pegasus. Delphinus is a relatively small constellation with few bright stars.
Delphinus 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. The constellation is best viewed in the evenings in the early northern hemisphere autumn and early southern hemisphere spring.
The globular cluster NGC 6934 lies in Dephinus. It 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.
Crédito: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope
Link do crédito
Termos do Glossário:
Magnitude aparente , Coordenadas celestes , Equador Celeste , Constelação , Declinação , Aglomerado Globular , Ascensão Reta (AR) , Aquário
Categorias
Astronomia a Olho Nu
Licença: Creative Commons Attribution 4.0 International (CC BY 4.0) Creative Commons Attribution 4.0 International (CC BY 4.0) ícones
Arquivo
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70.98 kB)
Arquivo PDF
(PDF file
147.37 kB)
Canes Venatici Constellation Map
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Legenda: The constellation Canes Venatici with its brighter stars and surrounding constellations. Canes Venatici is surrounded by (going clockwise from the top): Ursa Major, Coma Berenices and Boötes.
Canes Venatici is a northern constellation and thus the whole constellation is visible at some point in the year from the whole of the northern hemisphere. The whole of the constellation is also visible from equatorial regions of the southern hemisphere with parts of it visible from temperate southern regions. The constellation is best viewed in the northern hemisphere late spring and southern hemisphere late autumn.
The famous spiral galaxy commonly known as the Whirlpool Galaxy (M51) lies in Canes Venatici and is marked here with a red ellipse. Other notable spiral galaxies in the constellation include M63, M94, M106 and NGC 4631. All are marked here with red ellipses. The globular cluster M3 is marked here with a yellow circle with a plus symbol 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.
Crédito: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope
Link do crédito
Termos do Glossário:
Magnitude aparente , Coordenadas celestes , Constelação , Declinação , Aglomerado Globular , Ascensão Reta (AR) , Galáxia espiral
Categorias
Astronomia a Olho Nu
Licença: Creative Commons Attribution 4.0 International (CC BY 4.0) Creative Commons Attribution 4.0 International (CC BY 4.0) ícones
Arquivo
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93.71 kB)
Arquivo PDF
(PDF file
165.31 kB)
Corona Australis Constellation Map
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Legenda: The constellation Corona Australis with its brighter stars and surrounding constellations. Corona Australis is surrounded by (going clockwise from the top): Sagittarius, Scorpius, Ara and Telescopium. This constellation has relatively few bright stars.
Corona Australis is a southern constellation and thus the whole constellation is visible in the southern hemisphere at some point in the year. The constellation can also be viewed from equatorial and some temperate regions of the northern hemisphere. The constellation is best viewed in the evening in the northern hemisphere summer and southern hemisphere winter.
The globular cluster NGC 6541 lies in Corona Australis 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. The blue line at the top right of the diagram marks the ecliptic.
Crédito: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope
Link do crédito
Termos do Glossário:
Magnitude aparente , Coordenadas celestes , Constelação , Declinação , Eclíptica , Aglomerado Globular , Ascensão Reta (AR) , Escorpião , Sagitário
Categorias
Astronomia a Olho Nu
Licença: Creative Commons Attribution 4.0 International (CC BY 4.0) Creative Commons Attribution 4.0 International (CC BY 4.0) ícones
Arquivo
( imagem
88.22 kB)
Arquivo PDF
(PDF file
158.70 kB)
Lyra Constellation Map
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Legenda: The constellation Lyra with its bright stars and surrounding constellations. Lyra is surrounded by (going clockwise from the top): Draco, Hercules, Vulpecula and Cygnus. Lyra is dominated by its brightest star Vega which is used to define the zero point of one of the most commonly used magnitude scales of stellar brightness. Vega forms one vertex of the prominent Summer Triangle asterism that is visible in northern hemisphere summer evenings.
Lyra is a northern constellation and thus is visible at some point in the year throughout the northern hemisphere. The whole constellation is also visible from all equatorial and some temperate regions of the southern hemisphere. Parts of the constellation are visible from the remaining southern temperate areas. Lyra is best viewed in the evenings in the northern hemisphere summer and southern hemisphere winter.
The famous planetary nebula M57, commonly known as the Ring Nebula, lies in Lyra. It is marked here with a green circle superimposed on a plus sign. The globular cluster M56 also lies in Lyra 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.
Crédito: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope
Link do crédito
Termos do Glossário:
Magnitude aparente , Coordenadas celestes , Constelação , Declinação , Aglomerado Globular , Nebulosa Planetária , Ascensão Reta (AR) , Asterismo
Categorias
Astronomia a Olho Nu
Licença: Creative Commons Attribution 4.0 International (CC BY 4.0) Creative Commons Attribution 4.0 International (CC BY 4.0) ícones
Arquivo
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81.99 kB)
Arquivo PDF
(PDF file
160.41 kB)
