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- North_polar_sequence abstract "The North polar sequence is a group of 96 stars that was used to define stellar magnitudes and colors. The cluster of stars lies within two degrees of the Northern Celestial pole, which makes them visible to everyone on the northern hemisphere.Originally proposed by Edward Charles Pickering, the system was used between 1900 and 1950. Today it has been replaced by the UBV photometric system.".
- North_polar_sequence wikiPageExternalLink books?id=tZpQR_nYKeYC&pg=PA446.
- North_polar_sequence wikiPageExternalLink north-polar-sequence.html.
- North_polar_sequence wikiPageID "24379121".
- North_polar_sequence wikiPageLength "766".
- North_polar_sequence wikiPageOutDegree "8".
- North_polar_sequence wikiPageRevisionID "604568993".
- North_polar_sequence wikiPageWikiLink Apparent_magnitude.
- North_polar_sequence wikiPageWikiLink Category:Photometric_systems.
- North_polar_sequence wikiPageWikiLink Celestial_pole.
- North_polar_sequence wikiPageWikiLink Edward_Charles_Pickering.
- North_polar_sequence wikiPageWikiLink Northern_Hemisphere.
- North_polar_sequence wikiPageWikiLink Northern_hemisphere.
- North_polar_sequence wikiPageWikiLink Photometric_system.
- North_polar_sequence wikiPageWikiLink Stellar_classification.
- North_polar_sequence wikiPageWikiLink Stellar_magnitude.
- North_polar_sequence wikiPageWikiLink UBV_photometric_system.
- North_polar_sequence wikiPageWikiLinkText "North polar sequence".
- North_polar_sequence hasPhotoCollection North_polar_sequence.
- North_polar_sequence wikiPageUsesTemplate Template:Astronomy-stub.
- North_polar_sequence wikiPageUsesTemplate Template:Star.
- North_polar_sequence wikiPageUsesTemplate Template:Unreferenced.
- North_polar_sequence subject Category:Photometric_systems.
- North_polar_sequence hypernym Group.
- North_polar_sequence type Article.
- North_polar_sequence type Band.
- North_polar_sequence type Article.
- North_polar_sequence comment "The North polar sequence is a group of 96 stars that was used to define stellar magnitudes and colors. The cluster of stars lies within two degrees of the Northern Celestial pole, which makes them visible to everyone on the northern hemisphere.Originally proposed by Edward Charles Pickering, the system was used between 1900 and 1950. Today it has been replaced by the UBV photometric system.".
- North_polar_sequence label "North polar sequence".
- North_polar_sequence sameAs m.07s8psd.
- North_polar_sequence sameAs Северный_полярный_ряд.
- North_polar_sequence sameAs Північний_полярний_ряд.
- North_polar_sequence sameAs Q4412390.
- North_polar_sequence sameAs Q4412390.
- North_polar_sequence sameAs 北极星序.
- North_polar_sequence wasDerivedFrom North_polar_sequence?oldid=604568993.
- North_polar_sequence isPrimaryTopicOf North_polar_sequence.