NGC 4226 is a Barred Spiral Galaxy in the Canes Venatici constellation. NGC 4226 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 14.36, NGC 4226 is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

NGC 4226 is a Radio Galaxy located in the constellation of Canes Venatici in the northern hemisphere. NGC 4226's distance from Earth is 388,126,089.46 light years. NGC 4226 is called NGC 4226 in the New General Catalogue (NGC).

NGC 4226 was discovered by John Herschel on 19 March 1828. With an angular extent of about 1.0 x 0.5 arc minutes, it is quite small and is only 14 magnitudes bright. The galaxy appears to have a bar-spiral structure.

2023年8月14日 · Added Caldwell ID to NGC 4236, and updated and completed the entry. Physical Information: Based on a recessional velocity of 2375 km/sec, NGC 4200 is about 110 million light-years away. Given that and its apparent size of 1.5 by 0.9 arcmin, it is about 50 thousand light-years across.

2024年12月26日 · NGC 4226 is a Barred Spiral Galaxy in the Canes Venatici constellation. NGC 4226 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 14.36, NGC 4226 is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

NGC 4226 est une galaxie spirale située dans la constellation des Chiens de chasse. Sa vitesse par rapport au fond diffus cosmologique est de 7 455 ± 15 km/s, ce qui correspond à une distance de Hubble de 110,0 ± 7,7 Mpc (∼359 millions d' al) 1. NGC 4226 a été découverte par l'astronome britannique John Herschel en 1828.

NGC 4226 este o galaxie spirală situată în constelația Câinii de Vânătoare. [7] [8] [9] A fost descoperită în 19 martie 1828 de către John Herschel. [10] Se află la o distanță de 121,9 de megaparseci de Pământ. [11] [12]

2025年1月22日 · Data at NED - NASA/IPAC Extragalactic Database : NGC 4226. Link by name to the catalogue in VizieR:

2017年8月16日 · NGC 4217（銀河）, 光度：11.2 mag, 直径：5.2′ x 1.5′, 分類：Sb 距離6000万光年の位置にある渦状銀河で、おそらくM106の伴星雲です。 この銀河の暗黒帯の構造はHSTで詳しく調べられ塵のフィラメント構造などがみつかっています。

NGC 4226 Galaxy in Canes Venatici Dreyer's description: F, S, lE, f of 2 . Cross Identifications: GC 2816, h 1155.