NGC 5473 is a lenticular galaxy in the constellation Ursa Major. It was discovered on April 14, 1789, by the astronomer William Herschel. [6] Located roughly 85 million light-years (26.2 megaparsecs) away, it is part of a small galaxy group including NGC 5475 and NGC 5485. [3]

NGC 5473 is a Barred Spiral Galaxy located in the constellation of Ursa Major in the northern hemisphere. NGC 5473's distance from Earth is 88,933,059.51 light years. NGC 5473 is called NGC 5473 in the New General Catalogue (NGC).

NGC 5473 is a Elliptical/Spiral Galaxy in the Ursa Major constellation. NGC 5473 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 12.5, NGC 5473 is visible with the help of a telescope having an aperture of 10 inches (250mm) or more.

We present detailed 2D maps of stellar population properties, i.e., age, metallicity, extinction, and stellar mass surface density, for two early-type galaxies observed in the J-PLUS and CALIFA surveys. These galaxies are NGC 5473 and NGC 5485. Radial structures are also compared and luminosity- and mass-weighted profiles are derived.

2018年4月10日 · We present detailed 2D maps of stellar population properties (age, metallicity, extinction, and stellar mass surface density) for two early-type galaxies observed in both, J-PLUS and CALIFA surveys: NGC 5473 and NGC 5485. Radial structures are also compared and luminosity- and mass-weighted profiles are derived.

From Virginia Beach , NGC5473 is visible in the morning sky, becoming accessible around 22:54, when it reaches an altitude of 21° above your north-eastern horizon. It will then reach its highest point in the sky at 05:52, 71° above your northern horizon. It will be lost to dawn twilight at around 06:05, 71° above your northern horizon.

Visual Observation Notes:- NGC 5473. Fairly small. Bright star-like core surrounded by a faint oval halo. Very faint star east of core. Sevaral brighter stars surrounding the galaxy. 18" f/5 newtonian. 16mm nagler eyepiece. 143x. Sky View observatory. Zenith limiting magnitude 6.7.

NGC 5473 est une galaxie lenticulaire située dans la constellation de la Grande Ourse. Sa vitesse par rapport au fond diffus cosmologique est de 2 140 ± 10 km/s, ce qui correspond à une distance de Hubble de 32,6 ± 2,2 Mpc (∼106 millions d'al) [1]. NGC 5473 a été découverte par l'astronome germano-britannique William Herschel en 1789.

Radio sources in low-luminosity active galactic nuclei. IV. Radio luminosity function, importance of jet power, and radio properties of the complete Palomar sample

TV#073 M101, NGC: 5473, 5474,5485,5422 Equipment Acquisition details Comments. Sky plot. Histogram. In these collections 1. All Images AL - Two in the View Messier Catalogue About. AstroBin is an image hosting platform and social network for amateur astronomers and astrophotographers. ...