NGC 7475 is a Galaxy Pair in the Pegasus constellation. NGC 7475 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain times of the year. The image below is a photograph of NGC 7475 from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel.

NGC 7475 is a Galaxy located in the constellation of Pegasus in the northern hemisphere. NGC 7475 is called NGC 7475 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to update John Herschel's earlier work. NGC 7475 is not a Messier Object and doesn't have a Messier Number.

NGC 7475 ist ein interagierendes Galaxienpaar im Sternbild Pegasus. Sie ist schätzungsweise 508 Millionen Lichtjahre von der Milchstraße entfernt. Das Objekt wurde am 9. September 1864 von Albert Marth entdeckt. [4]

2022年6月3日 · The SIMBAD astronomical database provides basic data, cross-identifications, bibliography and measurements for astronomical objects outside the solar system.

2024年8月21日 · Physical Information: Based on a recessional velocity of 810 km/sec, NGC 7457 is about 38 million light years away, and although for such a small radial velocity, peculiar (non-Hubble expansion) velocities could considerably alter the result, the value is in good agreement with redshift-independent distance estimates of 38 to 43 million light ...

NGC 7474/7475-1,2 Pegasus Penryn, California September 2007 FS-128G (ag, ST-4) ST-2000XM LRGB 5 minutes subs. NGC 7474 is the type SO at lower center and NGC 7475-1 and NGC 7475-2 are the interacting duo at the center position. The galaxies are dimmed considerably by the pervasive galactic dust in the constellation of Pegasus

< NGC List NGC 7475 NED02 NGC 7475 NED02 is a galaxy located in the constellation of Pegasus. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 7475 NED02:

NGC 7475 est une paire de galaxies elliptiques relativement éloignée, située dans la constellation de Pégase. La vitesse de la paire par rapport au fond diffus cosmologique est de 10 821 ± 43 km/s, ce qui correspond à une distance de Hubble de 159,6 ± 11,2 Mpc (∼521 millions d' al) 2.

Sulentic & Tifft (1973) The RNGC (Sulentic and Tifft 1973) notes that this is a 15.0 mag galaxy. Their coded description reads SYST OF4,E,R,BM+3COM 2STEL OBJ P &1 NF.

Articoli relazionati The UZC-SSRS2 Group CatalogWe apply a friends-of-friends algorithm to the combined Updated ZwickyCatalog and Southern Sky Redshift Survey to construct a catalog of 1168groups of galaxies; 411 of these groups have five or more members withinthe redshift survey. The group catalog covers 4.69 sr, and all groupsexceed the number density contrast threshold, δρ/ρ=80 ...