NGC 4175 is an Active Galactic Nuclei/Nucleus located in the constellation of Coma Berenices in the northern hemisphere. NGC 4175's distance from Earth is 137,637,991.39 light years. NGC 4175 is called NGC 4175 in the New General Catalogue (NGC).

The galaxy NGC 4175 in the west of the group of four is a spiral galaxy of type S or Sb, roughly like M 31. The angle of inclination is 86 degrees, so we are almost looking at the edge. Their escape speed is somewhat higher with about 3900 km/s relative to the local group, which equates to a distance of 170 million light years. [134]

NGC 4175 is a Barred Spiral Galaxy in the Coma Berenices constellation. NGC 4175 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its visual magnitude of 13.45, NGC 4175 is visible with the help of a telescope having an aperture of 10 inches (250mm) or more.

NGC 4175 is 14.3-magnitude edge-on spiral that shows evidence of interaction with a neighbor. At 260x this galaxy appeared as an elongated haze. Finally, NGC 4173 is the largest of the four, but the most difficult. Another interacting spiral galaxy, this 13.8 magnitude galaxy has a very low mean surface brightness of 23.7 mag/arc-sec 2.

2018年4月11日 · Hickson 61, also known as "The Box" galaxy group is located in Coma Berenices. The large bluish irregular spiral NGC 4173, elliptical NGC 4169, the small NGC 4174 and edge-on NGC 4175 compose the box. NGC 4173 is at a closer distance of 50 mly and is a foreground galaxy. The other three at 180 mly are likely physically related.

NGC 4175 is a magnitude 14.3 edge-on spiral that shows evidence of interaction with its apparent neighbor, NGC 4173, which is the largest of the four but the most difficult to see because of its low surface brightness.

2023年9月14日 · The SIMBAD astronomical database provides basic data, cross-identifications, bibliography and measurements for astronomical objects outside the solar system.

2012年6月13日 · NGC 4175 was very long (4:1) with a slight central concentration and slightly brighter nucleus, but overall it appeared much fainter than the two western galaxies. Finally, NGC 4173 was the real phantom. Very long (5:1) and very faint, with a very low surface brightness and practically no central brightening.

NGC 4175 - galaxy in the constellation Comae Berenices Type: Sbc - The angular dimensions: 1.80'x0.4' magnitude: V=13.3 m; B=14.2 m The surface brightness: 12.8 mag/arcmin 2 Coordinates for epoch J2000: Ra= 12 h 12 m 31 s; Dec= 29°10'7" redshift (z): 0.013384 The distance from the Sun to NGC 4175: based on the amount of redshift (z) - 56.5 Mpc ...

From Virginia Beach , NGC4175 is visible in the morning sky, becoming accessible around 22:12, when it reaches an altitude of 21° above your eastern horizon. It will then reach its highest point in the sky at 03:44, 82° above your southern horizon. It will be lost to dawn twilight around 06:02, 60° above your western horizon.