NGC 4316 is an edge-on spiral galaxy located about 70 million light-years away [2] in the constellation Virgo.It was discovered by astronomer Wilhelm Tempel on March 17, 1882. [3] NGC 4316 is a member of the Virgo Cluster [4] [5] and is classified as LINER and as a Seyfert galaxy. [2] [6]The galaxy has undergone ram-pressure stripping in the past. [7]On February 28, 2003 a type II supernova ...

NGC 4316 is a Spiral Galaxy in the Virgo constellation. NGC 4316 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. Given its B magnitude of 14, NGC 4316 is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

2024年7月1日 · Per Dreyer, NGC 4316 (Tempel list V (#17), 1860 RA 12 15 34, NPD 79 53.4) is "very faint, small, much extended, 2 knots". (A critical reference for the identification of NGC 4315.) Apparent size 2.5 by 0.5 arcmin. Listed as a member (VCC 576) of the Virgo Cluster.

NGC 4316 (NGC4316) is a galaxy that has a distance from Earth of 90,909,567.15 light years. It can be found in the constellation of Virgo.

NGC 4316 -- Galaxy towards a Group of Galaxies The astronomical object called NGC 4316 is a Galaxy towards a Group of Galaxies Origin of the objects types :

NGC 4316 galaxy. NGC 4316 is a galaxy in the Virgo Cluster. The Virgo Cluster spans the constellations of Virgo and Coma Berenices and contains approximately 2,000 galaxies, including a number of Messier objects.

NGC 4316 Galaxy in Virgo Dreyer's description: vF, S, mE, 2 knots . Cross Identifications: Tempel V, Stephan XIII.

Revised NGC Data for NGC 4316 Data from Wolfgang Steinicke's Revised NGC and IC Catalog. Object: NGC 4316 (*) Galaxy, type Sc, in Virgo Right Ascension (2000.0): 12:22:42.1 (h:m:s) Declination (2000.0): +09:19:57 (deg:m:s) m_b: 13.8 (mag) , m_v: 13.1 (mag) , SB: 13.2 (mag per square arcmin) Dimension: 2.50 x 0.5 (arcmin) , PA: 113

NGC 4316 est une galaxie spirale vue par la tranche et située dans la constellation de la Vierge. Sa vitesse par rapport au fond diffus cosmologique est de 1 589 ± 24 km/s, ce qui correspond à une distance de Hubble de 23,4 ± 1,7 Mpc (∼76,3 millions d' al) 1. Elle a été découverte par l'astronome allemand Wilhelm Tempel en 1882.

Media in category "NGC 4316" The following 2 files are in this category, out of 2 total.