NGC 3110, also known as NGC 3122 and NGC 3518, is an active spiral galaxy in the constellation Sextans. [1][2] It contains extensive Hubble-type Sb star-forming regions, and is located south of the celestial equator. [3] It is estimated to be 218 million light-years from the Milky Way and has a diameter of around 100,000 ly.

2023年9月11日 · Physical Information: Since NGC 3518 is an erroneous and duplicate observation of NGC 3110, see the corresponding entry for its probable companion following NGC 3110's entry.

Data from Wolfgang Steinicke 's Revised NGC and IC Catalog Object: NGC 3518 (*) Duplicate NGC/IC Object, type Sb, in Sextans Right Ascension (2000.0): 10:04:01.9 (h:m:s) Declination (2000.0): -06:28:29 (deg:m:s) m_b: 13.5 (mag) , m_v: 12.7 (mag) , SB: 12.8 (mag per square arcmin) Dimension: 1.60 x 0.8 (arcmin) , PA: 162 Cross Identifications: NGC 3110, NGC 3122, MCG -1-26-14, PGC 29192 ...

NGC 3718, also called Arp 214, is a galaxy located approximately 52 million light years from Earth in the constellation Ursa Major. [4][2][5] It is either a lenticular or spiral galaxy.

NGC 3518 NGC 3518 is a duplicate located in the constellation Sextans. Some key stats include: ... Right Ascension units = HH:MM:SS.SS Declination units = DD:MM:SS.SS PN = planetary …

duplicate of the galaxy NGC 3110

The following is a list of NGC objects, that is objects listed in the New General Catalogue (NGC). It is one of the largest comprehensive astronomical catalogues for deep sky objects such as star clusters, nebulae, and galaxies.

Please type in the NGC number (number only, or preceded by "N" or "NGC") or the IC number preceded by "I" or "IC", or the Messier number preceded by "M".

NGC 3718 est une vaste galaxie spirale barrée située dans la constellation de la Grande Ourse. Sa vitesse par rapport au fond diffus cosmologique est de 993 ± 1 km/s, ce qui correspond à une distance de Hubble de 17,36 ± 1,23 Mpc (∼56,6 millions d' al) 1.

NGC 3522 Arslon yulduz turkumidagi E (elliptik galaktika) tipli galaktikadir [1]. Ushbu obyektni Lewis Swift 1883-yilda kashf etgan. Ushbu obyekt Yangi umumiy katalog asl nashrida mavjud [2].