NGC 4197 is a Intermediate Spiral Galaxy in the Virgo constellation. NGC 4197 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.

From Virginia Beach , NGC4197 is visible in the morning sky, becoming accessible around 22:24, when it reaches an altitude of 21° above your eastern horizon. It will then reach its highest point in the sky at 02:52, 58° above your southern horizon. It will be lost to dawn twilight around 05:51, 38° above your south-western horizon.

NGC 4197 (NGC4197) is a galaxy that has a distance from Earth of 90,593,195.47 light years. It can be found in the constellation of Virgo.

Media in category "NGC 4197" The following 2 files are in this category, out of 2 total.

2022年1月27日 · NGC 4197 -- HII Galaxy The astronomical object called NGC 4197 is a HII Galaxy: Origin of the objects types : (Ref) Object type as listed in the reference "Ref" (acronym) Object type linked to the acronym according to the original reference Anterior to 2007, before we can link the objet type to a reference, or given by the CDS team in some ...

对象 NGC 4197 正好位于图片的中心. NGC 4197 - 星系 在星座 室女座 类型: Sc - 螺旋星系 角度尺寸: 3.40'x0.6' 恒星的大小: V=12.8 m; B=13.5 m 表面亮度: 13.5 mag/arcmin 2 这个时代的坐标 J2000: Ra= 12 h 14 m 38.6 s; Dec= 5°48'22" 红移 (z): 0.006885 从太阳距离 NGC 4197: 基于红移值 (z) - 29.1 MPC;

NGC 4197 (također poznat kao IRAS 12121+0605, MCG 1-31-29, PGC 39114 i UGC 7247) je spiralna galaksija koja je udaljena oko 95 miliona sg od Zemlje i nalazi se u sazviježđu Djevica. Najveći prečnik je 3,40 (94 hiljade sg) a najmanji 0,6 uglovnih minuta (17 hiljada sg).

NGC 4197. 0 references. Identifiers. Google Knowledge Graph ID /g/12226tts. 0 references. New General Catalogue ID. 4197. 0 references. Principal Galaxies Catalogue ID. 39114. 0 references. SIMBAD ID. NGC 4197. 1 reference. imported from Wikimedia project. Polish Wikipedia. Uppsala General Catalogue ID. 7247.

HI content in galaxies in loose groups Gas deficiency in cluster spirals is well known and ram-pressurestripping is considered the main gas removal mechanism.

NGC 4197 — Yeni Ümumi Kataloqda qeydə alınmış qalaktika. Göy üzündə Qız bürcü istiqamətində yerləşir. Sc tipli qalaktikadır. İngilis astronomu Vilyam Herşel tərəfindən 1784-cü ildə 47.5 sm (18.7 düymə) ölçülü reflektor vasitəsilə kəşf edilmişdir. [6]