NGC 988 is a spiral galaxy located in the constellation Cetus. [4] It lies at a distance of 50 million light years from Earth, which, given its apparent dimensions, means that NGC 988 is about 75,000 light years across. The magnitude 7.1 star HD 16152 is superposed 52" northwest of the center of NGC 988.

ngc 988 是鲸鱼座的一個星系。 维基共享资源上的相關多媒體資源：ngc 988. ned – ngc 988; seds – ngc 988; simbad – ngc 988; vizier – ngc 988

A peculiar galaxy's debut on Astrobin, NGC 988 is a barred spiral galaxy in the southern part of the constellation Cetus. It is actually quite large in angular size, allowing for great detail to be re...

NGC 988 is a Spiral Galaxy in the Cetus constellation. NGC 988 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 11.73, NGC 988 is visible with the help of a telescope having an aperture of 8 inches (200mm) or more.

NGC 988 is an Barred Spiral Galaxy located in the constellation of Cetus in the equatorial region. NGC 988's distance from Earth is 49,820,386.69 light years. NGC 988 is called NGC 988 in the New General Catalogue (NGC).

The Carnegie-Irvine Galaxy Survey (CGS) Data Products . Images • summary from image atlas • original FITS images (B, V, R, I) • color-composite image (original) • color-composite image (star-cleaned) • stacked image • structure maps (B, V, R, I) • color index maps (B-R, R-I) Radial Profiles

The structure of galactic disks. Studying late-type spiral galaxies using SDSS Using imaging data from the SDSS survey, we present the g' and r' radialstellar light distribution of a complete sample of ~90 face-on tointermediate inclined, nearby, late-type (Sb-Sdm) spiral galaxies.

2022年10月8日 · NGC 988 -- Emission-line galaxy The astronomical object called NGC 988 is a Emission-line 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 ...

NGC 988 . NGC 988 is a late spiral galaxy located in the constellation Cetus. Some key stats include:

NGC 988 是 鲸鱼座 的一个 星系。 维基共享资源 上的相关多媒体资源： NGC 988.

NGC988 is a small galaxy lying near a border to Eridanus in eastern edge of Cetus. The galaxy has a long axis of a bit larger than 5 arc minutes and barred shape with 11th magnitude in brightness. You can detect a 7th magnitude inner-galactic star being on top of the galaxy. Copyright (c) 2012 by Naoyuki Kurita, All rights reserved.

NGC 988 是 鯨魚座 的一個 星系。

From Virginia Beach , NGC988 is not observable – it will reach its highest point in the sky during daytime and is no higher than 18° above the horizon at dusk. "Uppsala General Catalogue of …

NGC 988 - galaxy in the constellation Ceti Type: SBc - spiral galaxy with bar The angular dimensions: 4.10'x1.6' magnitude: V=11.0 m; B=11.4 m The surface brightness: 13.5 mag/arcmin 2 Coordinates for epoch J2000: Ra= 2 h 35 m 27.3 s; Dec= -9°21'18" redshift (z): 0.005037 The distance from the Sun to NGC 988: based on the amount of redshift (z ...

An astrophotograph by OklahomAstro on AstroBin

Q1040741 SIMBAD ID: NGC 988. The following 2 files are in this category, out of 2 total.

撮影メモ： くじら座の東の外れのエリダヌス座との境界付近に位置する小型の系外星雲です。 長径が5分強，明るさが11等級の棒渦巻型をしています。 銀河本体の上に，7等級の銀河系内の恒星が重なっています。 御意見，御感想をお聞かせください。 →メールはこちらまで・・・ Copyright (c) 2012 by Naoyuki Kurita, All rights reserved.

NGC 988 (također poznat kao IRAS 02330-0934, MCG -2-7-37, PGC 9843 i UGCA 35) je prečkasta spiralna galaksija koja je udaljena oko 69 miliona sg od Zemlje i nalazi se u …

NGC 988 est une galaxie spirale barrée située dans la constellation de la Baleine. Sa vitesse par rapport au fond diffus cosmologique est de 1 288 ± 16 km/s, ce qui correspond à une distance de Hubble de 19,0 ± 1,4 Mpc (∼62 millions d' al) 1. NGC 988 a été découverte par l'astronome français Édouard Stephan en 1880.

NGC 988 ha una classe di luminosità III-IV e presenta una larga riga a 21 cm dell'idrogeno neutro. [2] Nella galassia sono presenti anche regioni di idrogeno ionizzato. [2]Nelle immagini, proprio davanti alla galassia è situata prospetticamente la stella SAO 129994, la quale con la sua luminosità nasconde la porzione nordoccidentale della galassia.