NGC 151 is a mid-sized barred spiral galaxy [3] located in the constellation Cetus. The galaxy was discovered by English astronomer William Herschel on November 28, 1785. In 1886, Lewis Swift observed the same galaxy and catalogued it as NGC 153 , only for it …

ngc 151 (ngc 153, mcg -2-2-54,iras00315-0958)是鲸鱼座的一個星系。 星等 為11.6， 赤經 為34分2.8秒， 赤緯 為-9°42'18"。 在1785年11月28日被 約翰·弗里德里希·威廉·赫歇爾 發現。

NGC 151 is a Spiral Galaxy in the Cetus constellation. NGC 151 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 visual magnitude of 11.59, NGC 151 is visible with the help of a telescope having an aperture of 8 inches (200mm) or more.

6 天之前 · NGC 151 is an Active Galactic Nuclei/Nucleus located in the constellation of Cetus in the equatorial region. NGC 151's distance from Earth is 125,733,283.60 light years. NGC 151 is called NGC 151 in the New General Catalogue (NGC).

NGC151 is a 12th magnitude barred galaxy located at 8.5 degrees NNW of βCet (Deneb Kaitos). The galaxy has a slightly asymmetrical spiral structure with a major axis of about 4 arc minutes. Its estimated distance is approximately 170 million light-years. Copyright (c) 2023 by Naoyuki Kurita, All rights reserved.

ngc 151是位于鲸鱼座的一个星系。它的赤经为 0 34，赤纬为 -9° 42′，大小 3.7′。

NGC 151 . NGC 151 is a spiral galaxy located in the constellation Cetus. Some key stats include:

NGC 151 is a fainter member of the Sculptor group of galaxies that includes the more well known NGC 55 and NGC 253. The total magnitude is around 12.3, and the galaxy is readily visible in an 8" telescope under dark skies as a round, nebulous patch with a slightly brighter centre.

2022年12月4日 · NGC 151 is quite a small target in the field of view. It is a medium sized barred spiral galaxy with active areas of star formation. It is located 170 million light years away in Cetus. Imaged in LRGB on our Planewave CDK 1000 at Observatorio El Sauce, Chile. Proudly powered by …

2014年2月24日 · This galaxy's purple-like appearance indicates the bluish spiral arms have many reddish dust lanes and HII regions. However, at a distance of 160 million light years away, these details are not well resolved in this image. This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.