In today's article, we are going to delve into the fascinating world of Cetus Dwarf. Whatever your interest or concern, we are sure that you will find relevant and useful information that will help you better understand this topic. From its origins to its evolution today, we will dive into key aspects that will allow you to gain a deeper knowledge about Cetus Dwarf. Regardless of whether you are an expert in the field or if you are just beginning to explore this topic, this article aims to provide a comprehensive and enriching vision that allows you to broaden your horizons and enrich your perspective on Cetus Dwarf. Get ready to embark on a journey of discovery and learning that will pleasantly surprise you!
| Cetus Dwarf | |
|---|---|
Cetus Dwarf with legacy surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 00h 26m 11.0s[1] |
| Declination | −11° 02′ 40″[1] |
| Distance | 2.46 ± 0.08 Mly (755 ± 24 kpc)[2] |
| Apparent magnitude (V) | 14.4[1] |
| Characteristics | |
| Type | dSph[1] |
| Apparent size (V) | 5.0′ × 4.3′[1] |
| Other designations | |
| PGC 3097691[1] | |

Cetus Dwarf is a dwarf spheroidal galaxy. It lies approximately 2.46 Million light-years from Earth. It is an isolated galaxy of the Local Group, which also contains the Milky Way.[3] All of the most readily observable stars in the galaxy are red giants.[4]
The Cetus Dwarf was discovered in 1999 by Alan B. Whiting, George Hau and Mike Irwin and was found to be a member of the Local Group.[2][5]
As of 2000, no known neutral hydrogen gas has been found that is related to the Cetus dwarf galaxy.[5]