ngc 1062 是三角座的一粒恆星，由羅夫·科普蘭於1873年10月11日記錄，後收錄入天體新總表（ ngc ），但是科普蘭將此恆星誤認為一團暗淡的星雲狀物。 有天體表將螺旋星系PGC 10331列為NGC 1062，但這與科普蘭原先觀察的數據（相對於 NGC 1061 的位置）有出入。

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NGC 1062 is a Star in the Triangulum constellation. NGC 1062 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. The image below is a photograph of NGC 1062 from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the ...

2022年3月13日 · NGC 1062 is a Spiral Galaxy located in the constellation of Triangulum in the northern hemisphere. NGC 1062 is called NGC 1062 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to update John Herschel's earlier work.

===== NGC 1062 is a star found by Copeland in the NGC 1061 group (actually in the core of an extended cluster of galaxies) with Lord Rosse's 72-inch "Leviathan." The offsets from NGC 1061 measured by him fall precisely on a faint star, so the identity is certain.

NGC 1062是一个位于三角座的星系，发现者是罗夫·科普兰，发现日期为1873年10月11日。

Historical Identification: As discussed at the entry for NGC 1062, overzealous efforts to find a nebular object to assign to NGC 1062 (which is actually a star) led to PGC 10331 being mistakenly listed as that object in some catalogs, and the error still persists in places. Hence this entry, serving as a warning about the misidentification.

ngc 1062 是三角座的一粒恆星，由羅夫·科普蘭於1873年10月11日記錄，後收錄入天體新總表（ ngc ），但是科普蘭將此恆星誤認為一團暗淡的星雲狀物。 有天體表將螺旋星系PGC 10331列為NGC 1062，但這與科普蘭原先觀察的數據（相對於 NGC 1061 的位置）有出入。

2022年2月2日 · NGC 1057 - 1067 - posted in Experienced Deep Sky Imaging: This is a really nice field of galaxies located in Triangulum. See the annotated image link. Note that NGC 1062 is really the galaxy labeled PGC 10331.

The UZC-SSRS2 Group Catalog We apply a friends-of-friends algorithm to the combined Updated ZwickyCatalog and Southern Sky Redshift Survey to construct a catalog of 1168groups of galaxies; 411 of these groups have five or more members withinthe redshift survey.