NGC 6602 is a Spiral Galaxy located in the constellation of Hercules in the northern hemisphere. NGC 6602 is called NGC 6602 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to …

NGC 6602 is a Intermediate Spiral Galaxy in the Hercules constellation. NGC 6602 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 14.6, NGC 6602 is visible with the help of a telescope having an aperture of 20 inches (500mm) or more.

NGC 6602 -- Galaxy The astronomical object called NGC 6602 is a 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 particular ...

NGC 6602, yew cısmê asmêniyo. No cısım Katalogê Neweyê Pêroyi de, komê estareyan ê Herkules miyan de ca gêno. 1 Temuz 1886 de terefê Guillaume Bigourdani ra keşıf biyo.

Guides to the night sky. Location: Redmond (47.67°N; 122.12°W) NGC6602 (Galaxy)

Revised NGC Data for NGC 6602 Data from Wolfgang Steinicke's Revised NGC and IC Catalog. Object: NGC 6602 (*) Galaxy, type SB?, in Hercules Right Ascension (2000.0): 18:16:34.2 …

Object NGC 6602 is located exactly in the center of the picture. NGC 6602 - galaxy in the constellation Herculis Type: SB? - spiral galaxy with bar The angular dimensions: 1.00'x0.7' magnitude: V=13.8 m; B=14.6 m The surface brightness: 13.3 mag/arcmin 2 Coordinates for epoch J2000: Ra= 18 h 16 m 34.2 s; Dec= 25°2'37" redshift (z): 0.010270

ngc 6602 في الفهرس العام الجديد، هي مجرة، تقع في كوكبة الجاثي. اكتشفت في 1 يوليو 1886 .

NGC 6602 este o galaxie situată în constelația Hercule. [2] [3] [4] A fost descoperită în 1 iulie 1886 de către Guillaume Bigourdan ⁠(d). [5]

NGC 6602 est une galaxie spirale intermédiaire située dans la constellation d'Hercule. Sa vitesse par rapport au fond diffus cosmologique est de 2 930 ± 8 km/s [1], ce qui correspond à une distance de Hubble de 43,2 ± 3,0 Mpc (∼141 millions d'al) [1].