NGC 1775 is a Open Cluster in the Mensa constellation. NGC 1775 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual magnitude of 12.55, NGC 1775 is visible with the help of a telescope having an aperture of 10 inches (250mm) or more.

< NGC List NGC 1775. NGC 1775 is a open cluster located in the constellation of Mensa. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 1775:

Media in category "NGC 1775" The following 2 files are in this category, out of 2 total.

Association of clusters in the constellation of Mensa In this image we can see several star clusters such as NGC1845, NGC 1833, NGC 1837, NGC 1813, NGC 1815, NGC 1791 and NGC 1775. PROCESSING AND CAPTURE: Adobe Photoshop, ASTAP, SGP, PHD2 and PixInsight

NGC 1775 est un amas ouvert situé dans la constellation de la Table. Cet amas est situé dans le Grand Nuage de Magellan. Il a été découvert par l'astronome britannique John Herschel en 1836.

NGC 1775 Mensa yulduz turkumidagi OCL (ochiq klaster) tipli ochiq klasterdir. Ushbu obyektni John Herschel 1836-yilda kashf etgan. Ushbu obyekt Yangi umumiy katalog asl nashrida mavjud.

Revised NGC Data for NGC 1775 Data from Wolfgang Steinicke's Revised NGC and IC Catalog. Object: NGC 1775 (*) Open Cluster, type OCL, in Mensa Right Ascension (2000.0): 04:56:53.4 …

2024年3月12日 · NGC 1775 -- Cluster of Stars The astronomical object called NGC 1775 is a Cluster of Stars: 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 ...

Language Label Description Also known as; English: NGC 1775. star cluster

Infrared Surface Brightness Fluctuations of Magellanic Star Clusters We present surface brightness fluctuations (SBFs) in the near-IR for 191Magellanic star clusters available in the Second Incremental and All SkyData releases of the Two Micron All Sky Survey (2MASS) and compare themwith SBFs of Fornax Cluster galaxies and with predictions from stellarpopulation models as well.