NGC 4965 is a Intermediate Spiral Galaxy in the Hydra constellation. NGC 4965 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its B magnitude of 12.76, NGC 4965 is visible with the help of a telescope having an aperture of 10 inches (250mm) or more.

From Virginia Beach , NGC4965 is visible in the morning sky, becoming accessible around 03:50, when it reaches an altitude of 21° above your southern horizon. It will then reach its highest point in the sky at 05:14, 24° above your southern horizon. It will be lost to dawn twilight around 06:07, 23° above your southern horizon.

NGC 4965 -- Emission-line galaxy The astronomical object called NGC 4965 is a Emission-line 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 ...

NGC 4965 (također poznat kao ESO 443-70, IRAS 13044-2757, MCG -5-31-36, PGC 45437 i UGCA 326) je prečkasta spiralna galaksija koja je udaljena oko 104 miliona sg od Zemlje i nalazi se u sazviježđu Vodena zmija. Najveći prečnik je 2,40 (73 hiljade sg) a najmanji 2,0 uglovnih minuta (61 hiljada sg).

The Carnegie-Irvine Galaxy Survey (CGS) Data Products . Images • summary from image atlas • original FITS images (B, V, R, I) • color-composite image (original) • color-composite image (star-cleaned) • stacked image • structure maps (B, V, R, I) • color index maps (B-R, R-I) Radial Profiles

Spiral galaxies observed in the near-infrared K band. I. Data analysis and structural parameters Deep surface photometry in the K band was obtained for 54 normal spiralgalaxies, with the aim of quantifying the percentage of faint bars andstudying the morphology of spiral arms.

NGC 4965 (NGC4965) is a emission-line galaxy that is 125951808.37 light years away from Earth in the constellation of Hydra.

NGC 4965 Gidra yulduz turkumidagi SBcd tipli galaktikadir. Ushbu obyektni John Herschel 1834-yilda kashf etgan. Ushbu obyekt Yangi umumiy katalog asl nashrida mavjud.

NGC 4965 é uma galáxia espiral barrada (SBcd) localizada na direcção da constelação de Hydra. Possui uma declinação de -28° 13' 42" e uma ascensão recta de 13 horas, 07 minutos e 09,2 segundos. A galáxia NGC 4965 foi descoberta em 5 de Maio de 1834 por John Herschel.

NGC 4965 este o emission-line galaxy ⁠(d) situată în constelația Hidra. [4] [5] [6] A fost descoperită în 5 mai 1834 de către John Herschel. [7]