NGC 1956 - Spiral Galaxy in Mensa
NGC 1956 is a Spiral Galaxy in the Mensa constellation. NGC 1956 is situated close to the southern celestial pole and, as such, it is easilty visible for most part of the year from the southern hemisphere.
See also NGC 1956 rise and set times.
Given its B magnitude of 14.05, NGC 1956 is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.
Photometric information of NGC 1956
The following table lists the magnitude of NGC 1956 in different bands of the electomagnetic spectrum (when available), from the B band (445nm wavelength, corresponding to the Blue color), to the V band ( 551nm wavelength, corresponding to Green/Yellow color), to the J, H, K bands (corresponding to 1220nm, 1630nm, 2190nm wavelengths respectively, which are colors not visible to the human eye).
For more information about photometry in astronomy, check the photometric system article on Wikipedia.
The surface brightess reported below is an indication of the brightness per unit of angular area of NGC 1956.
Apparent size of NGC 1956The following table reports NGC 1956 apparent angular size. The green area displayed on top of the DSS2 image of NGC 1956 is a visual representation of it.
Digitized Sky Survey image of NGC 1956
The image below is a photograph of NGC 1956 from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the image is 0.5x0.5 degrees (30x30 arcmins).
NGC 1956 - Spiral Galaxy in Mensa morphological classification
NGC 1956 - Spiral Galaxy in Mensa is classified as Spiral (SAa) according to the Hubble and de Vaucouleurs galaxy morphological classification. The diagram below shows a visual representation of the position of NGC 1956 - Spiral Galaxy in Mensa in the Hubble de Vaucouleurs sequence.
Celestial coordinates and finder chart of NGC 1956
Celestial coordinates for the J2000 equinox of NGC 1956 are provided in the following table:
The simplified sky charts below show the position of NGC 1956 in the sky. The first chart has a field of view of 60° while the second one has a field of view of 10°.