IC 1211 - Elliptical Galaxy
IC 1211 is a Elliptical Galaxy in the Draco constellation. IC 1211 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere.
Photometric information of IC 1211
The following table lists the magnitude of IC 1211 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 IC 1211.
Apparent size of IC 1211The following table reports IC 1211 apparent angular size. The green area displayed on top of the DSS2 image of IC 1211 is a visual representation of it.
Digitized Sky Survey image of IC 1211
The image below is a photograph of IC 1211 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).
IC 1211 - Elliptical Galaxy morphological classification
IC 1211 - Elliptical Galaxy is classified as Elliptical (E) according to the Hubble and de Vaucouleurs galaxy morphological classification. The diagram below shows a visual representation of the position of IC 1211 - Elliptical Galaxy in the Hubble de Vaucouleurs sequence.
Celestial coordinates and finder chart of IC 1211
Celestial coordinates for the J2000 equinox of IC 1211 are provided in the following table:
The simplified sky charts below show the position of IC 1211 in the sky. The first chart has a field of view of 60° while the second one has a field of view of 10°.
Rise ans set times of IC 1211 from your location
IC 1211 - Elliptical Galaxy is circumpolar and transits at 18:54 UTC (altitude: 88.5°)