HR9075 is a multiple hypergiant star in the constellation of Andromeda.
HR9075 visual magnitude is 6.58. Because of its reltive faintness, HR9075 should be visible only from locations with dark skyes, while it is not visible at all from skyes affected by light pollution.
The table below summarizes the key facts about HR9075:
Celestial coordinates and finder chart of HR9075
HR9075 is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR9075 are provided in the following table:
The simplified sky map below shows the position of HR9075 in the sky:
Visibility of HR9075 from your location
Digitized Sky Survey image of HR9075
The image below is a photograph of HR9075 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). The proper motion of HR9075 is -0.06 arcsec per year in Right Ascension and -0.08 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Spectral properties of HR9075
HR9075 belongs to spectral class G0 and has a luminosity class of V corresponding to a hypergiant star.
HR9075 star system properties
HR9075 is a visual double star which can be observed with the help of medium or large telescopes. The table below shows key information about the HR9075 double sysyem: