HR1932 is a variable and multiple main-sequence star in the constellation of Orion.
HR1932 visual magnitude is 6.65. Because of its reltive faintness, HR1932 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 HR1932:
Celestial coordinates and finder chart of HR1932
HR1932 is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR1932 are provided in the following table:
The simplified sky map below shows the position of HR1932 in the sky:
Visibility of HR1932 from your location
Digitized Sky Survey image of HR1932
The image below is a photograph of HR1932 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 HR1932 is -0.018 arcsec per year in Right Ascension and 0.012 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Spectral properties of HR1932
HR1932 belongs to spectral class B2 and has a luminosity class of V corresponding to a main-sequence star.
HR1932 star system properties
HR1932 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR1932 double sysyem: