HR1911 is a variable and double main-sequence star in the constellation of Orion.
HR1911 visual magnitude is 5.72. Because of its reltive faintness, HR1911 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 HR1911:
Celestial coordinates and finder chart of HR1911
HR1911 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 HR1911 are provided in the following table:
The simplified sky map below shows the position of HR1911 in the sky:
Visibility of HR1911 from your location
Digitized Sky Survey image of HR1911
The image below is a photograph of HR1911 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 HR1911 is -0.005 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.
Distance of HR1911 from the Sun and relative movement
HR1911 is distant 1,917.65 light years from the Sun and it is moving far from the Sun at the speed of 28 kilometers per second.
Spectral properties of HR1911
HR1911 belongs to spectral class B1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1911 is situated in the Hertzsprung–Russell diagram.
HR1911 star system properties
HR1911 is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the HR1911 double sysyem: