HR1950 is a main-sequence star in the constellation of Orion.
HR1950 visual magnitude is 6.22. Because of its reltive faintness, HR1950 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 HR1950:
Celestial coordinates and finder chart of HR1950
HR1950 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 HR1950 are provided in the following table:
The simplified sky map below shows the position of HR1950 in the sky:
Visibility of HR1950 from your location
Digitized Sky Survey image of HR1950
The image below is a photograph of HR1950 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 HR1950 is 0.008 arcsec per year in Right Ascension and 0.01 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1950 from the Sun and relative movement
HR1950 is distant 1,680.41 light years from the Sun and it is moving far from the Sun at the speed of 29 kilometers per second.
Spectral properties of HR1950
HR1950 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 HR1950 is situated in the Hertzsprung–Russell diagram.