HR2050 is a double main-sequence star in the constellation of Orion.
HR2050 visual magnitude is 6.59. Because of its reltive faintness, HR2050 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 HR2050:
Celestial coordinates and finder chart of HR2050
HR2050 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 HR2050 are provided in the following table:
The simplified sky map below shows the position of HR2050 in the sky:
Visibility of HR2050 from your location
Digitized Sky Survey image of HR2050
The image below is a photograph of HR2050 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 HR2050 is 0.008 arcsec per year in Right Ascension and -0.068 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2050 from the Sun and relative movement
HR2050 is distant 304.96 light years from the Sun and it is moving far from the Sun at the speed of 28 kilometers per second.
Spectral properties of HR2050
HR2050 belongs to spectral class A2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2050 is situated in the Hertzsprung–Russell diagram.
HR2050 star system properties
HR2050 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 HR2050 double sysyem: