HR2149 is a main-sequence star in the constellation of Columba.
HR2149 visual magnitude is 5.65. Because of its reltive faintness, HR2149 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 HR2149:
Celestial coordinates and finder chart of HR2149
HR2149 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR2149 are provided in the following table:
The simplified sky map below shows the position of HR2149 in the sky:
Visibility of HR2149 from your location
Digitized Sky Survey image of HR2149
The image below is a photograph of HR2149 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 HR2149 is -0.015 arcsec per year in Right Ascension and 0.119 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR2149 from the Sun and relative movement
HR2149 is distant 1,083.06 light years from the Sun and it is moving far from the Sun at the speed of 93 kilometers per second.
Spectral properties of HR2149
HR2149 belongs to spectral class B2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2149 is situated in the Hertzsprung–Russell diagram.