HR449 is a main-sequence star in the constellation of Cassiopeia.
HR449 visual magnitude is 6.58. Because of its reltive faintness, HR449 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 HR449:
Celestial coordinates and finder chart of HR449
HR449 is situated close to the northern celestial pole and, as such, it is visible for most part of the year from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR449 are provided in the following table:
The simplified sky map below shows the position of HR449 in the sky:
Visibility of HR449 from your location
HR449 is circumpolar and transits at 20:24 UTC (altitude: 67.2°)
Digitized Sky Survey image of HR449
The image below is a photograph of HR449 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 HR449 is 0.027 arcsec per year in Right Ascension and -0.009 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR449 from the Sun and relative movement
HR449 is distant 956.01 light years from the Sun and it is moving towards the Sun at the speed of 8 kilometers per second.
Spectral properties of HR449
HR449 belongs to spectral class B9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR449 is situated in the Hertzsprung–Russell diagram.