HR241 is a main-sequence star in the constellation of Cassiopeia.
HR241 visual magnitude is 6.21. Because of its reltive faintness, HR241 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 HR241:
Celestial coordinates and finder chart of HR241
HR241 is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR241 are provided in the following table:
The simplified sky map below shows the position of HR241 in the sky:
Visibility of HR241 from your location
HR241 is circumpolar and transits at 15:41 UTC (altitude: 89.9°)
Digitized Sky Survey image of HR241
The image below is a photograph of HR241 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 HR241 is -0.01 arcsec per year in Right Ascension and -0.019 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR241 from the Sun and relative movement
HR241 is distant 1,147.89 light years from the Sun and it is moving towards the Sun at the speed of 14 kilometers per second.
Spectral properties of HR241
HR241 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 HR241 is situated in the Hertzsprung–Russell diagram.