HR4435 is a sub-giant star in the constellation of Ursa Major.
HR4435 visual magnitude is 6.42. Because of its reltive faintness, HR4435 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 HR4435:
Celestial coordinates and finder chart of HR4435
HR4435 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 HR4435 are provided in the following table:
The simplified sky map below shows the position of HR4435 in the sky:
Visibility of HR4435 from your location
HR4435 is circumpolar and transits at 11:31 UTC (altitude: 86.4°)
Digitized Sky Survey image of HR4435
The image below is a photograph of HR4435 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 HR4435 is -0.229 arcsec per year in Right Ascension and -0.07 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR4435 from the Sun and relative movement
HR4435 is distant 328.30 light years from the Sun and it is moving far from the Sun at the speed of 38 kilometers per second.
Spectral properties of HR4435
HR4435 belongs to spectral class G9 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR4435 is situated in the Hertzsprung–Russell diagram.