HR3400 is a sub-giant star in the constellation of Ursa Major.
HR3400 visual magnitude is 5.66. Because of its reltive faintness, HR3400 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 HR3400:
Celestial coordinates and finder chart of HR3400
HR3400 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 HR3400 are provided in the following table:
The simplified sky map below shows the position of HR3400 in the sky:
Visibility of HR3400 from your location
HR3400 is circumpolar and transits at 04:18 UTC (altitude: 88.1°)
Digitized Sky Survey image of HR3400
The image below is a photograph of HR3400 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 HR3400 is -0.078 arcsec per year in Right Ascension and -0.017 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR3400 from the Sun and relative movement
HR3400 is distant 240.59 light years from the Sun and it is moving towards the Sun at the speed of 43 kilometers per second.
Spectral properties of HR3400
HR3400 belongs to spectral class G8 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR3400 is situated in the Hertzsprung–Russell diagram.