HR1385 is a main-sequence star in the constellation of Taurus.
HR1385 visual magnitude is 5.98. Because of its reltive faintness, HR1385 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 HR1385:
Celestial coordinates and finder chart of HR1385
HR1385 is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR1385 are provided in the following table:
The simplified sky map below shows the position of HR1385 in the sky:
Visibility of HR1385 from your location
Digitized Sky Survey image of HR1385
The image below is a photograph of HR1385 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 HR1385 is 0.105 arcsec per year in Right Ascension and -0.044 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR1385 from the Sun and relative movement
HR1385 is distant 159.80 light years from the Sun and it is moving far from the Sun at the speed of 37 kilometers per second.
Spectral properties of HR1385
HR1385 belongs to spectral class F4 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1385 is situated in the Hertzsprung–Russell diagram.