HR1785 is a main-sequence star in the constellation of Lepus.
HR1785 visual magnitude is 6.49. Because of its reltive faintness, HR1785 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 HR1785:
Celestial coordinates and finder chart of HR1785
HR1785 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR1785 are provided in the following table:
The simplified sky map below shows the position of HR1785 in the sky:
Visibility of HR1785 from your location
Digitized Sky Survey image of HR1785
The image below is a photograph of HR1785 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 HR1785 is 0.029 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 HR1785 from the Sun and relative movement
HR1785 is distant 170.86 light years from the Sun and it is moving far from the Sun at the speed of 51 kilometers per second.
Spectral properties of HR1785
HR1785 belongs to spectral class F6 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1785 is situated in the Hertzsprung–Russell diagram.