HR1737 is a variable subgiant star in the constellation of Lepus.
HR1737 visual magnitude is 5.5. Because of its reltive faintness, HR1737 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 HR1737:
Celestial coordinates and finder chart of HR1737
HR1737 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 HR1737 are provided in the following table:
The simplified sky map below shows the position of HR1737 in the sky:
Visibility of HR1737 from your location
Digitized Sky Survey image of HR1737
The image below is a photograph of HR1737 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 HR1737 is -0.012 arcsec per year in Right Ascension and -0.046 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1737 from the Sun and relative movement
HR1737 is distant 157.56 light years from the Sun and it is moving far from the Sun at the speed of 75 kilometers per second.
Spectral properties of HR1737
HR1737 belongs to spectral class G9
The red dot in the diagram below shows where HR1737 is situated in the Hertzsprung–Russell diagram.