HR1687 is a main-sequence star in the constellation of Orion.
HR1687 visual magnitude is 5.9. Because of its reltive faintness, HR1687 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 HR1687:
Celestial coordinates and finder chart of HR1687
HR1687 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 HR1687 are provided in the following table:
The simplified sky map below shows the position of HR1687 in the sky:
Visibility of HR1687 from your location
Digitized Sky Survey image of HR1687
The image below is a photograph of HR1687 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 HR1687 is 0.079 arcsec per year in Right Ascension and 0.001 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1687 from the Sun and relative movement
HR1687 is distant 125.19 light years from the Sun and it is moving far from the Sun at the speed of 31 kilometers per second.
Spectral properties of HR1687
HR1687 belongs to spectral class F5 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1687 is situated in the Hertzsprung–Russell diagram.