HR8607 is a main-sequence star in the constellation of Lacerta.
HR8607 visual magnitude is 6.38. Because of its reltive faintness, HR8607 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 HR8607:
Celestial coordinates and finder chart of HR8607
HR8607 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 HR8607 are provided in the following table:
The simplified sky map below shows the position of HR8607 in the sky:
Visibility of HR8607 from your location
HR8607 is circumpolar and transits at 18:08 UTC (altitude: 85.4°)
Digitized Sky Survey image of HR8607
The image below is a photograph of HR8607 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 HR8607 is -0.003 arcsec per year in Right Ascension and -0.019 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR8607 from the Sun and relative movement
HR8607 is distant 351.29 light years from the Sun and it is moving towards the Sun at the speed of 2 kilometers per second.
Spectral properties of HR8607
HR8607 belongs to spectral class A3 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR8607 is situated in the Hertzsprung–Russell diagram.