HR7000 is a sub-giant star in the constellation of Serpens.
HR7000 visual magnitude is 6.66. Because of its reltive faintness, HR7000 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 HR7000:
Celestial coordinates and finder chart of HR7000
HR7000 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 HR7000 are provided in the following table:
The simplified sky map below shows the position of HR7000 in the sky:
Visibility of HR7000 from your location
Digitized Sky Survey image of HR7000
The image below is a photograph of HR7000 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 HR7000 is -0.027 arcsec per year in Right Ascension and -0.012 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR7000 from the Sun and relative movement
HR7000 is distant 335.74 light years from the Sun and it is moving towards the Sun at the speed of 25 kilometers per second.
Spectral properties of HR7000
HR7000 belongs to spectral class F1 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR7000 is situated in the Hertzsprung–Russell diagram.