HR6007 is a main-sequence star in the constellation of Scorpius.
HR6007 visual magnitude is 5.54. Because of its reltive faintness, HR6007 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 HR6007:
Celestial coordinates and finder chart of HR6007
HR6007 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 HR6007 are provided in the following table:
The simplified sky map below shows the position of HR6007 in the sky:
Visibility of HR6007 from your location
Digitized Sky Survey image of HR6007
The image below is a photograph of HR6007 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 HR6007 is -0.023 arcsec per year in Right Ascension and -0.042 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6007 from the Sun and relative movement
HR6007 is distant 432.93 light years from the Sun and it is moving towards the Sun at the speed of 21 kilometers per second.
Spectral properties of HR6007
HR6007 belongs to spectral class B8 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6007 is situated in the Hertzsprung–Russell diagram.