HR6361 is a double main-sequence star in the constellation of Ophiuchus.
HR6361 visual magnitude is 6.38. Because of its reltive faintness, HR6361 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 HR6361:
Celestial coordinates and finder chart of HR6361
HR6361 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 HR6361 are provided in the following table:
The simplified sky map below shows the position of HR6361 in the sky:
Visibility of HR6361 from your location
Digitized Sky Survey image of HR6361
The image below is a photograph of HR6361 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 HR6361 is 0.033 arcsec per year in Right Ascension and -0.036 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6361 from the Sun and relative movement
HR6361 is distant 286.47 light years from the Sun and it is moving far from the Sun at the speed of 7 kilometers per second.
Spectral properties of HR6361
HR6361 belongs to spectral class A9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6361 is situated in the Hertzsprung–Russell diagram.
HR6361 star system properties
HR6361 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR6361 double sysyem: