HR8355 is a multiple main-sequence star in the constellation of Capricornus.
HR8355 visual magnitude is 6.59. Because of its reltive faintness, HR8355 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 HR8355:
Celestial coordinates and finder chart of HR8355
HR8355 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 HR8355 are provided in the following table:
The simplified sky map below shows the position of HR8355 in the sky:
Visibility of HR8355 from your location
Digitized Sky Survey image of HR8355
The image below is a photograph of HR8355 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 HR8355 is 0.012 arcsec per year in Right Ascension and -0.004 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR8355 from the Sun and relative movement
HR8355 is distant 1,436.12 light years from the Sun and it is moving towards the Sun at the speed of 11 kilometers per second.
Spectral properties of HR8355
HR8355 belongs to spectral class B9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR8355 is situated in the Hertzsprung–Russell diagram.
HR8355 star system properties
HR8355 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR8355 double sysyem: