HR4678 is a double main-sequence star in the constellation of Virgo.
HR4678 visual magnitude is 6.54. Because of its reltive faintness, HR4678 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 HR4678:
Celestial coordinates and finder chart of HR4678
HR4678 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 HR4678 are provided in the following table:
The simplified sky map below shows the position of HR4678 in the sky:
Visibility of HR4678 from your location
Digitized Sky Survey image of HR4678
The image below is a photograph of HR4678 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 HR4678 is -0.013 arcsec per year in Right Ascension and 0.024 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR4678 from the Sun and relative movement
HR4678 is distant 201.23 light years from the Sun and it is moving towards the Sun at the speed of 1 kilometers per second.
Spectral properties of HR4678
HR4678 belongs to spectral class F2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR4678 is situated in the Hertzsprung–Russell diagram.
HR4678 star system properties
HR4678 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR4678 double sysyem: