HR4085

HR4085 is a multiple main-sequence star in the constellation of Sextans.

HR4085 visual magnitude is 6.32. Because of its reltive faintness, HR4085 should be visible only from locations with dark skies, while it is not visible at all from skies affected by light pollution.

The proper motion of HR4085 is 0.037 arcsec per year in Right Ascension and -0.023 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Key facts about HR4085

Celestial coordinates and finder chart of HR4085

HR4085 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 HR4085 are provided in the following table:

The simplified sky map below shows the position of HR4085 in the sky:

Visibility of HR4085 from your location

Today's HR4085 rise, transit and set times from Greenwich, United Kingdom edit_location_alt are the following (all times relative to the local timezone Europe/London):

Distance of HR4085 from the Sun and relative movement

HR4085 is distant 327.64 light years from the Sun and it is moving towards the Sun at the speed of 14 kilometers per second.

Spectral properties of HR4085

HR4085 belongs to spectral class G9 and has a luminosity class of V corresponding to a main-sequence star.

The red dot in the diagram below shows where HR4085 is situated in the Hertzsprung–Russell diagram.

HR4085 star system properties

HR4085 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR4085 double sysyem:

Alternative designations of HR4085