μ Pictoris (mu Pictoris)

μ Pictoris is a double main-sequence star in the constellation of Pictor.

μ Pictoris visual magnitude is 5.7. Because of its reltive faintness, μ Pictoris 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 μ Pictoris is 0.004 arcsec per year in Right Ascension and -0.011 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Key facts about μ Pictoris

Celestial coordinates and finder chart of μ Pictoris

μ Pictoris is situated south of the celestial equator, as such, it is more easily visible from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of μ Pictoris are provided in the following table:

The simplified sky map below shows the position of μ Pictoris in the sky:

Visibility of μ Pictoris from your location

μ Pictoris (mu Pictoris) is currently not visible from Greenwich, United Kingdom edit_location_alt

Distance of μ Pictoris from the Sun and relative movement

μ Pictoris is distant 724.44 light years from the Sun and it is moving far from the Sun at the speed of 2 kilometers per second.

Spectral properties of μ Pictoris

μ Pictoris 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 μ Pictoris is situated in the Hertzsprung–Russell diagram.

μ Pictoris star system properties

μ Pictoris is a visual double star which can be observed with the help of medium or large telescopes. The table below shows key information about the μ Pictoris double sysyem:

Alternative designations of μ Pictoris