β Pyxidis (beta Pyxidis)

β Pyxidis is a double supergiant star in the constellation of Pyxis.

β Pyxidis visual magnitude is 3.97. Because of its moderate brightness, β Pyxidis should be easily visible from locations with dark skies, while it can be barely visible, or not visible at all, from skies affected by light pollution.

The proper motion of β Pyxidis is 0.012 arcsec per year in Right Ascension and -0.022 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Key facts about β Pyxidis

Celestial coordinates and finder chart of β Pyxidis

β Pyxidis 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 β Pyxidis are provided in the following table:

The simplified sky map below shows the position of β Pyxidis in the sky:

Visibility of β Pyxidis from your location

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

Distance of β Pyxidis from the Sun and relative movement

β Pyxidis is distant 388.10 light years from the Sun and it is moving towards the Sun at the speed of 13 kilometers per second.

Spectral properties of β Pyxidis

β Pyxidis belongs to spectral class G7 and has a luminosity class of I corresponding to a supergiant star.

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

β Pyxidis star system properties

β Pyxidis 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 β Pyxidis double sysyem:

Alternative designations of β Pyxidis