θ Volantis (theta Volantis)
θ Volantis is a multiple hypergiant star in the constellation of Volans.
θ Volantis visual magnitude is 5.2. Because of its reltive faintness, θ Volantis 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 θ Volantis:
Celestial coordinates and finder chart of θ Volantis
θ Volantis is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of θ Volantis are provided in the following table:
The simplified sky map below shows the position of θ Volantis in the sky:
Visibility of θ Volantis from your location
θ Volantis (theta Volantis) is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of θ Volantis
The image below is a photograph of θ Volantis 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 θ Volantis is 0.018 arcsec per year in Right Ascension and -0.04 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of θ Volantis from the Sun and relative movement
θ Volantis is distant 239.00 light years from the Sun and it is moving far from the Sun at the speed of 13 kilometers per second.
Spectral properties of θ Volantis
θ Volantis belongs to spectral class A0 and has a luminosity class of V corresponding to a hypergiant star.
The red dot in the diagram below shows where θ Volantis is situated in the Hertzsprung–Russell diagram.
θ Volantis star system properties
θ Volantis is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the θ Volantis double sysyem: