HR3219 is a multiple bright giant star in the constellation of Puppis.
HR3219 visual magnitude is 6.44. Because of its reltive faintness, HR3219 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 HR3219:
Celestial coordinates and finder chart of HR3219
HR3219 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 HR3219 are provided in the following table:
The simplified sky map below shows the position of HR3219 in the sky:
Visibility of HR3219 from your location
Today's HR3219 rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of HR3219
The image below is a photograph of HR3219 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 HR3219 is -0.012 arcsec per year in Right Ascension and 0.003 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR3219 from the Sun and relative movement
HR3219 is distant 2,451.13 light years from the Sun and it is moving far from the Sun at the speed of 39 kilometers per second.
Spectral properties of HR3219
HR3219 belongs to spectral class O9 and has a luminosity class of II corresponding to a bright giant star.
The red dot in the diagram below shows where HR3219 is situated in the Hertzsprung–Russell diagram.
HR3219 star system properties
HR3219 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 HR3219 double sysyem: