HR3327 is a variable and multiple main-sequence star in the constellation of Puppis.
HR3327 visual magnitude is 6.53. Because of its reltive faintness, HR3327 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 HR3327:
Celestial coordinates and finder chart of HR3327
HR3327 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 HR3327 are provided in the following table:
The simplified sky map below shows the position of HR3327 in the sky:
Visibility of HR3327 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
HR3327 is currently not visible from Greenwich, United Kingdom
Digitized Sky Survey image of HR3327
The image below is a photograph of HR3327 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 HR3327 is -0.017 arcsec per year in Right Ascension and -0.008 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR3327 from the Sun and relative movement
HR3327 is distant 612.78 light years from the Sun and it is moving far from the Sun at the speed of 28 kilometers per second.
Spectral properties of HR3327
HR3327 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 HR3327 is situated in the Hertzsprung–Russell diagram.
HR3327 star system properties
HR3327 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 HR3327 double sysyem: