HR3267
HR3267 is a double hypergiant star in the constellation of Puppis.
HR3267 visual magnitude is 6.7. Because of its reltive faintness, HR3267 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 HR3267:
HR3267 is below the horizon from Greenwich, United Kingdom .
Altitude: -75.5°
Azimuth: 345.7°
Direction: North-North-West
Celestial coordinates and finder chart of HR3267
HR3267 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 HR3267 are provided in the following table:
The simplified sky map below shows the position of HR3267 in the sky:

Visibility of HR3267 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's HR3267 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 HR3267
The image below is a photograph of HR3267 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 HR3267 is -0.022 arcsec per year in Right Ascension and 0.019 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR3267 from the Sun and relative movement
HR3267 is distant 1,336.07 light years from the Sun and it is moving far from the Sun at the speed of 17 kilometers per second.
Spectral properties of HR3267
HR3267 belongs to spectral class A0 and has a luminosity class of IV corresponding to a hypergiant star.
The red dot in the diagram below shows where HR3267 is situated in the HertzsprungāRussell diagram.

HR3267 star system properties
HR3267 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 HR3267 double sysyem: