Azmidi - ξ Puppis (xi Puppis)
Azmidi, also designated as ξ Puppis (xi Puppis), is a double supergiant star in the constellation of Puppis.
Azmidi visual magnitude is 3.34. Because of its moderate brightness, Azmidi should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about Azmidi:
Celestial coordinates and finder chart of Azmidi
Azmidi is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of Azmidi are provided in the following table:
The simplified sky map below shows the position of Azmidi in the sky:
Visibility of Azmidi from your location
Location: Greenwich, United Kingdom [change]
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Today's Azmidi - ξ Puppis (xi Puppis) rise, transit and set times from Greenwich, United Kingdom [change] are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of Azmidi
The image below is a photograph of Azmidi 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 Azmidi is -0.003 arcsec per year in Right Ascension and -0.002 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of Azmidi from the Sun and relative movement
Azmidi is distant 1,347.11 light years from the Sun and it is moving far from the Sun at the speed of 3 kilometers per second.
Spectral properties of Azmidi
Azmidi belongs to spectral class G6 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where Azmidi is situated in the Hertzsprung–Russell diagram.
Azmidi star system properties
Azmidi 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 Azmidi double sysyem: