HR3194 is a double main-sequence star in the constellation of Puppis.
HR3194 visual magnitude is 5.68. Because of its reltive faintness, HR3194 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 HR3194:
Celestial coordinates and finder chart of HR3194
HR3194 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 HR3194 are provided in the following table:
The simplified sky map below shows the position of HR3194 in the sky:
Visibility of HR3194 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Today's HR3194 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 HR3194
The image below is a photograph of HR3194 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 HR3194 is -0.017 arcsec per year in Right Ascension and -0.007 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR3194 from the Sun and relative movement
HR3194 is distant 920.90 light years from the Sun and it is moving far from the Sun at the speed of 33 kilometers per second.
Spectral properties of HR3194
HR3194 belongs to spectral class B2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR3194 is situated in the Hertzsprung–Russell diagram.
HR3194 star system properties
HR3194 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 HR3194 double sysyem: