HR672 is a hypergiant star in the constellation of Cetus.
HR672 visual magnitude is 5.58. Because of its reltive faintness, HR672 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 HR672:
Celestial coordinates and finder chart of HR672
HR672 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 HR672 are provided in the following table:
The simplified sky map below shows the position of HR672 in the sky:
Visibility of HR672 from your location
Today's HR672 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 HR672
The image below is a photograph of HR672 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 HR672 is 0.368 arcsec per year in Right Ascension and 0.369 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR672 from the Sun and relative movement
HR672 is distant 81.42 light years from the Sun and it is moving far from the Sun at the speed of 27 kilometers per second.
Spectral properties of HR672
HR672 belongs to spectral class G0 and has a luminosity class of IV corresponding to a hypergiant star.
The red dot in the diagram below shows where HR672 is situated in the Hertzsprung–Russell diagram.