HR176 is a main-sequence star in the constellation of Tucana.
HR176 visual magnitude is 5.89. Because of its reltive faintness, HR176 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 HR176:
Celestial coordinates and finder chart of HR176
HR176 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR176 are provided in the following table:
The simplified sky map below shows the position of HR176 in the sky:
Visibility of HR176 from your location
HR176 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR176
The image below is a photograph of HR176 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 HR176 is 0.889 arcsec per year in Right Ascension and 0.448 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR176 from the Sun and relative movement
HR176 is distant 83.04 light years from the Sun and it is moving far from the Sun at the speed of 2 kilometers per second.
Spectral properties of HR176
HR176 belongs to spectral class G1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR176 is situated in the Hertzsprung–Russell diagram.