HR5621

HR5621 is a bright giant star in the constellation of Triangulum Australe.

HR5621 visual magnitude is 5.76. Because of its reltive faintness, HR5621 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 HR5621:

Celestial coordinates and finder chart of HR5621

HR5621 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 HR5621 are provided in the following table:

The simplified sky map below shows the position of HR5621 in the sky:

Visibility of HR5621 from your location

HR5621 is currently not visible from Greenwich, United Kingdom [change]

Digitized Sky Survey image of HR5621

The image below is a photograph of HR5621 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 HR5621 is -0.005 arcsec per year in Right Ascension and -0.001 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.

Distance of HR5621 from the Sun and relative movement

HR5621 is distant 6,037.04 light years from the Sun and it is moving far from the Sun at the speed of 9 kilometers per second.

Spectral properties of HR5621

HR5621 belongs to spectral class F6 and has a luminosity class of II corresponding to a bright giant star.

The red dot in the diagram below shows where HR5621 is situated in the Hertzsprung–Russell diagram.

Alternative designations of HR5621