HR7190

HR7190 is a multiple hypergiant star in the constellation of Telescopium.

HR7190 visual magnitude is 5.93. Because of its reltive faintness, HR7190 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 HR7190:

Celestial coordinates and finder chart of HR7190

HR7190 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 HR7190 are provided in the following table:

The simplified sky map below shows the position of HR7190 in the sky:

Visibility of HR7190 from your location

HR7190 is currently not visible from Greenwich, United Kingdom [change]

Digitized Sky Survey image of HR7190

The image below is a photograph of HR7190 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 HR7190 is 0.028 arcsec per year in Right Ascension and -0.146 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.

Distance of HR7190 from the Sun and relative movement

HR7190 is distant 291.85 light years from the Sun and it is moving towards the Sun at the speed of 61 kilometers per second.

Spectral properties of HR7190

HR7190 belongs to spectral class K0 and has a luminosity class of III corresponding to a hypergiant star.

The red dot in the diagram below shows where HR7190 is situated in the Hertzsprung–Russell diagram.

HR7190 star system properties

HR7190 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 HR7190 double sysyem:

Alternative designations of HR7190