HR7411

HR7411 is a star in the constellation of Telescopium.

HR7411 visual magnitude is 5.75. Because of its reltive faintness, HR7411 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 HR7411:

Celestial coordinates and finder chart of HR7411

HR7411 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 HR7411 are provided in the following table:

The simplified sky map below shows the position of HR7411 in the sky:

Visibility of HR7411 from your location

HR7411 is currently not visible from Greenwich, United Kingdom [change]

Digitized Sky Survey image of HR7411

The image below is a photograph of HR7411 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 HR7411 is 0.029 arcsec per year in Right Ascension and -0.013 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR7411 from the Sun and relative movement

HR7411 is distant 404.97 light years from the Sun and it is moving far from the Sun at the speed of 14 kilometers per second.

Spectral properties of HR7411

HR7411 belongs to spectral class F HR7411 is also a so called metallic star.

The red dot in the diagram below shows where HR7411 is situated in the Hertzsprung–Russell diagram.

Alternative designations of HR7411