HR1357

HR1357 is a variable and double star in the constellation of Reticulum.

HR1357 visual magnitude is 6.37. Because of its reltive faintness, HR1357 should be visible only from locations with dark skies, while it is not visible at all from skies affected by light pollution.

The proper motion of HR1357 is 0.041 arcsec per year in Right Ascension and 0.019 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Key facts about HR1357

Celestial coordinates and finder chart of HR1357

HR1357 is situated south of the celestial equator, as such, it is more easily visible from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR1357 are provided in the following table:

The simplified sky map below shows the position of HR1357 in the sky:

Visibility of HR1357 from your location

HR1357 is currently not visible from Greenwich, United Kingdom

Distance of HR1357 from the Sun and relative movement

HR1357 is distant 387.63 light years from the Sun and it is moving far from the Sun at the speed of 22 kilometers per second.

Spectral properties of HR1357

HR1357 belongs to spectral class A HR1357 is also a EuCrSr chemically peculiar star.

The red dot in the diagram below shows where HR1357 is situated in the Hertzsprung–Russell diagram.

HR1357 star system properties

HR1357 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 HR1357 double sysyem:

Alternative designations of HR1357